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<article article-type="research-article" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:oasis="http://www.niso.org/standards/z39-96/ns/oasis-exchange/table"><front><journal-meta><journal-id journal-id-type="publisher-id">PRD</journal-id><journal-id journal-id-type="coden">PRVDAQ</journal-id><journal-title-group><journal-title>Physical Review D</journal-title><abbrev-journal-title>Phys. Rev. D</abbrev-journal-title></journal-title-group><issn pub-type="ppub">2470-0010</issn><issn pub-type="epub">2470-0029</issn><publisher><publisher-name>American Physical Society</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.1103/7njb-6v24</article-id><article-categories><subj-group subj-group-type="toc-major"><subject>ARTICLES</subject></subj-group><subj-group subj-group-type="toc-minor"><subject>String theory, quantum gravity, gauge/gravity duality</subject></subj-group></article-categories><title-group><article-title>Scaling functions in the soft-wall AdS/QCD models</article-title><alt-title alt-title-type="running-title">SCALING FUNCTIONS IN THE SOFT-WALL ADS/QCD MODELS</alt-title><alt-title alt-title-type="running-author">ZHANG, LI, YU, LI, AND WANG</alt-title></title-group><contrib-group><contrib contrib-type="author"><contrib-id authenticated="true" contrib-id-type="orcid">https://orcid.org/0009-0004-8528-5849</contrib-id><name><surname>Zhang</surname><given-names>Zhongzheng</given-names></name><xref ref-type="aff" rid="a1"><sup>1</sup></xref></contrib><contrib contrib-type="author"><contrib-id authenticated="true" contrib-id-type="orcid">https://orcid.org/0000-0002-1436-6893</contrib-id><name><surname>Li</surname><given-names>Danning</given-names></name><xref ref-type="aff" rid="a1"><sup>1</sup></xref><xref ref-type="author-notes" rid="n1"><sup>,*</sup></xref></contrib><contrib contrib-type="author"><name><surname>Yu</surname><given-names>Lang</given-names></name><xref ref-type="aff" rid="a2"><sup>2</sup></xref><xref ref-type="author-notes" rid="n2"><sup>,†</sup></xref></contrib><contrib contrib-type="author"><contrib-id authenticated="true" contrib-id-type="orcid">https://orcid.org/0000-0001-9232-0228</contrib-id><name><surname>Li</surname><given-names>Zhibin</given-names></name><xref ref-type="aff" rid="a3"><sup>3</sup></xref></contrib><contrib contrib-type="author"><contrib-id authenticated="true" contrib-id-type="orcid">https://orcid.org/0000-0002-0401-8510</contrib-id><name><surname>Wang</surname><given-names>Xinyang</given-names></name><xref ref-type="aff" rid="a4"><sup>4</sup></xref></contrib><aff id="a1"><label><sup>1</sup></label>Department of Physics and Siyuan Laboratory, <institution-wrap><institution>Jinan University</institution><institution-id institution-id-type="ror">https://ror.org/02xe5ns62</institution-id></institution-wrap>, Guangzhou 510632, China</aff><aff id="a2"><label><sup>2</sup></label>College of Physics, <institution-wrap><institution>Jilin University</institution><institution-id institution-id-type="ror">https://ror.org/00js3aw79</institution-id></institution-wrap>, Changchun 130012, People’s Republic of China</aff><aff id="a3"><label><sup>3</sup></label>Institute for Astrophysics, School of Physics, <institution-wrap><institution>Zhengzhou University</institution><institution-id institution-id-type="ror">https://ror.org/04ypx8c21</institution-id></institution-wrap>, Zhengzhou 450001, China</aff><aff id="a4"><label><sup>4</sup></label>Fundamental Physics Center, School of Mechanics and Physics, <institution-wrap><institution>Anhui University of Science and Technology</institution><institution-id institution-id-type="ror">https://ror.org/00q9atg80</institution-id></institution-wrap>, Huainan, Anhui 232001, China</aff></contrib-group><author-notes><fn id="n1"><label><sup>*</sup></label><p>Contact author: <email>lidanning@jnu.edu.cn</email></p></fn><fn id="n2"><label><sup>†</sup></label><p>Contact author: <email>yulang@jlu.edu.cn</email></p></fn></author-notes><pub-date iso-8601-date="2026-04-28" date-type="pub" publication-format="electronic"><day>28</day><month>April</month><year>2026</year></pub-date><pub-date iso-8601-date="2026-04-15" date-type="pub" publication-format="print"><day>15</day><month>April</month><year>2026</year></pub-date><volume>113</volume><issue>8</issue><elocation-id>086010</elocation-id><pub-history><event><date iso-8601-date="2025-08-06" date-type="received"><day>6</day><month>August</month><year>2025</year></date></event><event><date iso-8601-date="2026-03-27" date-type="accepted"><day>27</day><month>March</month><year>2026</year></date></event></pub-history><permissions><copyright-statement>Published by the American Physical Society</copyright-statement><copyright-year>2026</copyright-year><copyright-holder>authors</copyright-holder><license license-type="creative-commons" xlink:href="https://creativecommons.org/licenses/by/4.0/"><license-p content-type="usage-statement">Published by the American Physical Society under the terms of the <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution 4.0 International</ext-link> license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP<sup>3</sup>.</license-p></license></permissions><related-article ext-link-type="doi" xlink:href="10.48550/arXiv.2507.22724" related-article-type="preprint"/><abstract><p>We investigate the static scaling behavior of the chiral condensate near the two-flavor critical point within the framework of the soft-wall AdS/QCD. The scaling functions are extracted from the chiral order parameters and are found to precisely match those obtained through mean-field calculations. Additionally, it is also checked that the scaling functions are independent of the specific construction of the holographic model. Furthermore, we develop the formalism for calculating the chiral susceptibility and demonstrate that the pseudocritical temperatures obey the scaling law for moderate quark masses. It is shown that the temperature scaling could be comparable with those obtained from Dyson-Schwinger equations and lattice simulations. While the soft-wall AdS/QCD framework predicts mean-field critical exponents that are universal, the critical coefficients and the crossover dynamics are model dependent and provide quantitative constraints for phenomenological model building. These findings could help improve the effectiveness of the soft-wall AdS/QCD.</p></abstract><funding-group><award-group award-type="grant"><funding-source country="CN"><institution-wrap><institution>National Natural Science Foundation of China</institution><institution-id institution-id-type="doi" vocab="open-funder-registry" vocab-identifier="10.13039/open-funder-registry">10.13039/501100001809</institution-id></institution-wrap></funding-source><award-id>12275108</award-id><award-id>12235016</award-id></award-group></funding-group><counts><page-count count="15"/></counts></article-meta></front><body><sec id="s1"><label>I.</label><title>INTRODUCTION</title><p>Empirical and lattice-QCD studies indicate that, at nonzero temperature and baryon chemical potential, QCD undergoes two intertwined but conceptually distinct phase transitions: deconfinement, whereby color degrees of freedom become manifest over hadronic scales, and chiral-symmetry restoration characterized by the melting of the quark condensate. Clarifying the interplay between these two phenomena is essential for interpreting experimental observables in heavy-ion collisions, elucidating the equation of state of dense matter in compact stars and constraining scenarios for the evolution of the early Universe <xref ref-type="bibr" rid="c1 c2 c3 c4">[1–4]</xref>.</p><p>For physical quark masses, lattice-QCD studies establish that QCD matter undergoes a smooth analytic crossover at vanishing baryon chemical potential <xref ref-type="bibr" rid="c5 c6 c7 c8">[5–8]</xref>. In the two-flavor chiral limit, by contrast, the transition becomes a true phase transition whose order—second or first—depends on the relative hierarchy between chiral-symmetry restoration and the effective restoration of the axial <inline-formula><mml:math display="inline"><mml:mi>U</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>1</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> anomaly <xref ref-type="bibr" rid="c5">[5]</xref>. Besides its theoretical significance, mapping the QCD phase diagram in the quark-mass plane is essential for locating the critical end point (CEP), a primary objective of present heavy-ion-collision experiments; in particular, the chiral-limit transition temperature provides an upper bound for possible CEP temperatures at nonzero baryon chemical potential <xref ref-type="bibr" rid="c9">[9]</xref>. Since lattice simulations cannot be carried out directly in the exact chiral limit, analyses that exploit universal scaling functions are indispensable for extrapolating physical results to that limit.</p><p>Recent lattice-QCD results have revealed the anticipated <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>N</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> scaling behavior <xref ref-type="bibr" rid="c10 c11 c12">[10–12]</xref> of the chiral crossover. The connection based on the universal scaling equation is restricted to a finite domain referred to as the scaling window. The width of this window is still under debate. According to lattice-QCD results <xref ref-type="bibr" rid="c13 c14">[13,14]</xref>, the scaling region is located at relatively large values of the pion mass. Reference <xref ref-type="bibr" rid="c15">[15]</xref>, for example, explores the conformal window across different flavor numbers and suggests that, within the 3D <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>4</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> universality class, the physical pion mass may lie close to the critical point, with scaling behavior potentially extending into the high-temperature regime up to 300 MeV. In contrast, another lattice-QCD study <xref ref-type="bibr" rid="c16">[16]</xref> indicates that the scaling window may also extend below the physical quark mass and, based on the scaling function, provides an estimate of the transition temperature in the chiral limit. Consistently, alternative approaches such as Dyson-Schwinger equations (DSEs) <xref ref-type="bibr" rid="c9 c17 c18">[9,17,18]</xref> and the functional renormalization group (FRG) <xref ref-type="bibr" rid="c19 c20">[19,20]</xref> also demonstrate the presence of scaling behavior for quark masses below the physical point.</p><p>In the low-energy regime where QCD phase transitions take place, the strong coupling strength renders conventional perturbative techniques inadequate. Thus, it is essential to develop nonperturbative methods to explore the underlying physics. Among such methods, lattice QCD—formulated from first principles—has been recognized as a reliable tool. However, at large baryon densities, lattice QCD suffers from the notorious sign problem <xref ref-type="bibr" rid="c21">[21]</xref>, which has yet to be satisfactorily resolved. This limitation has motivated the search for alternative nonperturbative approaches.</p><p>In the 1990s, ’t Hooft proposed a preliminary form of the holographic principle <xref ref-type="bibr" rid="c22">[22]</xref>, which was subsequently integrated with string theory by Susskind <xref ref-type="bibr" rid="c23">[23]</xref>. The AdS/CFT correspondence, first conjectured by Maldacena <xref ref-type="bibr" rid="c24">[24]</xref>, has shed new light on solving strongly coupled problems in gauge field theories. In the study of QCD matter, a celebrated achievement of holographic approaches is the derivation of the universal lower bound <inline-formula><mml:math display="inline"><mml:mi>η</mml:mi><mml:mo>/</mml:mo><mml:mi>s</mml:mi><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:mn>4</mml:mn><mml:mi>π</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> for the shear viscosity to entropy density ratio, providing key insight into the nearly perfect-fluid behavior of the quark-gluon plasma from a theoretical perspective <xref ref-type="bibr" rid="c25 c26 c27">[25–27]</xref>. Employing a bottom-up strategy that prioritizes phenomenology over top-down string-theoretic origins, researchers have constructed a variety of holographic models—including light-front holographic QCD <xref ref-type="bibr" rid="c28">[28]</xref>, holographic model of QCD in the Veneziano limit <xref ref-type="bibr" rid="c29">[29]</xref>, and Einstein–Maxwell–Dilaton (EMD) setups <xref ref-type="bibr" rid="c30 c31 c32 c33 c34 c35 c36">[30–36]</xref>—to capture hadron spectra, thermodynamics, transport coefficients, and the QCD phase transition with remarkable success. From those phenomenological studies, it appears that the EMD model provides an adequate description of gluodynamics.</p><p>It has been shown that spontaneous chiral-symmetry breaking, as another key low-energy feature of QCD, can be effectively described within the hard-wall and soft-wall AdS/QCD models <xref ref-type="bibr" rid="c37 c38">[37,38]</xref>. A finite chiral condensate is dynamically generated, lifting the degeneracy between chiral partners in the hadron spectrum <xref ref-type="bibr" rid="c39 c40">[39,40]</xref>. As the temperature increases, this condensate is progressively suppressed; once it vanishes, chiral symmetry is restored and the chiral phase transition takes place <xref ref-type="bibr" rid="c41 c42">[41,42]</xref>.</p><p>The principal advantage of this model is that by elevating the four-dimensional (4D) global symmetry to a five-dimensional (5D) gauge symmetry, it naturally incorporates the conserved currents and the <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>q</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mi>q</mml:mi></mml:math></inline-formula> bilinear operator. This makes it straightforward to explore scenarios with arbitrary quark masses and finite charge densities. Studies have extended from simple two-flavor systems to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>N</mml:mi><mml:mi>f</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>2</mml:mn><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula> <xref ref-type="bibr" rid="c43 c44 c45">[43–45]</xref>, and more recently to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>N</mml:mi><mml:mi>f</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>2</mml:mn><mml:mo>+</mml:mo><mml:mn>1</mml:mn><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula> <xref ref-type="bibr" rid="c46">[46]</xref>. The phase diagram in the quark-mass plane (<inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>/</mml:mo><mml:mi>d</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:math></inline-formula>) can be summarized in a holographic version <xref ref-type="bibr" rid="c47">[47]</xref> of the so-called “Columbia plot,” which qualitatively agrees well with that obtained by combining the lattice simulations and other effective studies <xref ref-type="bibr" rid="c8 c48">[8,48]</xref>. By introducing the baryon and isospin chemical potentials <inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>B</mml:mi></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>I</mml:mi></mml:msub></mml:math></inline-formula> through the corresponding conserved currents, one can probe regimes of high baryon and isospin densities where recent studies predict the appearance of additional phases, e.g., the quarkyonic and pion-condensed phases <xref ref-type="bibr" rid="c49 c50 c51 c52">[49–52]</xref>. A magnetic field can be introduced by constructing the electromagnetic current from the baryon and isospin currents; inverse magnetic catalysis then emerges naturally, without fine-tuning of the model settings <xref ref-type="bibr" rid="c53 c54">[53,54]</xref>. Furthermore, as derived in <xref ref-type="bibr" rid="c55">[55]</xref>, the model can be reduced to a four-dimensional chiral perturbation theory. The matching of the near <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> behavior of its Goldstone modes <xref ref-type="bibr" rid="c56 c57 c58">[56–58]</xref> with those of the four-dimensional chiral perturbation theory <xref ref-type="bibr" rid="c59">[59]</xref> provides explicit evidence for this equivalence. Overall, the soft-wall model offers an excellent starting point for exploring chiral dynamics in QCD, serving in effect as a five-dimensional analog of chiral perturbation theory.</p><p>Although the above analyses have thoroughly validated the soft-wall model’s consistency and effectiveness in describing low-energy QCD, its universality has yet to be fully tested. While the critical exponents have been proved to be of mean-field level <xref ref-type="bibr" rid="c47">[47]</xref>, with <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>β</mml:mi><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>δ</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:math></inline-formula> in the two-flavor limit, the holographic investigation of mass scaling behavior of the pseudocritical temperature, as well as of the scaling function itself, remains largely undeveloped. Given that universal scaling functions enable chiral extrapolation in lattice QCD and are important for constraining holographic model building (while fitting at the physical point is valuable, it alone cannot fully validate a holographic model’s robustness), in this work, we aim to investigate the scaling behavior of the chiral phase transition temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> with respect to different quark and pion masses. We will calculate the scaling function and test the scaling window in the holographic model, which may provide further constraints for building a realistic holographic QCD model. In this work, we will focus on the two-flavor limit for simplicity.</p><p>The organization of this paper is as follows: In Sec. <xref ref-type="sec" rid="s2">II</xref>, we briefly review the soft-wall model and chiral phase transition in this model. In Sec. <xref ref-type="sec" rid="s3">III</xref>, we numerically extract the scaling functions and test the universal relations of those functions as a check of the self-consistency of the soft-wall AdS/QCD models. In Sec. <xref ref-type="sec" rid="s4">IV</xref>, we give analyses of the scaling behavior of the pseudocritical temperature. An additional constraint is given for constructing a more realistic holographic QCD model for chiral dynamics. Finally, a brief summary will be given in Sec. <xref ref-type="sec" rid="s5">V</xref>.</p></sec><sec id="s2"><label>II.</label><title>THE SOFT-WALL ADS/QCD MODEL</title><p>In this section, we provide a brief overview of the soft-wall model and introduce several modifications to explore its universal properties. As discussed above, the action of the soft-wall model is constructed by promoting the 4D global chiral symmetry <inline-formula><mml:math display="inline"><mml:mi>S</mml:mi><mml:mi>U</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>2</mml:mn><mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mi>L</mml:mi></mml:msub><mml:mo stretchy="false">⊗</mml:mo><mml:mi>S</mml:mi><mml:mi>U</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>2</mml:mn><mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mi>R</mml:mi></mml:msub></mml:math></inline-formula> to 5D gauge symmetry. Since we focus on the two-flavor limit, i.e., considering only the u and d quarks, the action of the soft-wall model is given as follows: <disp-formula id="d1"><mml:math display="block"><mml:mrow><mml:msub><mml:mrow><mml:mi>S</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn><mml:mi mathvariant="normal">D</mml:mi></mml:mrow></mml:msub><mml:mo id="d1a1">=</mml:mo><mml:mo>∫</mml:mo><mml:msup><mml:mrow><mml:mi>d</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow></mml:msup><mml:mi>x</mml:mi><mml:msqrt><mml:mrow><mml:mi>g</mml:mi></mml:mrow></mml:msqrt><mml:msup><mml:mrow><mml:mi>e</mml:mi></mml:mrow><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Φ</mml:mi></mml:mrow></mml:msup><mml:mi>Tr</mml:mi><mml:mo>{</mml:mo><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>D</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mi>X</mml:mi><mml:msup><mml:mrow><mml:mo stretchy="false">|</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>-</mml:mo><mml:msub><mml:mrow><mml:mi>V</mml:mi></mml:mrow><mml:mrow><mml:mi>X</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mo stretchy="false">|</mml:mo><mml:mi>X</mml:mi><mml:mo stretchy="false">|</mml:mo><mml:mo stretchy="false">)</mml:mo><mml:mspace linebreak="newline"/><mml:mo indentalign="id" indentshift="1em" indenttarget="d1a1">-</mml:mo><mml:mfrac><mml:mrow><mml:mn>1</mml:mn></mml:mrow><mml:mrow><mml:mn>4</mml:mn><mml:msubsup><mml:mrow><mml:mi>g</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac><mml:mo stretchy="false">(</mml:mo><mml:msubsup><mml:mrow><mml:mi>F</mml:mi></mml:mrow><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mrow><mml:mi>F</mml:mi></mml:mrow><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo stretchy="false">)</mml:mo><mml:mo>}</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math><label>(1)</label></disp-formula></p><p>In the above action, <inline-formula><mml:math display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> represents spacetime indices, <inline-formula><mml:math display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> is the determinant of the metric <inline-formula><mml:math display="inline"><mml:msub><mml:mi>g</mml:mi><mml:mrow><mml:mi>M</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> is an <inline-formula><mml:math display="inline"><mml:msub><mml:mi>N</mml:mi><mml:mi>f</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi>f</mml:mi></mml:msub></mml:math></inline-formula> matrix-valued scalar field, and <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Φ</mml:mi></mml:math></inline-formula> is the dilaton field. As in previous studies, we set the dilaton field as <disp-formula id="d2"><mml:math display="block"><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>=</mml:mo><mml:msubsup><mml:mi>μ</mml:mi><mml:mi>g</mml:mi><mml:mn>2</mml:mn></mml:msubsup><mml:msup><mml:mi>r</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mo>,</mml:mo></mml:math><label>(2)</label></disp-formula>with <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> being the holographic dimension. The 5D coupling constant <inline-formula><mml:math display="inline"><mml:msub><mml:mi>g</mml:mi><mml:mn>5</mml:mn></mml:msub></mml:math></inline-formula> can be determined as <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>g</mml:mi><mml:mn>5</mml:mn><mml:mn>2</mml:mn></mml:msubsup><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mn>12</mml:mn><mml:msup><mml:mi>π</mml:mi><mml:mn>2</mml:mn></mml:msup></mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:mfrac></mml:math></inline-formula> by matching the large-momentum expansion of the vector current <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>J</mml:mi><mml:mi>μ</mml:mi><mml:mi>a</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>q</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:msub><mml:mi>γ</mml:mi><mml:mi>μ</mml:mi></mml:msub><mml:msup><mml:mi>t</mml:mi><mml:mi>a</mml:mi></mml:msup><mml:mi>q</mml:mi></mml:math></inline-formula> correlation in AdS/QCD with that from the perturbative calculation <xref ref-type="bibr" rid="c37">[37]</xref>. The covariant derivative <inline-formula><mml:math display="inline"><mml:msub><mml:mi>D</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:math></inline-formula> and the field strength tensors <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>F</mml:mi><mml:mrow><mml:mi>M</mml:mi><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi>L</mml:mi><mml:mo>,</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:msubsup></mml:math></inline-formula> are defined as follows: <disp-formula id="d3"><mml:math display="block"><mml:mrow><mml:msub><mml:mrow><mml:mi>D</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mi>X</mml:mi><mml:mo id="d3a1">=</mml:mo><mml:msub><mml:mrow><mml:mo>∂</mml:mo></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mi>X</mml:mi><mml:mo>-</mml:mo><mml:mi>i</mml:mi><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mi>X</mml:mi><mml:mo>+</mml:mo><mml:mi>i</mml:mi><mml:mi>X</mml:mi><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mspace linebreak="newline"/><mml:msubsup><mml:mrow><mml:mi>F</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi>L</mml:mi></mml:mrow></mml:msubsup><mml:mo indentalign="id" indenttarget="d3a1">=</mml:mo><mml:msub><mml:mrow><mml:mo>∂</mml:mo></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mrow><mml:mo>∂</mml:mo></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>i</mml:mi><mml:mo stretchy="false">[</mml:mo><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">]</mml:mo><mml:mo>,</mml:mo><mml:mspace linebreak="newline"/><mml:msubsup><mml:mrow><mml:mi>F</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi>R</mml:mi></mml:mrow></mml:msubsup><mml:mo indentalign="id" indenttarget="d3a1">=</mml:mo><mml:msub><mml:mrow><mml:mo>∂</mml:mo></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mrow><mml:mo>∂</mml:mo></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>i</mml:mi><mml:mo stretchy="false">[</mml:mo><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">]</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math><label>(3)</label></disp-formula>with <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> being the 5D left- and right-handed gauge potentials, which are dual to the left- and right-handed chiral currents. <inline-formula><mml:math display="inline"><mml:msub><mml:mi>V</mml:mi><mml:mi>X</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mo stretchy="false">|</mml:mo><mml:mi>X</mml:mi><mml:mo stretchy="false">|</mml:mo><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> represents the scalar potential, which may generally include a coupling to the dilaton field. Since we consider the degenerate two-flavor case (<inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>d</mml:mi></mml:msub></mml:math></inline-formula>) only, the expectation of <inline-formula><mml:math display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> can be decomposed as <inline-formula><mml:math display="inline"><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mn>2</mml:mn></mml:mfrac><mml:mi>χ</mml:mi><mml:msub><mml:mi>I</mml:mi><mml:mn>2</mml:mn></mml:msub></mml:math></inline-formula>, with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>I</mml:mi><mml:mn>2</mml:mn></mml:msub></mml:math></inline-formula> the <inline-formula><mml:math display="inline"><mml:mn>2</mml:mn><mml:mo>×</mml:mo><mml:mn>2</mml:mn></mml:math></inline-formula> identity matrix. The factor <inline-formula><mml:math display="inline"><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:math></inline-formula> is introduced to ensure that the kinetic term in <inline-formula><mml:math display="inline"><mml:mi>χ</mml:mi></mml:math></inline-formula> is canonical. Then we denote the scalar potential in terms of <inline-formula><mml:math display="inline"><mml:mi>χ</mml:mi></mml:math></inline-formula> as <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mi>Tr</mml:mi><mml:mo stretchy="false">[</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi>X</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>X</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo stretchy="false">]</mml:mo></mml:math></inline-formula>. Since we do not consider the case with finite densities or consider the vector perturbations, the relevant part of the action reduces to <disp-formula id="d4"><mml:math display="block"><mml:mrow><mml:msub><mml:mrow><mml:mi>S</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn><mml:mi mathvariant="normal">D</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mo>∫</mml:mo><mml:msup><mml:mrow><mml:mi>d</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow></mml:msup><mml:mi>x</mml:mi><mml:msqrt><mml:mrow><mml:mi>g</mml:mi></mml:mrow></mml:msqrt><mml:msup><mml:mrow><mml:mi>e</mml:mi></mml:mrow><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Φ</mml:mi></mml:mrow></mml:msup><mml:mo>[</mml:mo><mml:mfrac><mml:mrow><mml:mn>1</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mfrac><mml:mi>χ</mml:mi><mml:msup><mml:mrow><mml:mo>′</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>-</mml:mo><mml:mi>V</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>]</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math><label>(4)</label></disp-formula></p><p>To study chiral dynamics in this model, a specific form of the background metric is necessary. In consideration of the symmetries of the four-dimensional theory at finite temperature, the metric ansatz is adopted as follows: <disp-formula id="d5"><mml:math display="block"><mml:mi>d</mml:mi><mml:msup><mml:mi>s</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mn>2</mml:mn><mml:mi>A</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mi>d</mml:mi><mml:msup><mml:mi>t</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:mi>d</mml:mi><mml:msup><mml:mi>x</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mrow><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:mfrac><mml:mi>d</mml:mi><mml:msup><mml:mi>r</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow><mml:mo>.</mml:mo></mml:math><label>(5)</label></disp-formula>A simple consideration is to take the AdS-Schwarzschild black hole solution with <disp-formula id="d6"><mml:math display="block"><mml:mi>A</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo id="d6a1">=</mml:mo><mml:mo>-</mml:mo><mml:mi>ln</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>,</mml:mo><mml:mspace linebreak="newline"/><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo indentalign="id" indenttarget="d6a1">=</mml:mo><mml:mn>1</mml:mn><mml:mo>-</mml:mo><mml:mfrac><mml:msup><mml:mi>r</mml:mi><mml:mn>4</mml:mn></mml:msup><mml:msubsup><mml:mi>r</mml:mi><mml:mi>h</mml:mi><mml:mn>4</mml:mn></mml:msubsup></mml:mfrac><mml:mo>.</mml:mo></mml:math><label>(6)</label></disp-formula>Here, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub></mml:math></inline-formula> denotes the black hole horizon, at which the blackening factor satisfies <inline-formula><mml:math display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>. This can be mapped to the temperature through the Hawking temperature defined as <disp-formula id="d7"><mml:math display="block"><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mrow><mml:mo>|</mml:mo><mml:mfrac><mml:mrow><mml:msup><mml:mi>f</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>4</mml:mn><mml:mi>π</mml:mi></mml:mrow></mml:mfrac><mml:mo>|</mml:mo></mml:mrow><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mrow><mml:mi>π</mml:mi><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mo>.</mml:mo></mml:math><label>(7)</label></disp-formula></p><p>To solve this model, one has to derive the equation of motion for <inline-formula><mml:math display="inline"><mml:mi>χ</mml:mi></mml:math></inline-formula> from the action Eq. <xref ref-type="disp-formula" rid="d4">(4)</xref>, which reads <disp-formula id="d8"><mml:math display="block"><mml:msup><mml:mi>χ</mml:mi><mml:mo>′′</mml:mo></mml:msup><mml:mo>+</mml:mo><mml:mrow><mml:mo>(</mml:mo><mml:mn>3</mml:mn><mml:msup><mml:mi>A</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>+</mml:mo><mml:mfrac><mml:msup><mml:mi>f</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mi>f</mml:mi></mml:mfrac><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow><mml:msup><mml:mi>χ</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>-</mml:mo><mml:mfrac><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mn>2</mml:mn><mml:mi>A</mml:mi></mml:mrow></mml:msup><mml:mi>f</mml:mi></mml:mfrac><mml:msub><mml:mi>V</mml:mi><mml:mrow><mml:mo>,</mml:mo><mml:mi>χ</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo>,</mml:mo></mml:math><label>(8)</label></disp-formula>with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>V</mml:mi><mml:mrow><mml:mo>,</mml:mo><mml:mi>χ</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>≡</mml:mo><mml:msub><mml:mo>∂</mml:mo><mml:mi>χ</mml:mi></mml:msub><mml:mi>V</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>. Here we have assumed that the system is in an equilibrium state, so <inline-formula><mml:math display="inline"><mml:mi>χ</mml:mi></mml:math></inline-formula> depends on <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> only. The overprime <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mtext> </mml:mtext><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> in the above equation denotes differentiation with respect to <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>.</p><p>It is not difficult to derive from the above equation the near boundary (<inline-formula><mml:math display="inline"><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>) and near horizon (<inline-formula><mml:math display="inline"><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub></mml:math></inline-formula>) expansion of <inline-formula><mml:math display="inline"><mml:mi>χ</mml:mi></mml:math></inline-formula> as <disp-formula-group id="d9"><label>(9)</label><disp-formula id="d9a"><mml:math display="block"><mml:mi>χ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mi>ζ</mml:mi><mml:mi>r</mml:mi><mml:mo>+</mml:mo><mml:mo>⋯</mml:mo><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn>3</mml:mn></mml:msup><mml:mi>σ</mml:mi></mml:mrow><mml:mi>ζ</mml:mi></mml:mfrac><mml:mo>+</mml:mo><mml:mi mathvariant="script">O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msup><mml:mi>r</mml:mi><mml:mn>4</mml:mn></mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mo>,</mml:mo></mml:math><label>(9a)</label></disp-formula><disp-formula id="d9b"><mml:math display="block"><mml:mi>χ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:mfrac><mml:mrow><mml:msup><mml:mi>V</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>4</mml:mn><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="script">O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub><mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mn>2</mml:mn></mml:msup><mml:mo>,</mml:mo></mml:math><label>(9b)</label></disp-formula></disp-formula-group>where <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi><mml:mo>≡</mml:mo><mml:mo stretchy="false">⟨</mml:mo><mml:mover accent="true"><mml:mi>q</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mi>q</mml:mi><mml:mo stretchy="false">⟩</mml:mo></mml:math></inline-formula> are two independent integration constants in the UV region, dual to the quark mass and the chiral condensate, respectively. <inline-formula><mml:math display="inline"><mml:msub><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula> is an integration constant in the IR region and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo>≡</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>. In Ref. <xref ref-type="bibr" rid="c60">[60]</xref>, <inline-formula><mml:math display="inline"><mml:mi>ζ</mml:mi></mml:math></inline-formula> is identified as a normalization constant with the value <inline-formula><mml:math display="inline"><mml:mi>ζ</mml:mi><mml:mo>=</mml:mo><mml:mfrac><mml:msqrt><mml:msub><mml:mi>N</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:msqrt><mml:mrow><mml:mn>2</mml:mn><mml:mi>π</mml:mi></mml:mrow></mml:mfrac></mml:math></inline-formula>, which is obtained by mapping the correlation of the scalar operator to that from the 4D perturbative calculation. Here, we will take <inline-formula><mml:math display="inline"><mml:msub><mml:mi>N</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:math></inline-formula>. One of the integration constants in the IR region is discarded due to its association with a divergent solution at <inline-formula><mml:math display="inline"><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub></mml:math></inline-formula>. Thus, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula> is kept as the only coefficient corresponding to a regular solution at the horizon.</p><p>This study focuses on the scaling behavior of the chiral phase transition temperature. By utilizing the asymptotic expansions of the solutions near the UV boundary <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> and the IR horizon <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub></mml:math></inline-formula> as provided in Eqs. <xref ref-type="disp-formula" rid="d9a">(9a)</xref> and <xref ref-type="disp-formula" rid="d9b">(9b)</xref>, the boundary-valued problem can be reformulated as an iterative problem following the procedure established in our previous work <xref ref-type="bibr" rid="c42 c57">[42,57]</xref>. This enables the application of the “shooting method” <xref ref-type="bibr" rid="c61">[61]</xref> to extract the chiral condensate <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi></mml:math></inline-formula>. Before one can work it out, the scalar potential should be specified as well.</p><p>Following our previous study <xref ref-type="bibr" rid="c42">[42]</xref>, we choose the scalar potential to be <disp-formula id="d10"><mml:math display="block"><mml:mi>V</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mn>2</mml:mn></mml:mfrac><mml:msubsup><mml:mi>m</mml:mi><mml:mn>5</mml:mn><mml:mn>2</mml:mn></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:msup><mml:mi>χ</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mfrac><mml:mi>λ</mml:mi><mml:mn>8</mml:mn></mml:mfrac><mml:msup><mml:mi>χ</mml:mi><mml:mn>4</mml:mn></mml:msup><mml:mo>.</mml:mo></mml:math><label>(10)</label></disp-formula>Here, one can assume a general coupling between the scalar field and the dilaton field, such as <inline-formula><mml:math display="inline"><mml:msub><mml:mi>g</mml:mi><mml:mn>2</mml:mn></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>ϕ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:msup><mml:mi>χ</mml:mi><mml:mn>2</mml:mn></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>g</mml:mi><mml:mn>4</mml:mn></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>ϕ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:msup><mml:mi>χ</mml:mi><mml:mn>4</mml:mn></mml:msup></mml:math></inline-formula> with <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>g</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>g</mml:mi></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> two coupling functions. In this case, effective <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-dependent <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>m</mml:mi><mml:mn>5</mml:mn><mml:mn>2</mml:mn></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>λ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> can be introduced. That is why we treat <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>m</mml:mi><mml:mn>5</mml:mn><mml:mn>2</mml:mn></mml:msubsup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>λ</mml:mi></mml:math></inline-formula> as <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-dependent functions in the above potential. Following Ref. <xref ref-type="bibr" rid="c45">[45]</xref>, we will take <disp-formula id="d11"><mml:math display="block"><mml:mrow><mml:mi>Model</mml:mi><mml:mtext> </mml:mtext><mml:mi mathvariant="normal">I</mml:mi><mml:mo>:</mml:mo><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msubsup><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn>3</mml:mn><mml:mo>-</mml:mo><mml:msubsup><mml:mrow><mml:mi>μ</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:msup><mml:mrow><mml:mi>r</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math><label>(11)</label></disp-formula>and a constant <inline-formula><mml:math display="inline"><mml:mi>λ</mml:mi></mml:math></inline-formula>, which we will call “model I.” Here, the leading term <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo><mml:mn>3</mml:mn></mml:math></inline-formula> comes from the AdS/CFT prescription <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>M</mml:mi><mml:mn>5</mml:mn><mml:mn>2</mml:mn></mml:msubsup><mml:mo>=</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:mi>d</mml:mi><mml:mo>-</mml:mo><mml:mi>p</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:mi>d</mml:mi><mml:mo>+</mml:mo><mml:mi>p</mml:mi><mml:mo>-</mml:mo><mml:mn>4</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> with the dimension <inline-formula><mml:math display="inline"><mml:mi>d</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> for the scalar <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>q</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mi>q</mml:mi></mml:math></inline-formula> operator. Following Ref. <xref ref-type="bibr" rid="c62">[62]</xref>, we will take <disp-formula id="d12"><mml:math display="block"><mml:mrow><mml:mi>Model</mml:mi><mml:mtext> </mml:mtext><mml:mi>II</mml:mi><mml:mo>:</mml:mo><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msubsup><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn>3</mml:mn><mml:mo stretchy="false">[</mml:mo><mml:mn>1</mml:mn><mml:mo>+</mml:mo><mml:mi>γ</mml:mi><mml:mi>tanh</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>κ</mml:mi><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo stretchy="false">]</mml:mo></mml:mrow></mml:math><label>(12)</label></disp-formula>and a constant <inline-formula><mml:math display="inline"><mml:mi>λ</mml:mi></mml:math></inline-formula>, which we will call “model II.” The light meson spectra have been carefully studied in these two models, and the model parameters are fitted as shown in Table <xref ref-type="table" rid="t1">I</xref> for model I and in Table <xref ref-type="table" rid="t2">II</xref> for model II, which are taken from Refs. <xref ref-type="bibr" rid="c45 c62">[45,62]</xref>, respectively. The quark mass enters the two models through the boundary expansion of <inline-formula><mml:math display="inline"><mml:mi>χ</mml:mi></mml:math></inline-formula>, and the physical values <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>h</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> in Tables <xref ref-type="table" rid="t1">I</xref> and <xref ref-type="table" rid="t2">II</xref> give pion masses around the experimental value (we take 139.6 MeV). Here, the pion masses can be obtained by considering the perturbation of the Goldstone modes (for details, please refer to Refs. <xref ref-type="bibr" rid="c37 c38">[37,38]</xref>).</p><table-wrap id="t1" specific-use="style-1col"><object-id>I</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.t1</object-id><label>TABLE I.</label><caption><p>Fitting parameters in model I.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5"><oasis:colspec align="left" colname="col1" colsep="0" colwidth="24%"/><oasis:colspec align="center" colname="col2" colsep="0" colwidth="27%"/><oasis:colspec align="center" colname="col3" colsep="0" colwidth="23%"/><oasis:colspec align="center" colname="col4" colsep="0" colwidth="22%"/><oasis:colspec align="center" colname="col5" colsep="0" colwidth="11%"/><oasis:thead><oasis:row><oasis:entry valign="top">Parameters</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>h</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (MeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>g</mml:mi></mml:msub></mml:math></inline-formula> (MeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> (GeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:mi>λ</mml:mi></mml:math></inline-formula></oasis:entry></oasis:row></oasis:thead><oasis:tbody><oasis:row rowsep="0"><oasis:entry>Value</oasis:entry><oasis:entry>3.22</oasis:entry><oasis:entry>0.44</oasis:entry><oasis:entry>1.45</oasis:entry><oasis:entry>80</oasis:entry></oasis:row></oasis:tbody></oasis:tgroup></oasis:table></table-wrap><table-wrap id="t2" specific-use="style-1col"><object-id>II</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.t2</object-id><label>TABLE II.</label><caption><p>Fitting parameters in model II.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="6"><oasis:colspec align="left" colname="col1" colsep="0" colwidth="24%"/><oasis:colspec align="center" colname="col2" colsep="0" colwidth="27%"/><oasis:colspec align="center" colname="col3" colsep="0" colwidth="22%"/><oasis:colspec align="center" colname="col4" colsep="0" colwidth="9%"/><oasis:colspec align="center" colname="col5" colsep="0" colwidth="11%"/><oasis:colspec align="center" colname="col6" colsep="0" colwidth="14%"/><oasis:thead><oasis:row><oasis:entry valign="top">Parameters</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>h</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (MeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>g</mml:mi></mml:msub></mml:math></inline-formula> (MeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:mi>γ</mml:mi></mml:math></inline-formula></oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:mi>λ</mml:mi></mml:math></inline-formula></oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:mi>κ</mml:mi></mml:math></inline-formula></oasis:entry></oasis:row></oasis:thead><oasis:tbody><oasis:row rowsep="0"><oasis:entry>Value</oasis:entry><oasis:entry>3.90</oasis:entry><oasis:entry>0.35</oasis:entry><oasis:entry>6</oasis:entry><oasis:entry>25</oasis:entry><oasis:entry>0.85</oasis:entry></oasis:row></oasis:tbody></oasis:tgroup></oasis:table></table-wrap><p>Inserting the parameters in Tables <xref ref-type="table" rid="t1">I</xref> and <xref ref-type="table" rid="t2">II</xref> and into the two models, one can obtain the chiral condensate as a function of the temperature. Furthermore, since the quark mass appears in the boundary condition, it is also possible to vary its value, and correspondingly, one gets the function <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>. We plot the results in Fig. <xref ref-type="fig" rid="f1">1</xref>. In the upper, middle panels of the figure, the results of models I and II are presented, respectively. For each model, we show two different cases, with a physical quark mass and in the chiral limit. For the physical case, we tune the quark mass to get a pion mass of around 139.6 MeV, while in the chiral limit, we take <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> and correspondingly <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> for its Goldstone nature. The vacuum values of the condensate <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:math></inline-formula> and the second-order transition temperature are <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.01475</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msup><mml:mi>GeV</mml:mi><mml:mn>3</mml:mn></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>163.3</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:mrow></mml:math></inline-formula> for model I, and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.02749</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msup><mml:mi>GeV</mml:mi><mml:mn>3</mml:mn></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>160.9</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model II. For the physical quark masses, the pseudocritical temperatures extracted from the maxima of <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mi>d</mml:mi><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:mi>d</mml:mi><mml:mi>T</mml:mi><mml:mo stretchy="false">|</mml:mo></mml:math></inline-formula> are <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>164.0</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model I and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>161.2</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model II, while those from the maxima of the chiral susceptibility are <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>167.4</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model I and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>163.9</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model II (red dots). To eliminate the influence of other differences between the models, we plot the chiral condensate <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:math></inline-formula> (where <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:math></inline-formula> is the zero-temperature condensate) as a function of <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> across all the models, alongside lattice-QCD data (the filled black triangles) from Ref. <xref ref-type="bibr" rid="c6">[6]</xref>, as shown in Fig. <xref ref-type="fig" rid="f2">2</xref>. The results reveal a systematic trend: Models I and II (dashed and dotted-dashed lines) track the lattice data reasonably well near the pseudocritical temperature (<inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula>), but deviate significantly in the high-temperature crossover region (<inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula>). We explored parameter variations to improve the agreement, but the effect was marginal. The main reason is that the crossover transition at the physical quark mass appears too sharp in these two models, as illustrated in the figures, exhibiting an overly rapid decrease of the chiral condensate at high temperatures.</p><fig id="f1"><object-id>1</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f1</object-id><label>FIG. 1.</label><caption><p>Chiral phase transitions and the crossover region for different pion masses. The blue line corresponds to the chiral limit <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>, while the red line is for the physical pion mass (<inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>139.6</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>). The shaded gray area highlights the region between these two curves. Blue dots mark second-order phase-transition points; black and red dots indicate the pseudocritical temperatures obtained from the maxima of <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mi>d</mml:mi><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:mi>d</mml:mi><mml:mi>T</mml:mi><mml:mo stretchy="false">|</mml:mo></mml:math></inline-formula> and the chiral susceptibility, respectively.</p></caption><graphic xlink:href="e086010_1.eps"/></fig><fig id="f2"><object-id>2</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f2</object-id><label>FIG. 2.</label><caption><p>The variation of the normalized chiral condensate with <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> computed and compared with the lattice-QCD simulation results represented by black triangles with error bars, as reported in Ref. <xref ref-type="bibr" rid="c6">[6]</xref>.</p></caption><graphic xlink:href="e086010_2.eps"/></fig><p>To broaden the transition region, we note that the chiral condensate in the soft-wall model is sensitive to the quartic coupling. As demonstrated in Ref. <xref ref-type="bibr" rid="c47">[47]</xref>, a stronger quartic coupling term suppresses the chiral condensate more significantly at low temperatures. Specifically, if one introduces a quartic coefficient that depends on the coordinate <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> (induced by its coupling to the dilaton) and allows it to grow with increasing <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>, the low-temperature condensate is suppressed more strongly than its high-temperature counterpart. Furthermore, softening the potential at large <inline-formula><mml:math display="inline"><mml:mi>χ</mml:mi></mml:math></inline-formula> (e.g., by including a logarithmic term) enables the condensate to approach its <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> limit more gradually. The interplay between these two mechanisms is expected to effectively broaden the temperature profile of the condensate. Motivated by this insight, we propose a refined model formulation, defined as follows: <disp-formula id="d13"><mml:math display="block"><mml:mrow><mml:mi>Model</mml:mi><mml:mtext> </mml:mtext><mml:mi>III</mml:mi><mml:mo>:</mml:mo><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>V</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>χ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo id="d13a1">=</mml:mo><mml:mfrac><mml:mrow><mml:mn>1</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mfrac><mml:msubsup><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:msup><mml:mrow><mml:mi>χ</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:mn>1</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mfrac><mml:mi>λ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:msup><mml:mrow><mml:mi>χ</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mi>ln</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>1</mml:mn><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:msup><mml:mrow><mml:mi>χ</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mo>,</mml:mo><mml:mspace linebreak="newline"/><mml:msubsup><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo indentalign="id" indenttarget="d13a1">=</mml:mo><mml:mo>-</mml:mo><mml:mn>3</mml:mn><mml:mo>-</mml:mo><mml:msubsup><mml:mrow><mml:mi>μ</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:msup><mml:mrow><mml:mi>r</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:mspace linebreak="newline"/><mml:mi>λ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo indentalign="id" indenttarget="d13a1">=</mml:mo><mml:msub><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>−</mml:mo><mml:msub><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mn>1</mml:mn></mml:mrow></mml:msub><mml:mi>tanh</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub><mml:msup><mml:mrow><mml:mi>r</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math><label>(13)</label></disp-formula>We will call this model “model III.” As can be seen from the setup of these models, in addition to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>g</mml:mi></mml:msub></mml:math></inline-formula>, which accounts for linear confinement <xref ref-type="bibr" rid="c38">[38]</xref>, an additional scale is required to describe spontaneous chiral-symmetry breaking <xref ref-type="bibr" rid="c42">[42]</xref>.</p><p>Upon selecting parameter set 1 of model III from Table <xref ref-type="table" rid="t3">III</xref> and solving the equations of motion, we obtain the chiral condensate in this model. As illustrated in the bottom panel of Fig. <xref ref-type="fig" rid="f1">1</xref> and the green solid line in Fig. <xref ref-type="fig" rid="f2">2</xref>, model III (set 1) yields a broader crossover region, as expected. Compared to the other two models, model III with parameter set 1 (green solid line) achieves substantially better agreement with lattice-QCD results across the entire temperature range. It confirms that the functional form of the scalar potential itself—specifically, the logarithmic correction and <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> dependence in model III—is essential for capturing the quantitative thermodynamics of the chiral crossover. For later convenience, we also obtain the vacuum condensate <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:math></inline-formula> and the second-order transition temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> for model III set 1 as <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.002918</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msup><mml:mi>GeV</mml:mi><mml:mn>3</mml:mn></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>145.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>. Correspondingly, for physical quark masses, the pseudocritical temperature extracted from the maxima of <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mi>d</mml:mi><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:mi>d</mml:mi><mml:mi>T</mml:mi><mml:mo stretchy="false">|</mml:mo></mml:math></inline-formula> is <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>147.0</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model III set 1 (black dots), while that from the maxima of the chiral susceptibility is <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>151.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model III set 1 (red dots).</p><table-wrap id="t3" specific-use="style-1col"><object-id>III</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.t3</object-id><label>TABLE III.</label><caption><p>Fitting parameters in model III.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="8"><oasis:colspec align="left" colname="col1" colsep="0" colwidth="19%"/><oasis:colspec align="center" colname="col2" colsep="0" colwidth="21%"/><oasis:colspec align="center" colname="col3" colsep="0" colwidth="17%"/><oasis:colspec align="center" colname="col4" colsep="0" colwidth="17%"/><oasis:colspec align="center" colname="col5" colsep="0" colwidth="6%"/><oasis:colspec align="center" colname="col6" colsep="0" colwidth="8%"/><oasis:colspec align="center" colname="col7" colsep="0" colwidth="6%"/><oasis:colspec align="center" colname="col8" colsep="0" colwidth="9%"/><oasis:thead><oasis:row><oasis:entry valign="top">Parameters</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>h</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (MeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>g</mml:mi></mml:msub></mml:math></inline-formula> (MeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>μ</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> (GeV)</oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula></oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>a</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>a</mml:mi><mml:mn>1</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry><oasis:entry valign="top"><inline-formula><mml:math display="inline"><mml:msub><mml:mi>a</mml:mi><mml:mn>2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry></oasis:row></oasis:thead><oasis:tbody><oasis:row rowsep="0"><oasis:entry>Set 1</oasis:entry><oasis:entry>1.61</oasis:entry><oasis:entry>0.40</oasis:entry><oasis:entry>1.30</oasis:entry><oasis:entry>1</oasis:entry><oasis:entry>250</oasis:entry><oasis:entry>5</oasis:entry><oasis:entry>0.02</oasis:entry></oasis:row><oasis:row rowsep="0"><oasis:entry>Set 2</oasis:entry><oasis:entry>1.14</oasis:entry><oasis:entry>0.25</oasis:entry><oasis:entry>1.30</oasis:entry><oasis:entry>10</oasis:entry><oasis:entry>250</oasis:entry><oasis:entry>5</oasis:entry><oasis:entry>0.02</oasis:entry></oasis:row><oasis:row rowsep="0"><oasis:entry>Set 3</oasis:entry><oasis:entry>3.10</oasis:entry><oasis:entry>0.22</oasis:entry><oasis:entry>1.15</oasis:entry><oasis:entry>50</oasis:entry><oasis:entry>20</oasis:entry><oasis:entry>5</oasis:entry><oasis:entry>0.20</oasis:entry></oasis:row></oasis:tbody></oasis:tgroup></oasis:table></table-wrap><p>The broadening of the crossover region, which helps describe the lattice data at the physical quark mass in model III set 1, is also important for investigating scaling behaviors, particularly the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mi>–</mml:mi><mml:mi>m</mml:mi></mml:math></inline-formula> scaling. Since the primary objective of this work is to rigorously investigate these scaling behaviors, we introduce two additional parameter sets denoted as sets 2 and 3 (listed in Table <xref ref-type="table" rid="t3">III</xref>), which produce even broader crossover regions and provide a systematic assessment of how the crossover region affects the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mi>–</mml:mi><mml:mi>m</mml:mi></mml:math></inline-formula> scaling, as discussed in the following sections. As shown in the purple solid line in Fig. <xref ref-type="fig" rid="f2">2</xref>, model III set 2 produces a mild broadening of the phase transition region. Qualitatively, its deviation from the lattice-QCD data remains approximately within <inline-formula><mml:math display="inline"><mml:mn>1</mml:mn><mml:mi>σ</mml:mi></mml:math></inline-formula> for <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>&lt;</mml:mo><mml:mn>1.1</mml:mn><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> (with only a few data points slightly exceeding this bound). It should be emphasized that the “<inline-formula><mml:math display="inline"><mml:mn>1</mml:mn><mml:mi>σ</mml:mi></mml:math></inline-formula>” bound referred to here is a qualitative description rather than a rigorously defined statistical quantity. As shown in the blue solid line in Fig. <xref ref-type="fig" rid="f2">2</xref>, model III set 3 exhibits a larger deviation, remaining approximately within <inline-formula><mml:math display="inline"><mml:mn>5</mml:mn><mml:mi>σ</mml:mi></mml:math></inline-formula> for <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>&lt;</mml:mo><mml:mn>1.1</mml:mn><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula>. We qualitatively regard this as an upper bound on the effect of broadening the phase transition region. For later convenience, we also obtain <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.001688</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msup><mml:mi>GeV</mml:mi><mml:mn>3</mml:mn></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>163.1</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for set 2, and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.002175</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msup><mml:mi>GeV</mml:mi><mml:mn>3</mml:mn></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>144.4</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for set 3.</p><p>In summary, we have shown that the soft-wall model, with appropriate modifications, can accurately describe the chiral phase transition at the physical quark mass. Based on this, we will proceed to study the scaling properties in the subsequent sections.</p></sec><sec id="s3"><label>III.</label><title>SCALING FUNCTIONS IN THE HOLOGRAPHIC MODEL</title><p>As discussed in the last section, with arbitrarily small quark mass, the chiral phase transition turns into a crossover. When the transition point lies sufficiently close to the critical point, it can be strongly influenced by the critical point. A scaling window and universal scaling behavior appear in this region, which might be relevant to the search for the CEP of the QCD phase diagram if the CEP belongs to the same universality class. In this context, it has been verified that the chiral condensate near the critical point obeys the following scaling laws: <disp-formula id="d14"><mml:math display="block"><mml:mrow><mml:mi>σ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>T</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>q</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>∼</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>T</mml:mi><mml:msup><mml:mrow><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:mspace depth="0.0ex" height="0.0ex" width="2em"/><mml:mi>σ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>q</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>∼</mml:mo><mml:msubsup><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>q</mml:mi></mml:mrow><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:math><label>(14)</label></disp-formula>with <inline-formula><mml:math display="inline"><mml:mi>β</mml:mi><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:math></inline-formula> in the two-flavor limit <xref ref-type="bibr" rid="c47">[47]</xref>. However, these scaling laws capture the critical behavior only along certain directions, namely, holding <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> fixed for <inline-formula><mml:math display="inline"><mml:mi>β</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> fixed for <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi></mml:math></inline-formula>. To get more information about how the critical point governs the crossover region, one has to extract the scaling functions. This section is therefore devoted to their determination.</p><sec id="s3a"><label>A.</label><title>Scaling functions</title><p>The theoretical derivation of the universal scaling near a critical point can be easily found in a standard textbook <xref ref-type="bibr" rid="c63">[63]</xref> of statistical physics. Taking a spin system as an example, the order parameter or the magnetization <inline-formula><mml:math display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> obeys the scaling law <disp-formula id="d15"><mml:math display="block"><mml:mi>M</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>h</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msup><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>,</mml:mo></mml:math><label>(15)</label></disp-formula>where <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> is the scaling function, <inline-formula><mml:math display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula> is the source of the magnetization, and <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> is a scaling parameter defined as <disp-formula id="d16"><mml:math display="block"><mml:mrow><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mi>t</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mrow><mml:mi>h</mml:mi></mml:mrow><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:mspace depth="0.0ex" height="0.0ex" width="2em"/><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math><label>(16)</label></disp-formula>with <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>=</mml:mo><mml:mi>β</mml:mi><mml:mi>δ</mml:mi></mml:math></inline-formula>. If one takes <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> or <inline-formula><mml:math display="inline"><mml:mi>h</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>, the scaling law will be reduced to <disp-formula-group id="d17"><label>(17)</label><disp-formula id="d17a"><mml:math display="block"><mml:mi>M</mml:mi><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mi>h</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:math><label>(17a)</label></disp-formula><disp-formula id="d17b"><mml:math display="block"><mml:mi>M</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>h</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mi>β</mml:mi></mml:msup><mml:mo>,</mml:mo></mml:math><label>(17b)</label></disp-formula></disp-formula-group>which implies the conditions for <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub></mml:math></inline-formula>, <disp-formula id="d18"><mml:math display="block"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mspace depth="0.0ex" height="0.0ex" width="1em"/><mml:mi>and</mml:mi><mml:mspace depth="0.0ex" height="0.0ex" width="1em"/><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:munder><mml:mo stretchy="false">→</mml:mo><mml:mrow><mml:mi>z</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:mo>-</mml:mo><mml:mi>∞</mml:mi></mml:mrow></mml:munder><mml:mo stretchy="false">(</mml:mo><mml:mo>-</mml:mo><mml:mi>z</mml:mi><mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mi>β</mml:mi></mml:msup><mml:mo>.</mml:mo></mml:math><label>(18)</label></disp-formula></p><p>In the current model, the critical point locates at <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>. It can be numerically checked that the order parameter <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi></mml:math></inline-formula> in all three models obeys the following scaling law: <disp-formula-group id="d19"><label>(19)</label><disp-formula id="d19a"><mml:math display="block"><mml:mi>σ</mml:mi><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>=</mml:mo><mml:mi>A</mml:mi><mml:msubsup><mml:mi>m</mml:mi><mml:mi>q</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo></mml:math><label>(19a)</label></disp-formula><disp-formula id="d19b"><mml:math display="block"><mml:mrow><mml:mi>σ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>T</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>q</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mi>B</mml:mi><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>T</mml:mi><mml:msup><mml:mrow><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:mrow></mml:math><label>(19b)</label></disp-formula></disp-formula-group>with <inline-formula><mml:math display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> two coefficients, which can be numerically extracted. One can take <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> and vary <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> around <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> to get the near-critical temperature scaling. The results for the three models are given in Fig. <xref ref-type="fig" rid="f3">3</xref>. It is shown that <inline-formula><mml:math display="inline"><mml:msup><mml:mi>σ</mml:mi><mml:mn>2</mml:mn></mml:msup></mml:math></inline-formula> is almost a straight line as a function of <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, indicating <inline-formula><mml:math display="inline"><mml:mi>β</mml:mi><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:math></inline-formula>. Since the scaling function is a quantity independent of the specific parameter choice, and in order to more clearly compare the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling behavior of other holographic models in subsequent discussions, all results for model III presented in this section are obtained using parameter set 3, which yields a broader crossover region. By fitting the slope of the straight lines, one can get the coefficient <inline-formula><mml:math display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> as listed in Table <xref ref-type="table" rid="t4">IV</xref>. Similarly, one can take <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and vary <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> around <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>. It is found that in this case <inline-formula><mml:math display="inline"><mml:msup><mml:mi>σ</mml:mi><mml:mn>3</mml:mn></mml:msup></mml:math></inline-formula> is almost lying in a straight line as a function of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula>. Thus, one gets <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:math></inline-formula>. The coefficient <inline-formula><mml:math display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> can be obtained numerically, and we list the result in Table <xref ref-type="table" rid="t4">IV</xref>. In fact, those quantities can also be extracted analytically. Please refer to <xref ref-type="bibr" rid="c47">[47]</xref> for the details.</p><fig id="f3"><object-id>3</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f3</object-id><label>FIG. 3.</label><caption><p>Critical scaling behavior near the critical point across different models. Red and black symbols are numerical data from the three models; lines are fits.</p></caption><graphic xlink:href="e086010_3.eps"/></fig><table-wrap id="t4" specific-use="style-1col"><object-id>IV</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.t4</object-id><label>TABLE IV.</label><caption><p>The extracted values of <inline-formula><mml:math display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> as determined by various models.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3"><oasis:colspec align="left" colname="col1" colsep="0" colwidth="40%"/><oasis:colspec align="char" char="." colname="col2" colsep="0" colwidth="43%"/><oasis:colspec align="char" char="." colname="col3" colsep="0" colwidth="41%"/><oasis:thead><oasis:row><oasis:entry valign="top">Model</oasis:entry><oasis:entry align="center" valign="top"><inline-formula><mml:math display="inline"><mml:mi>A</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msup><mml:mi>GeV</mml:mi><mml:mrow><mml:mn>8</mml:mn><mml:mo>/</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:msup><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula></oasis:entry><oasis:entry align="center" valign="top"><inline-formula><mml:math display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:msup><mml:mi>GeV</mml:mi><mml:mn>2</mml:mn></mml:msup></mml:math></inline-formula>)</oasis:entry></oasis:row></oasis:thead><oasis:tbody><oasis:row rowsep="0"><oasis:entry>Model I</oasis:entry><oasis:entry>0.0367383</oasis:entry><oasis:entry>0.0935534</oasis:entry></oasis:row><oasis:row rowsep="0"><oasis:entry>Model II</oasis:entry><oasis:entry>0.0545202</oasis:entry><oasis:entry>0.172141</oasis:entry></oasis:row><oasis:row rowsep="0"><oasis:entry>Model III</oasis:entry><oasis:entry>0.00818794</oasis:entry><oasis:entry>0.0121398</oasis:entry></oasis:row></oasis:tbody></oasis:tgroup></oasis:table></table-wrap><p>To obtain the more general scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>, we follow the convention of <xref ref-type="bibr" rid="c64">[64]</xref> and define the magnetization as <inline-formula><mml:math display="inline"><mml:mi>M</mml:mi><mml:mo>=</mml:mo><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>σ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula>, the source <inline-formula><mml:math display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula> as <inline-formula><mml:math display="inline"><mml:mi>h</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>/</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. After that, we get <disp-formula-group id="d20"><label>(20)</label><disp-formula id="d20a"><mml:math display="block"><mml:mi>M</mml:mi><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo>,</mml:mo><mml:mi>h</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mi>A</mml:mi><mml:msup><mml:mi>h</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msup><mml:msubsup><mml:mi>m</mml:mi><mml:mn>0</mml:mn><mml:mrow><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msubsup></mml:mrow><mml:msub><mml:mi>σ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:mfrac><mml:mo>,</mml:mo></mml:math><label>(20a)</label></disp-formula><disp-formula id="d20b"><mml:math display="block"><mml:mi>M</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>h</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mi>B</mml:mi><mml:msup><mml:mi>t</mml:mi><mml:mi>β</mml:mi></mml:msup><mml:msubsup><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow><mml:mi>β</mml:mi></mml:msubsup></mml:mrow><mml:msub><mml:mi>σ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:mfrac><mml:mo>.</mml:mo></mml:math><label>(20b)</label></disp-formula></disp-formula-group>Then we get the scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> as <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mi>M</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi>h</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msup></mml:math></inline-formula>. By substituting the condition from Eq. <xref ref-type="disp-formula" rid="d17">(17)</xref> back into Eq. <xref ref-type="disp-formula" rid="d20">(20)</xref>, we can solve for <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>σ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula>, and then get the numerical results for <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>. We will discuss the numerical results in the next subsection.</p><p>In the literature, another scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> is widely studied. It is defined from the chiral susceptibility <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:math></inline-formula> as <disp-formula id="d21"><mml:math display="block"><mml:msub><mml:mi>χ</mml:mi><mml:mi>M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mo stretchy="false">∂</mml:mo><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">∂</mml:mo><mml:mi>h</mml:mi></mml:mrow></mml:mfrac><mml:mo>=</mml:mo><mml:mfrac><mml:msup><mml:mi>h</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mi>δ</mml:mi><mml:mo stretchy="false">-</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mi>m</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:mfrac><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>,</mml:mo></mml:math><label>(21)</label></disp-formula>which can be extracted from the near-critical values of chiral susceptibility in terms of the chiral condensate, <disp-formula id="d22"><mml:math display="block"><mml:msub><mml:mi>χ</mml:mi><mml:mi>M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:msub><mml:mi>m</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:msub><mml:mi>σ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:mfrac><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:msub><mml:mi>m</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:msub><mml:mi>σ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:mfrac><mml:mfrac><mml:mrow><mml:mo stretchy="false">∂</mml:mo><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">∂</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mo>.</mml:mo></mml:math><label>(22)</label></disp-formula>Here, although <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub></mml:math></inline-formula> can be extracted by numerically differentiating <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi></mml:math></inline-formula> with respect to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula>, it can be directly extracted by performing a perturbative analysis of Eq. <xref ref-type="disp-formula" rid="d8">(8)</xref>. If one gets a solution <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula> at a given temperature <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula>, a small variation <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> in the quark mass will induce a variation <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:mi>χ</mml:mi></mml:math></inline-formula> in <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula>. Then, it is easy to derive the equation of motion for <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:mi>χ</mml:mi></mml:math></inline-formula> as <disp-formula id="d23"><mml:math display="block"><mml:mi>δ</mml:mi><mml:msup><mml:mi>χ</mml:mi><mml:mo>′′</mml:mo></mml:msup><mml:mo>+</mml:mo><mml:mrow><mml:mo>(</mml:mo><mml:mn>3</mml:mn><mml:msup><mml:mi>A</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>+</mml:mo><mml:mfrac><mml:msup><mml:mi>f</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mi>f</mml:mi></mml:mfrac><mml:mo>-</mml:mo><mml:msup><mml:mi>ϕ</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow><mml:msup><mml:mrow><mml:mi>δ</mml:mi><mml:mi>χ</mml:mi></mml:mrow><mml:mo>′</mml:mo></mml:msup><mml:mo>-</mml:mo><mml:mfrac><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mn>2</mml:mn><mml:mi>A</mml:mi></mml:mrow></mml:msup><mml:mi>f</mml:mi></mml:mfrac><mml:msub><mml:mi>V</mml:mi><mml:mrow><mml:mo>,</mml:mo><mml:mi>χ</mml:mi><mml:mi>χ</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mi>χ</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mi>δ</mml:mi><mml:mi>χ</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo>.</mml:mo></mml:math><label>(23)</label></disp-formula>As in the above discussion, we can obtain the expansion of <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:mi>χ</mml:mi></mml:math></inline-formula> at <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi>h</mml:mi></mml:msub></mml:math></inline-formula> as <disp-formula-group id="d24"><label>(24)</label><disp-formula id="d24a"><mml:math display="block"><mml:mi>δ</mml:mi><mml:mi>χ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mi>δ</mml:mi><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mi>ζ</mml:mi><mml:mi>r</mml:mi><mml:mo>+</mml:mo><mml:mo>⋯</mml:mo><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:mi>δ</mml:mi><mml:mi>σ</mml:mi></mml:mrow><mml:mi>ζ</mml:mi></mml:mfrac><mml:msup><mml:mi>r</mml:mi><mml:mn>3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi mathvariant="script">O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msup><mml:mi>r</mml:mi><mml:mn>4</mml:mn></mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mo>,</mml:mo></mml:math><label>(24a)</label></disp-formula><disp-formula id="d24b"><mml:math display="block"><mml:mrow><mml:mi>δ</mml:mi><mml:mi>χ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:msub><mml:mrow><mml:mi>r</mml:mi></mml:mrow><mml:mrow><mml:mi>h</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo>−</mml:mo><mml:mfrac><mml:mrow><mml:msup><mml:mrow><mml:mi>V</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>c</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>4</mml:mn><mml:msub><mml:mrow><mml:mi>r</mml:mi></mml:mrow><mml:mrow><mml:mi>h</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mrow><mml:mi>r</mml:mi></mml:mrow><mml:mrow><mml:mi>h</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="script">O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>r</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mrow><mml:mi>r</mml:mi></mml:mrow><mml:mrow><mml:mi>h</mml:mi></mml:mrow></mml:msub><mml:msup><mml:mrow><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math><label>(24b)</label></disp-formula></disp-formula-group>Then, using the same shooting method as in Sec. <xref ref-type="sec" rid="s2">II</xref>, one can obtain <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:mi>σ</mml:mi></mml:math></inline-formula> as a function of <inline-formula><mml:math display="inline"><mml:mi>δ</mml:mi><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> for given temperatures. Thus, the chiral susceptibility can be obtained as <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>δ</mml:mi><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:mi>δ</mml:mi><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula>. We will discuss the numerical results later. Before that, we note that the scaling functions <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula> have a general relation. Performing the differentiation with respect to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula>, it is not difficult to get <disp-formula id="d25"><mml:math display="block"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mi>δ</mml:mi></mml:mfrac><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>-</mml:mo><mml:mfrac><mml:mi>z</mml:mi><mml:mrow><mml:mi>β</mml:mi><mml:mi>δ</mml:mi></mml:mrow></mml:mfrac><mml:msubsup><mml:mi>f</mml:mi><mml:mi>G</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>.</mml:mo></mml:math><label>(25)</label></disp-formula></p><p>Considering the case <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, Eqs. <xref ref-type="disp-formula" rid="d15">(15)</xref> and <xref ref-type="disp-formula" rid="d21">(21)</xref> yield that the ratio between the two scaling functions approaches a constant near the critical point, i.e., <disp-formula id="d26"><mml:math display="block"><mml:mfrac><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:mfrac><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mi>δ</mml:mi></mml:mfrac><mml:mo>.</mml:mo></mml:math><label>(26)</label></disp-formula>The above relations are quite general for different systems. Thus, a self-consistent holographic model should produce results obeying those constraints. We will check the numerical results from the soft-wall model in the next section.</p></sec><sec id="s3b"><label>B.</label><title>Numerical scaling functions from the soft-wall AdS/QCD models</title><p>With the preparations described above, we numerically extract the scaling functions in the soft-wall AdS/QCD models. First, we obtain the numerical data for the chiral condensate <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi></mml:math></inline-formula> near the critical point (<inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> near <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> around 0). Then, from Eqs. <xref ref-type="disp-formula" rid="d15">(15)</xref> and <xref ref-type="disp-formula" rid="d20a">(20a)</xref>, we can extract the results of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>. The numerical results of the three models and the comparison with the mean-field result from Ref. <xref ref-type="bibr" rid="c65">[65]</xref> are presented in Fig. <xref ref-type="fig" rid="f4">4</xref>. For each case, we take <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.1</mml:mn><mml:mo>,</mml:mo><mml:mn>0.2</mml:mn><mml:mo>,</mml:mo><mml:mn>0.3</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> as examples. It can be seen that for all models the scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> approaches the mean-field result (the black solid lines) from <xref ref-type="bibr" rid="c65">[65]</xref> when the quark mass approaches the chiral limit. It can be checked that <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula> for all models, consistent with the definition. In the range of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo><mml:mn>2</mml:mn><mml:mo>&lt;</mml:mo><mml:mi>z</mml:mi><mml:mo>&lt;</mml:mo><mml:mn>5</mml:mn></mml:math></inline-formula>, all three models merge with mean-field results together. But in the range of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo><mml:mn>5</mml:mn><mml:mo>&lt;</mml:mo><mml:mi>z</mml:mi><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn>2</mml:mn></mml:math></inline-formula>, the results in models I and II converge much faster to the mean field, while for model III it is slower and agrees with the mean-field result only when <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> is of order <inline-formula><mml:math display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> (that is why we add <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.01</mml:mn><mml:mo>,</mml:mo><mml:mn>0.03</mml:mn><mml:mo>,</mml:mo><mml:mn>0.05</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for model III). It is not difficult to understand this behavior, as the increase in <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> will drive the system away from the critical point, resulting in a violation of the scaling behavior. However, it appears that the scaling window for model III is smaller than the other two models. Later, we will see the impact of this in the scaling of the pseudocritical temperatures.</p><fig id="f4"><object-id>4</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f4</object-id><label>FIG. 4.</label><caption><p>Scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> for the three holographic models at several finite quark masses, together with the mean-field result (black solid line) taken from Ref. <xref ref-type="bibr" rid="c65">[65]</xref>.</p></caption><graphic xlink:href="e086010_4.eps"/></fig><p>As a check of the consistency of the model, we also examine the behavior of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> as <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> approaches <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo><mml:mi>∞</mml:mi></mml:math></inline-formula>. It is shown in Fig. <xref ref-type="fig" rid="f5">5</xref> that when <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> decreases to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo><mml:mn>8</mml:mn></mml:math></inline-formula>, in the three models, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> can be well described by <inline-formula><mml:math display="inline"><mml:mo stretchy="false">(</mml:mo><mml:mo>-</mml:mo><mml:mi>z</mml:mi><mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. From these calculations, we confirm that the full critical scaling of the soft-wall AdS/QCD models is governed by the mean-field scaling. To construct a more realistic model, we also compare the scaling function in model III with the lattice results for the <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>4</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> model in Fig. <xref ref-type="fig" rid="f6">6</xref>. From the figure, obvious deviations of the model results from the lattice results appear in the range of <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi><mml:mo>&gt;</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula>. Though the scaling function is defined at the critical point, for later discussion, we also present a direct extension through Eqs. <xref ref-type="disp-formula" rid="d15">(15)</xref> and <xref ref-type="disp-formula" rid="d20a">(20a)</xref> to <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>q</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0.01</mml:mn><mml:mo>,</mml:mo><mml:mn>0.3</mml:mn><mml:mo>,</mml:mo><mml:mn>1</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:mrow></mml:math></inline-formula> and the physical point. Interestingly, the extended scaling function bends toward the lattice results in the region of negative <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>. As the quark mass slightly increases, part of the scaling function gradually shifts toward the <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>4</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> behavior observed in lattice QCD <xref ref-type="bibr" rid="c66 c67">[66,67]</xref>. By comparison, the other two soft-wall models yield scaling functions that remain valid over a broader range as the quark mass changes. This might help improve the temperature scaling within the framework of the soft-wall model, which can be seen in the later discussion.</p><fig id="f5"><object-id>5</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f5</object-id><label>FIG. 5.</label><caption><p>The asymptotic fitting of the scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub></mml:math></inline-formula> to <inline-formula><mml:math display="inline"><mml:mo stretchy="false">(</mml:mo><mml:mo>-</mml:mo><mml:mi>z</mml:mi><mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mi>β</mml:mi></mml:msup></mml:math></inline-formula> as <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:mo>-</mml:mo><mml:mi>∞</mml:mi></mml:math></inline-formula>. The quark mass is set to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.01</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> for all three models.</p></caption><graphic xlink:href="e086010_5.eps"/></fig><fig id="f6"><object-id>6</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f6</object-id><label>FIG. 6.</label><caption><p>A comparison of the scaling function obtained from model III set 3 with those derived from the mean-field approximation <xref ref-type="bibr" rid="c65">[65]</xref> (the red dashed line) and lattice-QCD simulations for <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>4</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> model <xref ref-type="bibr" rid="c66 c67">[66,67]</xref> (the gray solid line).</p></caption><graphic xlink:href="e086010_6.eps"/></fig><p>For the scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula>, as mentioned in the previous section, it can be obtained in two different ways. First, we can directly extract it through the general relation Eq. <xref ref-type="disp-formula" rid="d25">(25)</xref>. The results in model III are given in Fig. <xref ref-type="fig" rid="f7">7</xref>, compared with the lattice simulation of Ref. <xref ref-type="bibr" rid="c16">[16]</xref>. From the figure, we obtain <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>≃</mml:mo><mml:mn>0.322</mml:mn></mml:math></inline-formula>. From Eq. <xref ref-type="disp-formula" rid="d26">(26)</xref>, this value should be <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mi>δ</mml:mi></mml:mfrac><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mn>3</mml:mn></mml:mfrac></mml:math></inline-formula>. The deviation from this exact value is mainly from the numerical errors, due to the complexity of directly taking <inline-formula><mml:math display="inline"><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> (instead, we take a tiny but finite value). It can also be seen that a peak with its center at <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn>1.115</mml:mn><mml:mo>,</mml:mo><mml:msubsup><mml:mi>f</mml:mi><mml:mi>χ</mml:mi><mml:mi>max</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:mn>0.406</mml:mn></mml:math></inline-formula> appears in the curve for <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula>. The ratio <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>χ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is approximately equal to 79%. Later, we will see an interesting connection between this ratio and the temperature scaling behavior. Since the holographic computation is restricted to the mean-field approximation, its prediction for <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula> cannot quantitatively agree with any of the lattice results obtained for the O(4), O(2), or Z(2) universality classes. The underlying scaling relations are nevertheless respected; all differences stem solely from the distinct critical exponents.</p><fig id="f7"><object-id>7</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f7</object-id><label>FIG. 7.</label><caption><p>A comparison of the scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> from model III set 3, with the corresponding results derived from lattice QCD in the <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>2</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>Z</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>2</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>4</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> universality classes <xref ref-type="bibr" rid="c16">[16]</xref>.</p></caption><graphic xlink:href="e086010_7.eps"/></fig><p>We can also obtain <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula> from the chiral susceptibility through Eq. <xref ref-type="disp-formula" rid="d21">(21)</xref>. Figure <xref ref-type="fig" rid="f8">8</xref> presents the computed <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula> from various models in this way, compared to the theoretical predictions obtained from Eq. <xref ref-type="disp-formula" rid="d25">(25)</xref>. From the figure, we can see that the results obtained from the two methods are almost the same when the quark masses are very small. Thus, the general relation between <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula> is satisfied in the soft-wall model. Notably, model III displays a stronger dependence on the quark mass, while models I and II exhibit relatively minor changes in their scaling functions. This suggests that, under the mean-field approximation, variations among models may lead to different scaling regions.</p><fig id="f8"><object-id>8</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f8</object-id><label>FIG. 8.</label><caption><p>The dependence of the scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula> on the quark mass. The solid curve denotes the theoretical prediction extracted from <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub></mml:math></inline-formula> through Eq. <xref ref-type="disp-formula" rid="d25">(25)</xref>, whereas the dashed curves illustrate the scaling functions for various quark masses.</p></caption><graphic xlink:href="e086010_8.eps"/></fig><p>In a short summary, all the soft-wall models obey the same scaling behavior. The obtained scaling functions are the same for various models. However, when extended to finite quark masses, the scaling functions might show a slight dependence on the quark mass, and the scaling region might be different for different models.</p></sec></sec><sec id="s4"><label>IV.</label><title>TC SCALING BEHAVIOR UNDER THE CHIRAL PHASE TRANSITION</title><p>As already mentioned in the above sections, by taking a tiny but finite quark mass, the chiral phase transition turns from a second-order transition into a continuous crossover. Although the continuous crossover is not a real phase transition, it is a smooth and rapid change between two different phases, and one can define a pseudocritical temperature in different ways. Generally, the pseudocritical temperature also obeys a certain kind of scaling law. In this section, we will investigate the scaling behavior of the transition temperature.</p><sec id="s4a"><label>A.</label><title>Chiral order parameters</title><p>Several kinds of chiral order parameters can be used in a pseudotransition. For the holographic calculation, two of them are suitable for extracting the transition temperature. One of them is defined from the peak of the derivative with temperature <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mi>d</mml:mi><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:mi>d</mml:mi><mml:mi>T</mml:mi><mml:mo stretchy="false">|</mml:mo></mml:math></inline-formula>, while the other is from the peak of the chiral susceptibility defined as <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mo stretchy="false">∂</mml:mo><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">∂</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:math></inline-formula>.</p><p>According to Ref. <xref ref-type="bibr" rid="c68">[68]</xref>, although the chiral order parameters differ, the extracted pseudocritical temperatures differ only slightly, whereas Ref. <xref ref-type="bibr" rid="c69">[69]</xref> shows that different chiral order parameters can lead to much larger discrepancies in pseudocritical temperature. To study the impact of the chiral order parameters, we take two different cases in model III set 3 with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.059</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>20</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>3.63</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>150</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> as examples. As shown in Fig. <xref ref-type="fig" rid="f9">9</xref>, we can extract <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> by identifying the temperatures corresponding to the peaks of the two different chiral order parameters. With <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.059</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>, as shown in the blue curves, the peak of <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mi>d</mml:mi><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:mi>d</mml:mi><mml:mi>T</mml:mi><mml:mo stretchy="false">|</mml:mo></mml:math></inline-formula> locates at <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mo>,</mml:mo><mml:mi>σ</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0.1444</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula> with a height of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>σ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>13.83</mml:mn></mml:math></inline-formula>, which are very close to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mo>,</mml:mo><mml:mi>χ</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0.1451</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>14.42</mml:mn></mml:math></inline-formula>. As for <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>3.63</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>, both the peak location and its height obtain larger differences, with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mo>,</mml:mo><mml:mi>σ</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0.1481</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>σ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>2.96</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mo>,</mml:mo><mml:mi>χ</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0.1586</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>2.13</mml:mn></mml:math></inline-formula>.</p><fig id="f9"><object-id>9</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f9</object-id><label>FIG. 9.</label><caption><p>The critical temperatures <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> from chiral susceptibility and chiral condensate, with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>150</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>20</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>. The normalized value denotes each susceptibility scaled by the mean of all susceptibilities.</p></caption><graphic xlink:href="e086010_9.eps"/></fig><p>Similar calculations can be imposed for the other values of the quark mass. To show the tendency of the chiral susceptibility, we give the results for various pion masses from model III set 3 in Fig. <xref ref-type="fig" rid="f10">10</xref>. From the figure, we can see that when the quark mass increases, the height of the peaks of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub></mml:math></inline-formula> decreases, while the pseudocritical temperature (the peak location) increases. We also present the results of the pseudocritical temperatures for all three models in Fig. <xref ref-type="fig" rid="f11">11</xref>. We observe that the critical temperatures obtained from the two different order parameters differ significantly at high temperatures, with the one from the chiral susceptibility being much more sensitive to the pion mass. Generally, the transition temperatures from the chiral susceptibility are higher than those from <inline-formula><mml:math display="inline"><mml:mi>d</mml:mi><mml:mi>σ</mml:mi><mml:mo>/</mml:mo><mml:mi>d</mml:mi><mml:mi>T</mml:mi></mml:math></inline-formula> with the same quark mass. It is self-consistent that the differences of the two transition temperatures vanish toward the chiral limit, when the transition becomes a rigorous one and an exact transition temperature can be defined. For the effect of the model setting, it is easy to see that both transition temperatures from the two order parameters in model III are more sensitive to the pion mass than those in models I and II. In fact, this is why we adopt the model proposed in this work to study the dependence of the critical temperature, extracted from the chiral susceptibility, on both the quark mass and the pion mass. Since the chiral susceptibility is widely used in both functional renormalization group calculations and lattice QCD, we will identify the pseudocritical temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> with the maximum (<inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi><mml:mi>max</mml:mi></mml:msubsup></mml:math></inline-formula>) of the chiral susceptibility in later calculations, in order to give a straightforward comparison with the other methods.</p><fig id="f10"><object-id>10</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f10</object-id><label>FIG. 10.</label><caption><p>Chiral susceptibility for various pion masses in model III set 3.</p></caption><graphic xlink:href="e086010_10.eps"/></fig><fig id="f11"><object-id>11</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f11</object-id><label>FIG. 11.</label><caption><p>The pseudopion mass varies with different chiral order parameters and the temperature of the phase transition. The open circles represent the critical temperatures extracted using the chiral condensate as the order parameter, while the solid circles correspond to those obtained from the chiral susceptibility. All temperatures are shifted by subtracting the pseudocritical temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> in the chiral limit.</p></caption><graphic xlink:href="e086010_11.eps"/></fig></sec><sec id="s4b"><label>B.</label><title><inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling</title><p>Generally, with a small value of quark mass, the physics near the transition temperature is still governed by the critical scaling behavior. Thus, for small quark masses, the corresponding pseudocritical temperature also obeys a scaling law as <disp-formula id="d27"><mml:math display="block"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>α</mml:mi><mml:mo>×</mml:mo><mml:msubsup><mml:mi>m</mml:mi><mml:mi>q</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>,</mml:mo></mml:math><label>(27)</label></disp-formula>with <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>=</mml:mo><mml:mrow><mml:mi>β</mml:mi><mml:mi>δ</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> the critical temperature in the chiral limit, and <inline-formula><mml:math display="inline"><mml:mi>α</mml:mi></mml:math></inline-formula> a coefficient depending on the models. This scaling law can be derived from the near-critical scaling of <inline-formula><mml:math display="inline"><mml:mi>σ</mml:mi></mml:math></inline-formula>. Since the holographic model gives the mean-field critical exponents <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>β</mml:mi><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>δ</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:math></inline-formula>, we have <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:math></inline-formula>. As proved in <xref ref-type="bibr" rid="c37">[37]</xref>, the Gell-Mann-Oakes-Renner relation <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>m</mml:mi><mml:mi>π</mml:mi><mml:mn>2</mml:mn></mml:msubsup><mml:msubsup><mml:mi>f</mml:mi><mml:mi>π</mml:mi><mml:mn>2</mml:mn></mml:msubsup><mml:mo>=</mml:mo><mml:mn>2</mml:mn><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo stretchy="false">⟨</mml:mo><mml:mover accent="true"><mml:mi>q</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mi>q</mml:mi><mml:mo stretchy="false">⟩</mml:mo></mml:math></inline-formula> is satisfied in the soft-wall model; thus, we have <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi>m</mml:mi><mml:mi>π</mml:mi><mml:mn>2</mml:mn></mml:msubsup><mml:mo>∝</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mi>m</mml:mi><mml:mi>π</mml:mi><mml:mrow><mml:mn>4</mml:mn><mml:mo>/</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>.</p><p>As an explicit check of this scaling behavior, we extract the pseudocritical temperatures as functions of the quark mass for the three models, as shown in the blue dots in Fig. <xref ref-type="fig" rid="f12">12</xref>. The upper, middle, and lower panels show the results in models I, II, and III, respectively. There, we show that the pseudocritical temperatures can be well described by the scaling law (the red dashed lines) with <inline-formula><mml:math display="inline"><mml:mi>α</mml:mi><mml:mo>=</mml:mo><mml:mn>4.0</mml:mn></mml:math></inline-formula> for model I, <inline-formula><mml:math display="inline"><mml:mi>α</mml:mi><mml:mo>=</mml:mo><mml:mn>3.0</mml:mn></mml:math></inline-formula> for model II, and <inline-formula><mml:math display="inline"><mml:mi>α</mml:mi><mml:mo>=</mml:mo><mml:mn>12.3</mml:mn></mml:math></inline-formula> for model III, with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> taking the values in the chiral limit of the corresponding models. From the fitting, it is interesting to see that the “slope” <inline-formula><mml:math display="inline"><mml:mi>α</mml:mi></mml:math></inline-formula> in model III set 3 is much larger than that in models I and II.</p><fig id="f12"><object-id>12</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f12</object-id><label>FIG. 12.</label><caption><p>The dependence of the pseudocritical temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> on the scaled quark mass <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>h</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, with the physical quark mass <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>h</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> corresponding to <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>139.6</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>. The red dashed curve represents the fit obtained using the data points.</p></caption><graphic xlink:href="e086010_12.eps"/></fig><p>In Fig. <xref ref-type="fig" rid="f13">13</xref>, we present the results for the pseudocritical temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> as a function of the pion mass. Because of the limited availability of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>N</mml:mi><mml:mi>f</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>2</mml:mn></mml:math></inline-formula> data, we take the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>N</mml:mi><mml:mi>f</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>2</mml:mn><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula> results from lattice QCD (the orange-brown dot-dashed line, from <xref ref-type="bibr" rid="c16">[16]</xref>), FRG (the medium gray dashed line, from <xref ref-type="bibr" rid="c70">[70]</xref>), and DSE approaches (the light blue dashed line and light blue dotted line, from <xref ref-type="bibr" rid="c9">[9]</xref>) for comparison. We have subtracted the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> data from <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> in order to get rid of the effect of differences in <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. From the figure, it can be seen that, unlike the LQCD and FRG results, our model does not exhibit a linear dependence. The linear dependence observed in the FRG and LQCD results is because their critical exponents are beyond the mean-field level of the 3D <inline-formula><mml:math display="inline"><mml:mi>O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>4</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> universal class. Here we show the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula>-scaling blue band corresponding to different parameter choices in model III. It is evident that, in the case of the largest values, our results approach those obtained from the DSE analysis.</p><fig id="f13"><object-id>13</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f13</object-id><label>FIG. 13.</label><caption><p>The pseudocritical temperature as a function of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub></mml:math></inline-formula> for different models. The lattice-QCD results are taken from Ref. <xref ref-type="bibr" rid="c16">[16]</xref>, the FRG results are taken from Ref. <xref ref-type="bibr" rid="c70">[70]</xref>, and the DSEs approach results are taken from Ref. <xref ref-type="bibr" rid="c9">[9]</xref>.</p></caption><graphic xlink:href="e086010_13.eps"/></fig><p>Besides the match of scaling exponent <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> with the DSE results for all three models, it is obvious that the increasing rates in models I and II are too small compared with the DSE results, as well as the lattice simulations. However, by doing a further modification to the scalar potentials, we find a way to cure this problem in model III. The logarithmic term and the <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-dependent coupling in the scalar potential soften the potential, thereby broadening the continuous transition and making the scaling slope steeper. This is why we try to propose a new modification to the soft-wall model. We note that the scaling of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> should be taken into account in model construction within the soft-wall framework. It is important to clarify, however, that the primary goal of this work is to demonstrate the qualitative capability of model III, rather than to present a finalized, perfectly optimized parameter set. The three parameter sets of model III represented by the blue band in Fig. <xref ref-type="fig" rid="f13">13</xref> demonstrate that model III has the potential to achieve <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling results closer to those of lattice QCD and DSE.</p><p>Furthermore, in Fig. <xref ref-type="fig" rid="f14">14</xref> we show the relation between the maximum chiral susceptibility <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mrow><mml:mi>σ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub></mml:math></inline-formula>. According to Ref. <xref ref-type="bibr" rid="c71">[71]</xref>, they obey the following scaling behavior: <disp-formula id="d28"><mml:math display="block"><mml:msub><mml:mi>χ</mml:mi><mml:mrow><mml:mi>σ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi>C</mml:mi><mml:mo>×</mml:mo><mml:msubsup><mml:mi>m</mml:mi><mml:mi>q</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>δ</mml:mi><mml:mo>-</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:msubsup><mml:mo>.</mml:mo></mml:math><label>(28)</label></disp-formula>It can be seen from the figure that the scaling law (the blue dotted lines) fits the numerical data quite well. The coefficient <inline-formula><mml:math display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is fitted as <inline-formula><mml:math display="inline"><mml:mi>C</mml:mi><mml:mo>=</mml:mo><mml:mn>0.015</mml:mn></mml:math></inline-formula> for model I, <inline-formula><mml:math display="inline"><mml:mi>C</mml:mi><mml:mo>=</mml:mo><mml:mn>0.023</mml:mn></mml:math></inline-formula> for model II, and <inline-formula><mml:math display="inline"><mml:mi>C</mml:mi><mml:mo>=</mml:mo><mml:mn>0.0034</mml:mn></mml:math></inline-formula> for model III set 3. Again, we see that the coefficient in model III set 3 has a different order from models I and II, which might be important in improving the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling with pion mass.</p><fig id="f14"><object-id>14</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f14</object-id><label>FIG. 14.</label><caption><p>Dependence of the maximum chiral susceptibility <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mrow><mml:mi>σ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> on the quark mass.</p></caption><graphic xlink:href="e086010_14.eps"/></fig><p>Therefore, we have seen that all the scaling laws are satisfied in the soft-wall AdS/QCD models, though all the exponents are at the mean-field level. It can also be seen that the models with a simple power of the scalar potential cannot well describe the coefficients (or the slopes). We propose a way to improve this behavior and get comparable <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling in both the exponents and the coefficients, with those obtained from the other nonperturbative methods.</p></sec><sec id="s4c"><label>C.</label><title>The transition temperature toward the chiral limit</title><p>Before closing this section, we will discuss another interesting topic. As we know, it is more expensive for lattice simulations to work with a smaller quark mass. In particular, it is very hard in the chiral limit. Thus, different ways have been developed to extrapolate the finite quark-mass calculation to get reliable results in the chiral limit. To get the critical temperature in the chiral limit at a lower cost, it is better to find certain observables from which the critical temperatures converge to that in the chiral limit more rapidly. As shown in lattice simulations <xref ref-type="bibr" rid="c16">[16]</xref>, the ratio <inline-formula><mml:math display="inline"><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>χ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> coincides with the ratio of the chiral susceptibility evaluated at the critical temperature in the chiral limit to its peak value, i.e., <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>χ</mml:mi><mml:mrow><mml:mi>σ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>χ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi>R</mml:mi></mml:math></inline-formula> for small quark masses. Such a conclusion comes from the fact that the pseudocritical temperatures for small quark masses are governed by the critical point and thus controlled by <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub></mml:math></inline-formula> as well (<inline-formula><mml:math display="inline"><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> characterizes the critical point). A direct consequence of this relation is that <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> can be obtained from calculations at finite quark masses from the condition <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mi>R</mml:mi><mml:msub><mml:mi>χ</mml:mi><mml:mrow><mml:mi>σ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (here, we note that there are two temperatures satisfying this condition, and one has to choose the lower one). In this section, we provide explicit holographic confirmation of this relation.</p><p>From the previous discussion, we have <inline-formula><mml:math display="inline"><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>χ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub><mml:mo>≃</mml:mo><mml:mn>79</mml:mn><mml:mo>%</mml:mo></mml:math></inline-formula> in the soft-wall model. Thus, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> is expected to correspond to the 79% height of the peaks at finite quark masses. As an explicit check, in Fig. <xref ref-type="fig" rid="f15">15</xref>, we compare the temperatures corresponding to the peak of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub></mml:math></inline-formula> (the blue solid line) for different pion masses with those obtained from the 79% height of the peak (the black dots), in reference to our critical temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (the red dashed line). The figure clearly shows that the percentage-temperature <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>percent</mml:mi></mml:msub></mml:math></inline-formula> approaches <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> much faster than <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula>. For <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>60</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>MeV</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>percent</mml:mi></mml:msub></mml:math></inline-formula> almost reaches <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, while <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> only in the chiral limit <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>. Here, although we have so far presented results only for model III set 3, we have checked that the relation holds in models I and II as well. Therefore, the holographic calculation confirms that the percentage temperature is a good observable for extracting <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> from finite quark-mass calculations.</p><fig id="f15"><object-id>15</object-id><object-id pub-id-type="doi">10.1103/7njb-6v24.f15</object-id><label>FIG. 15.</label><caption><p>The relation between the pion mass <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub></mml:math></inline-formula> and the temperature at which <inline-formula><mml:math display="inline"><mml:msub><mml:mi>χ</mml:mi><mml:mi>σ</mml:mi></mml:msub></mml:math></inline-formula> reaches 79% of its maximum value.</p></caption><graphic xlink:href="e086010_15.eps"/></fig></sec></sec><sec id="s5"><label>V.</label><title>CONCLUSION AND DISCUSSION</title><p>The critical point of the two-flavor soft-wall AdS/QCD model is systematically studied in Ref. <xref ref-type="bibr" rid="c47">[47]</xref>, and it is proved to exhibit mean-field scaling laws with exponents <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>β</mml:mi><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>δ</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:math></inline-formula>, when tuning either the temperature or the quark mass in its vicinity. However, the universal scaling functions that arise when the temperature and quark mass are varied simultaneously, together with the scaling behavior of the pseudocritical temperature itself, remain largely unexplored in this model. To verify the effectiveness and internal consistency of this holographic model, we present a careful study of the near-critical scaling behavior of various chiral order parameters.</p><p>Under different model settings and physical conditions, we find that the rescaled magnetization <inline-formula><mml:math display="inline"><mml:mi>M</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi>h</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>δ</mml:mi></mml:mrow></mml:msup></mml:math></inline-formula> in the chiral limit collapses onto a single, universal curve in the chiral limit <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>q</mml:mi></mml:msub><mml:mo stretchy="false">→</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>, defining the scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>. Quantitatively, this scaling function obtained numerically from holography is in excellent agreement with its four-dimensional mean-field counterpart. Furthermore, we derive a perturbative equation to evaluate the chiral susceptibility, from which we obtain another universal scaling function <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula>. It is found that the universal relationship <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mi>δ</mml:mi></mml:mfrac><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi>G</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>-</mml:mo><mml:mfrac><mml:mi>z</mml:mi><mml:mrow><mml:mi>β</mml:mi><mml:mi>δ</mml:mi></mml:mrow></mml:mfrac><mml:msubsup><mml:mi>f</mml:mi><mml:mi>G</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> holds in all three models, confirming the theoretical consistency of this holographic framework.</p><p>Furthermore, we extract the pseudocritical temperature from the peak of the susceptibility and from the inflection point of the chiral condensate. In contrast to the claim in Ref. <xref ref-type="bibr" rid="c68">[68]</xref>, the three models yield markedly different pseudocritical temperatures when extracted from the two order parameters, although the results coincide in the chiral limit. In this context, our results are consistent with the view in Ref. <xref ref-type="bibr" rid="c69">[69]</xref>, which suggests that different order parameters can yield significantly different pseudocritical temperatures. Adopting the susceptibility-peak definition of the transition temperature, we numerically verify that in all three holographic models the pseudocritical temperature obeys the universal scaling law <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>∼</mml:mo><mml:msubsup><mml:mi>m</mml:mi><mml:mi>q</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>β</mml:mi><mml:mi>δ</mml:mi></mml:mrow></mml:msubsup></mml:math></inline-formula> or <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo>∼</mml:mo><mml:msubsup><mml:mi>m</mml:mi><mml:mi>π</mml:mi><mml:mrow><mml:mn>2</mml:mn><mml:mo>/</mml:mo><mml:mi>β</mml:mi><mml:mi>δ</mml:mi></mml:mrow></mml:msubsup></mml:math></inline-formula>. The scaling region in these models can extend below the physical quark mass. These findings support the consistency of soft-wall models with mean-field universality. Moreover, we find that the percentage temperature defined by the 79% [the value is set by the ratio <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>χ</mml:mi></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:mn>0</mml:mn><mml:mo stretchy="false">)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>χ</mml:mi><mml:mo>,</mml:mo><mml:mi>max</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>], converges to its chiral-limit value much faster than the pseudocritical temperature, offering a practical observable for determining <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>.</p><p>While the three holographic models share identical critical exponents and scaling functions in the chiral limit, their scaling coefficients span orders of magnitude. Compared with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling from DSE <xref ref-type="bibr" rid="c9">[9]</xref>, FRG <xref ref-type="bibr" rid="c70">[70]</xref>, and lattice QCD <xref ref-type="bibr" rid="c16">[16]</xref>, models I and II yield a slope, i.e., the scaling coefficient, that is roughly one third as large, a discrepancy that appears to afflict earlier soft-wall constructions as well. It is interesting to see that by softening the scalar potential with certain logarithmic terms and <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-dependent coefficients, model III reproduces a <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling in quantitative agreement with the DSE results <xref ref-type="bibr" rid="c9">[9]</xref>. This improvement can be attributed to the logarithmic modification in the scalar potential. While models I and III are equivalent at the critical point (sharing the same subleading expansion), the logarithmic term in model III effectively incorporates higher-order interactions that become relevant for finite quark masses, driving the model toward better agreement with QCD phenomenology. These findings might offer valuable guidance for refining future model constructions in the soft-wall AdS/QCD. It is worth noting that due to the complexity of the numerical computations and the high dimensionality of the parameter space, this work does not present a single parameter set that simultaneously reproduces both the chiral condensate and the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>T</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:math></inline-formula> scaling with high precision. Nevertheless, we anticipate that future optimization strategies, such as those employing machine learning algorithms, will enable more refined fittings. Finally, in this study, we have restricted our attention to the two-flavor chiral critical point. Extending the analysis to the entire critical lines in the quark-mass phase diagram, and examining the resulting consequences for the critical end point within the same holographic framework, constitutes an interesting direction for future work.</p></sec></body><back><ack><title>ACKNOWLEDGMENTS</title><p>This work is supported by the National Natural Science Foundation of China under Grants No. 12275108 and No. 12235016.</p></ack><sec sec-type="data-availability"><title>DATA AVAILABILITY</title><p>The data that support the findings of this article are not publicly available. 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