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<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="1.3" xml:lang="en"><front><journal-meta><journal-id journal-id-type="publisher-id">cpc</journal-id><journal-title-group><journal-title xml:lang="en">Chinese Physics C</journal-title></journal-title-group><issn pub-type="ppub">1674-1137</issn><publisher><publisher-name>Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd
				</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">cpc_49_6_064101</article-id><article-id pub-id-type="doi">10.1088/1674-1137/adb385</article-id><article-id pub-id-type="manuscript">adb385</article-id><article-id custom-type="cstr" pub-id-type="custom">32044.14.ChinesePhysicsC.49064101</article-id><article-categories><subj-group subj-group-type="display-article-type"><subject>Paper</subject></subj-group><subj-group subj-group-type="section"><subject>Nuclear physics</subject></subj-group></article-categories><title-group><article-title>Probing the mass effect of heavy quark jets in high-energy nuclear collisions<xref ref-type="fn" rid="cpc_49_6_064101_fn1">*</xref>
               <fn id="cpc_49_6_064101_fn1"><label>*</label><p>Supported by the MajorProject of Basic and Applied Basic Research of Guangdong  Province, China (2020B0301030008, 2023A1515011460), and the National Natural Science Foundation of China (11935007, 12035007, 12247127, 12375137). Sa Wang is supported by the Open Foundation of Key Laboratory of Quark and Lepton Physics (MOE) (QLPL2023P01) and the Talent Scientific Star-up Foundation of the China Three Gorges University, China (CTGU) (2024RCKJ013)</p></fn>
            </article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wang</surname><given-names>Sa</given-names></name><name content-type="non-latin-no-space" name-style="eastern"><surname>王</surname><given-names>洒</given-names></name><xref ref-type="aff" rid="affiliation01">1</xref><xref ref-type="aff" rid="affiliation02">2</xref><xref ref-type="aff" rid="affiliation03">3</xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Li</surname><given-names>Shuang</given-names></name><name content-type="non-latin-no-space" name-style="eastern"><surname>李</surname><given-names>双</given-names></name><xref ref-type="aff" rid="affiliation01">1</xref><xref ref-type="aff" rid="affiliation02">2</xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Li</surname><given-names>Yao</given-names></name><name content-type="non-latin-no-space" name-style="eastern"><surname>李</surname><given-names>瑶</given-names></name><xref ref-type="aff" rid="affiliation03">3</xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zhang</surname><given-names>Ben-Wei</given-names></name><name content-type="non-latin-no-space" name-style="eastern"><surname>张</surname><given-names>本威</given-names></name><xref ref-type="aff" rid="affiliation03">3</xref><email>bwzhang@mail.ccnu.edu.cn</email></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wang</surname><given-names>Enke</given-names></name><name content-type="non-latin-no-space" name-style="eastern"><surname>王</surname><given-names>恩科</given-names></name><xref ref-type="aff" rid="affiliation04">4</xref></contrib><aff id="affiliation01">
               <label>1</label>
               <institution xlink:type="simple">College of Science, China Three Gorges University</institution>, Yichang 443002, <country>China</country>
            </aff><aff id="affiliation02">
               <label>2</label>
               <institution xlink:type="simple">Center for Astronomy and Space Sciences and Institute of Modern Physics, China Three Gorges University</institution>, Yichang 443002, <country>China</country>
            </aff><aff id="affiliation03">
               <label>3</label>
               <institution xlink:type="simple">Key Laboratory of Quark &amp; Lepton Physics (MOE) and Institute of Particle Physics, Central China Normal University</institution>, Wuhan 430079, <country>China</country>
            </aff><aff id="affiliation04">
               <label>4</label>
               <institution xlink:type="simple">Guangdong-Hong Kong Joint Laboratory of Quantum Matter, Guangdong Provincial Key Laboratory of Nuclear Science, Southern Nuclear Science Computing Center, South China Normal University</institution>, Guangzhou 510006, <country>China</country>
            </aff></contrib-group><pub-date pub-type="ppub"><day>01</day><month>6</month><year>2025</year></pub-date><pub-date pub-type="open-access"><day>7</day><month>2</month><year>2025</year></pub-date><volume>49</volume><issue>6</issue><elocation-id content-type="artnum">064101</elocation-id><history><date date-type="received"><day>13</day><month>11</month><year>2024</year></date><date date-type="published-online"><day>7</day><month>2</month><year>2025</year></date><date date-type="oa-requested"><day>13</day><month>11</month><year>2024</year></date></history><permissions><copyright-statement>© 2025 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd</copyright-statement><copyright-year>2025</copyright-year><license xlink:href="http://creativecommons.org/licenses/by/3.0/" license-type="cc-by" xlink:type="simple"><license-p>
                  <graphic xlink:href="cpc_49_6_064101_ccby.tif" content-type="online" orientation="portrait" position="float" xlink:type="simple"/>Content from this work may be used under the terms of the <ext-link xlink:href="http://creativecommons.org/licenses/by/3.0" ext-link-type="uri" xlink:type="simple">Creative Commons Attribution 3.0 licence</ext-link>. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Article funded by SCOAP<sup>3</sup> and published under licence by Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd
</license-p></license></permissions><self-uri xlink:href="cpc_49_6_064101.pdf" content-type="pdf" xlink:type="simple"/><abstract><title>Abstract</title><p>The production of heavy-quark (HQ) jets is a new area that addresses the mass effect of jet quenching in heavy-ion physics. This paper presents a theoretical study of HQ jet yield suppression in Pb+Pb collisions at the Large Hadron Collider (LHC) and focuses on the energy loss of HQ jets produced by different mechanisms. The <italic toggle="yes">p+p</italic> baseline is provided by the generator simulation of high-energy reactions of particles (SHERPA), and the jet-medium interactions are described by the SHELL transport model, which considers the elastic and inelastic partonic energy loss in the quark-gluon plasma (QGP). In <italic toggle="yes">p+p</italic> collisions, our numerical results indicate that the HQ jets from gluon splitting (<inline-formula>
                  <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M1.jpg" xlink:type="simple"/>
               </inline-formula>-jet) are the dominant contribution at high <inline-formula>
                  <tex-math><?CDATA $ p_T $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M2.jpg" xlink:type="simple"/>
               </inline-formula>, displaying more dispersive structures than the HQ-initiated (<inline-formula>
                  <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M3.jpg" xlink:type="simple"/>
               </inline-formula>-jet). In nucleus-nucleus collisions, our calculations were consistent with the inclusive and b-jet <inline-formula>
                  <tex-math><?CDATA $ R_{AA} $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M4.jpg" xlink:type="simple"/>
               </inline-formula> recently measured by the ATLAS collaboration, revealing a remarkable manifestation of the mass effect of jet energy loss. As a result of the dispersive substructure, the <inline-formula>
                  <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M5.jpg" xlink:type="simple"/>
               </inline-formula>-jet loses more energy than the <inline-formula>
                  <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M6.jpg" xlink:type="simple"/>
               </inline-formula>-jet in the QGP. Due to the significant contribution of <inline-formula>
                  <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M7.jpg" xlink:type="simple"/>
               </inline-formula>-jet, the <inline-formula>
                  <tex-math><?CDATA $ R_{AA} $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M8.jpg" xlink:type="simple"/>
               </inline-formula> of <italic toggle="yes">c</italic>-jet is comparable or even smaller than that of inclusive jet. To experimentally distinguish the <inline-formula>
                  <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M9.jpg" xlink:type="simple"/>
               </inline-formula>-jet and <inline-formula>
                  <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M10.jpg" xlink:type="simple"/>
               </inline-formula>-jet, we propose event selection strategies based on their topological features and test their performances. By isolating the <inline-formula>
                  <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M11.jpg" xlink:type="simple"/>
               </inline-formula>-jet, <inline-formula>
                  <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M12.jpg" xlink:type="simple"/>
               </inline-formula>-jet, and the jets initiated by heavy quarks, we predicted that the order of their <inline-formula>
                  <tex-math><?CDATA $ R_{AA} $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M13.jpg" xlink:type="simple"/>
               </inline-formula> are in line with the mass hierarchy of energy loss. Future measurements on the <inline-formula>
                  <tex-math><?CDATA $ R_{AA} $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M14.jpg" xlink:type="simple"/>
               </inline-formula> of <inline-formula>
                  <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M15.jpg" xlink:type="simple"/>
               </inline-formula>-jet and <inline-formula>
                  <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
                  <inline-graphic xlink:href="cpc_49_6_064101_M16.jpg" xlink:type="simple"/>
               </inline-formula>-jet will provide a unique opportunity for testing the flavor/mass dependence of energy loss at the jet level.</p></abstract><kwd-group kwd-group-type="author"><kwd>heavy-ion collisions</kwd><kwd>quark-gluon plasma</kwd><kwd>jet quenching</kwd><kwd>heavy quark jet</kwd><kwd>energy loss</kwd></kwd-group><kwd-group kwd-group-type="author-pacs"><kwd>25.75.Ld</kwd><kwd>25.75.Gz</kwd><kwd>24.10.Nz</kwd></kwd-group><funding-group><open-access><p content-type="scoap3">Article funded by SCOAP<sup>3</sup>
               </p></open-access></funding-group><counts><page-count count="11"/></counts></article-meta></front><body><sec id="cpc_49_6_064101_s01"><label>I.</label><title>INTRODUCTION</title><p>High-energy nuclear collisions at the Relativistic Heavy Ion Collider (RHIC) and Large Hadron Collider (LHC) provide an excellent opportunity for unraveling the mysteries of the quark-gluon plasma (QGP), a new state of nuclear matter formed at extremely high temperatures and densities. The "jet quenching" effect, referring to the energy attenuation of fast partons due to their strong interactions with the constituents of the QGP medium, has piqued the interest of physicists who have studied them extensively [<xref ref-type="bibr" rid="cpc_49_6_064101_bib1">1</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib21">21</xref>]. Investigations of the jet quenching phenomenon have deepened our understanding of the quantum chromodynamics (QCD) under extreme conditions and revealed the properties of the strongly-coupled nuclear matter [<xref ref-type="bibr" rid="cpc_49_6_064101_bib22">22</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib24">24</xref>].</p><p>As a result of the large mass (<inline-formula>
               <tex-math><?CDATA $M_Q\gg\Lambda_{\rm QCD}$?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M17.jpg" xlink:type="simple"/>
            </inline-formula>), heavy quarks (HQ) are powerful hard probes for exploring the transport properties of the QGP [<xref ref-type="bibr" rid="cpc_49_6_064101_bib25">25</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib30">30</xref>]. Over the past two decades, measurements on the nuclear modification factor <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M18.jpg" xlink:type="simple"/>
            </inline-formula> [<xref ref-type="bibr" rid="cpc_49_6_064101_bib31">31</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib34">34</xref>] and collective flow <inline-formula>
               <tex-math><?CDATA $ v_n $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M19.jpg" xlink:type="simple"/>
            </inline-formula> [<xref ref-type="bibr" rid="cpc_49_6_064101_bib35">35</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib38">38</xref>] of heavy-flavor hadrons have enriched our knowledge with regard to the energy loss mechanisms and hadronization patterns of heavy quarks in high-energy heavy-ion collisions. Because of the "dead-cone" effect [<xref ref-type="bibr" rid="cpc_49_6_064101_bib39">39</xref>], heavy quarks lose less energy than the massless light partons [<xref ref-type="bibr" rid="cpc_49_6_064101_bib40">40</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib42">42</xref>]. By comparing the <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M20.jpg" xlink:type="simple"/>
            </inline-formula> of heavy-flavor hadrons [<xref ref-type="bibr" rid="cpc_49_6_064101_bib43">43</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib46">46</xref>] and their decayed leptons [<xref ref-type="bibr" rid="cpc_49_6_064101_bib47">47</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib49">49</xref>] with those of light-flavor ones,  evidence of the mass effect has been partly addressed [<xref ref-type="bibr" rid="cpc_49_6_064101_bib50">50</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib52">52</xref>].</p><p>The HQ jets, defined as jets containing heavy-flavor quarks/hadrons [<xref ref-type="bibr" rid="cpc_49_6_064101_bib53">53</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib54">54</xref>], are also excellent tools for capturing the mass effect of energy loss at the jet level [<xref ref-type="bibr" rid="cpc_49_6_064101_bib55">55</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib63">63</xref>]. The richer inner structure of HQ jets compared to that of single particles provides a unique opportunity for exploring the exquisite interaction mechanisms between the hard parton and the medium. The investigation of the production mechanisms and substructures of HQ jets has also attracted much attention both experimentally [<xref ref-type="bibr" rid="cpc_49_6_064101_bib64">64</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib71">71</xref>] and theoretically [<xref ref-type="bibr" rid="cpc_49_6_064101_bib72">72</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib81">81</xref>]. The recent measurements on the jet radial profile [<xref ref-type="bibr" rid="cpc_49_6_064101_bib64">64</xref>] and jet shape by the Compact Muon Solenoid (CMS) collaboration [<xref ref-type="bibr" rid="cpc_49_6_064101_bib69">69</xref>] imply that the HQ jets produced by different mechanisms may exhibit distinct topologies and structures [<xref ref-type="bibr" rid="cpc_49_6_064101_bib82">82</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib83">83</xref>]. In this context, it would be of great interest to explore the energy loss effect of HQ jets produced by different channels and their relation to their substructures. Note that the HQ jet samples selected in the experiment included the jets initiated by heavy quarks (<inline-formula>
               <tex-math><?CDATA $ Q\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M21.jpg" xlink:type="simple"/>
            </inline-formula>-jet) and a considerable contribution from the gluon splitting (<inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M22.jpg" xlink:type="simple"/>
            </inline-formula>-jet). The former is initiated by a heavy quark created in the early stages of the QCD hard scattering, whereas the latter can be produced by the splitting of a high-energy gluon (<inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q\bar{Q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M23.jpg" xlink:type="simple"/>
            </inline-formula>) during the parton shower. However, experimentally comparing the mass effect of the jet energy loss of the HQ-initiated jet with that of the massless one is challenging. Suitable selection strategies can be explored to isolate the HQ jets produced by different production mechanisms, to enable a direct comparison of the yield suppression of the HQ-initiated jets with that of the light-flavor ones.</p><p>In this study, the yield suppression of HQ jets in heavy-ion collisions was explored to address the mass effect of jet energy loss. At first, the fractional contributions from different production mechanisms to the HQ jet yields in p+p collisions was estimated, further discussing their main characteristics in the jet substructure. In nucleus-nucleus collisions, we systematically estimated the fractional contribution and energy loss of HQ jets from <inline-formula>
               <tex-math><?CDATA $ Q\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M24.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M25.jpg" xlink:type="simple"/>
            </inline-formula>-jet, demonstrating that a significant contribution of <inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M26.jpg" xlink:type="simple"/>
            </inline-formula>-jet and its dispersive jet substructure \lead to a comparable <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M27.jpg" xlink:type="simple"/>
            </inline-formula> of the c-jet relative to the inclusive jet. Furthermore, to realize the separation of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M28.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M29.jpg" xlink:type="simple"/>
            </inline-formula>-jet in experimental measurements, strategies are proposed to distinguish them based on their topological features. By comparing the yield suppression of the select <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M30.jpg" xlink:type="simple"/>
            </inline-formula>-jet sample with that of the inclusive jet, we show that the mass hierarchy of energy loss (<inline-formula>
               <tex-math><?CDATA $ \Delta E_{\rm incl-jet} \gt \Delta E_{\rm c-jet} \gt \Delta E_{\rm b-jet} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M31.jpg" xlink:type="simple"/>
            </inline-formula>) at the jet level holds true.</p><p>The remainder of this paper is organized as follows. In Sec. II, the mechanisms of producing HQ jets in <italic toggle="yes">p+p</italic> collisions is presented. In Sec. III, the theoretical framework of the transport model used to study the medium modifications of the HQ jet is introduced. In Sec. IV, the main results and  specific discussions are provided. Finally, the work is summarized in Sec. IV.</p></sec><sec id="cpc_49_6_064101_s02"><label>II.</label><title>HEAVY QUARK JET PRODUCTION IN <italic toggle="yes">P+P</italic> COLLISIONS</title><p>Production of open heavy flavors in hadron collisions has been studied over the past decades using various theoretical schemes [<xref ref-type="bibr" rid="cpc_49_6_064101_bib84">84</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib89">89</xref>]. <xref ref-type="fig" rid="cpc_49_6_064101_f1">Fig. 1 </xref>displays  the typical QCD Feynman diagrams contributing to the production of HQ jets, which are usually categorized into three classes: flavor creation (FCR), flavor excitation (FEX), and gluon splitting (GSP) [<xref ref-type="bibr" rid="cpc_49_6_064101_bib82">82</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib83">83</xref>]. The first two represent the pair creation of heavy quarks in hard scattering at leading order, in which the incoming partons are light quarks or gluons, and the outcoming <inline-formula>
               <tex-math><?CDATA $ Q\bar{Q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M32.jpg" xlink:type="simple"/>
            </inline-formula> pairs usually emerge back-to-back in azimuth. Higher-order QCD processes of heavy quark production are not negligible in hadron collisions at the LHC energy. Diagrams 1(c) and 1(d) represent the FCR processes at next-to-leading order (NLO) with an extra radiated gluon in the final state. <xref ref-type="fig" rid="cpc_49_6_064101_f1">Fig. 1</xref>(e)  depicts the typical FEX process, in which a heavy quark from the parton distribution function of one incoming proton is excited in hard scattering by a light parton of another proton. The most distinct feature of FEX compared to FCR is that only one heavy quark is produced by the hard scattering. The last diagram in <xref ref-type="fig" rid="cpc_49_6_064101_f1">Fig. 1</xref> depicts the splitting process of a final-state hard gluon during the parton shower, whereby in general, <inline-formula>
               <tex-math><?CDATA $ Q\bar{Q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M33.jpg" xlink:type="simple"/>
            </inline-formula> pairs are produced with a smaller opening angle in azimuth compared to that of FCR. The prior clarification of the different kinematics features of these subprocesses may help us understand the  corresponding substructures and topological features of HQ jets.</p><fig id="cpc_49_6_064101_f1" orientation="portrait" position="float"><label>Fig. 1</label><caption id="cpc_49_6_064101_fc1"><p>(color online) Typical examples of QCD Feynman diagrams contributing to the production of HQ jets. Flavor creation: (a, b) LO; (c, d) NLO; (e) Flavor excitation; (f) Gluon splitting. Red fermion lines denote the produced heavy quarks.</p></caption><graphic xlink:href="cpc_49_6_064101_f1.eps" content-type="print" id="cpc_49_6_064101_f1_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f1.jpg" content-type="online" id="cpc_49_6_064101_f1_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>In this study, we employed the Monte Carlo event generator simulation of high-energy reactions of particles (SHERPA) [<xref ref-type="bibr" rid="cpc_49_6_064101_bib90">90</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib91">91</xref>] to compute the initial HQ jet production in <italic toggle="yes">p+p</italic> collisions, which matches that of the hard QCD processes at next-to-leading order with the vacuum parton shower effect (NLO+PS). The resummation of the parton shower based on Catani-Seymour subtraction method [<xref ref-type="bibr" rid="cpc_49_6_064101_bib92">92</xref>] is merged with fixed-order NLO calculations based on the MC@NLO prescription [<xref ref-type="bibr" rid="cpc_49_6_064101_bib93">93</xref>]. The NNPDF 3.0 [<xref ref-type="bibr" rid="cpc_49_6_064101_bib94">94</xref>] parton distribution functions (PDFs) were chosen for the SHERPA calculations. In the upper panel of <xref ref-type="fig" rid="cpc_49_6_064101_f2">Fig. 2</xref>, the calculated differential cross section of the <inline-formula>
               <tex-math><?CDATA $ D^0 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M34.jpg" xlink:type="simple"/>
            </inline-formula> meson tagged-jet by SHERPA in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M35.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV are compared with a large ion collider experiment (ALICE) data [<xref ref-type="bibr" rid="cpc_49_6_064101_bib95">95</xref>]. The charged jets are reconstructed by using the Fastjet program [<xref ref-type="bibr" rid="cpc_49_6_064101_bib96">96</xref>] with anti-<inline-formula>
               <tex-math><?CDATA $ k_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M36.jpg" xlink:type="simple"/>
            </inline-formula> algorithm [<xref ref-type="bibr" rid="cpc_49_6_064101_bib97">97</xref>] at <italic toggle="yes">R</italic> = 0.2, 0.4, 0.6 and rapidity range <inline-formula>
               <tex-math><?CDATA $ |\eta^{\rm jet}| \lt 0.9-R $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M37.jpg" xlink:type="simple"/>
            </inline-formula>. The <inline-formula>
               <tex-math><?CDATA $ D^0 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M38.jpg" xlink:type="simple"/>
            </inline-formula> mesons are required to have 2<inline-formula>
               <tex-math><?CDATA $ \lt p_T^{D} \lt $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M39.jpg" xlink:type="simple"/>
            </inline-formula> 36 GeV. In the lower panel of <xref ref-type="fig" rid="cpc_49_6_064101_f2">Fig. 2</xref>, the yield of <italic toggle="yes">
               <underline>b</underline>
            </italic>-jet in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s}= 5.02 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M40.jpg" xlink:type="simple"/>
            </inline-formula> TeV compared with a toroidal LHC apparatus (ATLAS) and ALICE data [<xref ref-type="bibr" rid="cpc_49_6_064101_bib59">59</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib98">98</xref>]. For the ATLAS measurement, the <italic toggle="yes">b</italic>-jets were constructed using the anti-<inline-formula>
               <tex-math><?CDATA $ k_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M41.jpg" xlink:type="simple"/>
            </inline-formula> jet algorithm for <inline-formula>
               <tex-math><?CDATA $ R=0.2 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M42.jpg" xlink:type="simple"/>
            </inline-formula> and <inline-formula>
               <tex-math><?CDATA $ R=0.4 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M43.jpg" xlink:type="simple"/>
            </inline-formula> within <inline-formula>
               <tex-math><?CDATA $ |y_{\rm jet}| \lt 2.1 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M44.jpg" xlink:type="simple"/>
            </inline-formula>. As for the ALICE data, the <italic toggle="yes">b</italic>-jet were constructed using charged particles with <inline-formula>
               <tex-math><?CDATA $ R=0.4 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M45.jpg" xlink:type="simple"/>
            </inline-formula> within <inline-formula>
               <tex-math><?CDATA $ |\eta_{\rm jet}| \lt 0.5 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M46.jpg" xlink:type="simple"/>
            </inline-formula>. The calculations by SHERPA are consistent with the experimental measurements of the HQ jet yields both for <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet, establishing a good baseline for subsequent studies of nuclear modifications.</p><fig id="cpc_49_6_064101_f2" orientation="portrait" position="float"><label>Fig. 2</label><caption id="cpc_49_6_064101_fc2"><p>(color online) Upper panel: differential cross sections of the <inline-formula>
                     <tex-math><?CDATA $ D^0 $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M47.jpg" xlink:type="simple"/>
                  </inline-formula> meson tagged-jet by SHERPA in p+p collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M48.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV compared with the ALICE data [<xref ref-type="bibr" rid="cpc_49_6_064101_bib95">95</xref>], at <italic toggle="yes">R</italic> = 0.2, 0.4, 0.6. Lower panel: differential cross section of <italic toggle="yes">b</italic>-jet in p+p collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M49.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV compared with ALICE [<xref ref-type="bibr" rid="cpc_49_6_064101_bib98">98</xref>] and ATLAS [<xref ref-type="bibr" rid="cpc_49_6_064101_bib59">59</xref>] data.</p></caption><graphic xlink:href="cpc_49_6_064101_f2.eps" content-type="print" id="cpc_49_6_064101_f2_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f2.jpg" content-type="online" id="cpc_49_6_064101_f2_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>In Monte Carlo simulations, the three mechanisms mentioned in <xref ref-type="fig" rid="cpc_49_6_064101_f1">Fig. 1</xref> can be distinguished based on their topological features. The events that produce one and two heavy quarks in the hard processes can be categorized into FEX and FCR, respectively. In contrast, the events for the HQ jet created only in the parton shower stage are regarded as the GSP type. As shown in <xref ref-type="fig" rid="cpc_49_6_064101_f3">Fig. 3</xref>, the fractional contributions of the three mechanisms to the total yield was estimated as a function of jet <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M50.jpg" xlink:type="simple"/>
            </inline-formula> for both <italic toggle="yes">c</italic>-jet (upper) and <italic toggle="yes">b</italic>-jet (lower) in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M51.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV. At <inline-formula>
               <tex-math><?CDATA $ 12 \lt p_T \lt 400 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M52.jpg" xlink:type="simple"/>
            </inline-formula> GeV, The proportions of GSP increase with jet <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M53.jpg" xlink:type="simple"/>
            </inline-formula> and eventually become the most dominant mechanism for both <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet production, which is consistent with the estimation in [<xref ref-type="bibr" rid="cpc_49_6_064101_bib83">83</xref>]. For <italic toggle="yes">c</italic>-jet, at lower <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M54.jpg" xlink:type="simple"/>
            </inline-formula> the contributions of these three mechanisms are nonnegligible. As for <italic toggle="yes">b</italic>-jet, at lower <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M55.jpg" xlink:type="simple"/>
            </inline-formula>, the most important contributioons (above 50<inline-formula>
               <tex-math><?CDATA $ \% $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M56.jpg" xlink:type="simple"/>
            </inline-formula>) are from the FEX mechanism, in contrast to the GSP contributing less than <inline-formula>
               <tex-math><?CDATA $ 20\% $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M57.jpg" xlink:type="simple"/>
            </inline-formula>. FCR and FEX denote the jets initiated by heavy quarks, whereas GSP corresponds to HQ jets initiated by high-energy gluon. Focusing on their essential differences makes it convenient to categorize these three mechanisms into two subprocesses, <inline-formula>
               <tex-math><?CDATA $ Q\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M58.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M59.jpg" xlink:type="simple"/>
            </inline-formula>-jet, in the remainder of this paper.</p><fig id="cpc_49_6_064101_f3" orientation="portrait" position="float"><label>Fig. 3</label><caption id="cpc_49_6_064101_fc3"><p>(color online) The fractional contributions of the three production mechanisms to the total HQ jet differential cross section as functions of jet <inline-formula>
                     <tex-math><?CDATA $ p_T $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M60.jpg" xlink:type="simple"/>
                  </inline-formula> in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M61.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV for <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet.</p></caption><graphic xlink:href="cpc_49_6_064101_f3.eps" content-type="print" id="cpc_49_6_064101_f3_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f3.jpg" content-type="online" id="cpc_49_6_064101_f3_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>To inuitibely show the essential differences of <inline-formula>
               <tex-math><?CDATA $ Q\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M62.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M63.jpg" xlink:type="simple"/>
            </inline-formula>-jet in substructures,  two-dimensional (<inline-formula>
               <tex-math><?CDATA $ z_Q, r_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M64.jpg" xlink:type="simple"/>
            </inline-formula>) diagrams of these two types of jets are plotted in <xref ref-type="fig" rid="cpc_49_6_064101_f4">Figs. 4</xref> and <xref ref-type="fig" rid="cpc_49_6_064101_f5">5</xref> in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M65.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV for both <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet. Here <inline-formula>
               <tex-math><?CDATA $ z_Q=p_T^Q/p_T^{\rm jet} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M66.jpg" xlink:type="simple"/>
            </inline-formula> denotes the transverse momentum fraction carried by heavy quarks in jets, and <inline-formula>
               <tex-math><?CDATA $ r_Q=\sqrt{(\phi_Q-\phi_{\rm jet})^2+(\eta_Q-\eta_{\rm jet})^2} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M67.jpg" xlink:type="simple"/>
            </inline-formula> is the radial distance of heavy quarks to the jet axis. The two observables, <inline-formula>
               <tex-math><?CDATA $ z_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M68.jpg" xlink:type="simple"/>
            </inline-formula> and <inline-formula>
               <tex-math><?CDATA $ r_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M69.jpg" xlink:type="simple"/>
            </inline-formula>, quantify the energy dominance of heavy quarks in jets and their angular location in the jet cone. For <inline-formula>
               <tex-math><?CDATA $ Q\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M70.jpg" xlink:type="simple"/>
            </inline-formula>-jet of both <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet, the most heavy quarks carry above <inline-formula>
               <tex-math><?CDATA $ 80\% $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M71.jpg" xlink:type="simple"/>
            </inline-formula> of the jet momentum; and their moving directions collimate with the jet axis. Understandably, heavy quarks still dominate the jet's momentum even after soft shower evolution. However, the situation is quite different for the <inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M72.jpg" xlink:type="simple"/>
            </inline-formula>-jet in the lower panels, where heavy quarks are more dispersed in the (<inline-formula>
               <tex-math><?CDATA $ z_Q, r_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M73.jpg" xlink:type="simple"/>
            </inline-formula>) diagrams. We observe a banded region, especially for the <inline-formula>
               <tex-math><?CDATA $ g\rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M74.jpg" xlink:type="simple"/>
            </inline-formula>-jet, which is distinctly different from that of <inline-formula>
               <tex-math><?CDATA $ c\rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M75.jpg" xlink:type="simple"/>
            </inline-formula>-jet. Plenty of heavy quarks produced by the gluon splitting carry smaller energy fractions and are located in larger radii in jets. In the remainder of this paper, we show that the large fraction of <inline-formula>
               <tex-math><?CDATA $ g\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M76.jpg" xlink:type="simple"/>
            </inline-formula>-jet and its distinct substructure compared to <inline-formula>
               <tex-math><?CDATA $ Q\rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M77.jpg" xlink:type="simple"/>
            </inline-formula>-jet play critical roles in the energy loss and yield suppression of HQ jets in high-energy nucleus-nucleus collisions.</p><fig id="cpc_49_6_064101_f4" orientation="portrait" position="float"><label>Fig. 4</label><caption id="cpc_49_6_064101_fc4"><p>(color online) Two-dimensional (<inline-formula>
                     <tex-math><?CDATA $ z_Q,r_Q $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M78.jpg" xlink:type="simple"/>
                  </inline-formula>) correlation diagrams of <inline-formula>
                     <tex-math><?CDATA $ c\rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M79.jpg" xlink:type="simple"/>
                  </inline-formula>-jet (upper panel) and <inline-formula>
                     <tex-math><?CDATA $ b\rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M80.jpg" xlink:type="simple"/>
                  </inline-formula>-jet (lower panel) in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M81.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV.</p></caption><graphic xlink:href="cpc_49_6_064101_f4.eps" content-type="print" id="cpc_49_6_064101_f4_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f4.jpg" content-type="online" id="cpc_49_6_064101_f4_online" orientation="portrait" position="float" xlink:type="simple"/></fig><fig id="cpc_49_6_064101_f5" orientation="portrait" position="float"><label>Fig. 5</label><caption id="cpc_49_6_064101_fc5"><p>(color online) Two-dimensional (<inline-formula>
                     <tex-math><?CDATA $ z_Q,r_Q $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M82.jpg" xlink:type="simple"/>
                  </inline-formula>) correlation diagrams of <inline-formula>
                     <tex-math><?CDATA $ g\rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M83.jpg" xlink:type="simple"/>
                  </inline-formula>-jet (upper panel) and <inline-formula>
                     <tex-math><?CDATA $ g\rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M84.jpg" xlink:type="simple"/>
                  </inline-formula>-jet (lower panel) in p+p collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M85.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV.</p></caption><graphic xlink:href="cpc_49_6_064101_f5.eps" content-type="print" id="cpc_49_6_064101_f5_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f5.jpg" content-type="online" id="cpc_49_6_064101_f5_online" orientation="portrait" position="float" xlink:type="simple"/></fig></sec><sec id="cpc_49_6_064101_s03"><label>III.</label><title>JET TRANSPORT IN THE QUARK-GLUON PLASMA</title><p>Because of the large mass (<inline-formula>
               <tex-math><?CDATA $ M_Q\gg T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M86.jpg" xlink:type="simple"/>
            </inline-formula>), the heavy quarks are effective hard probes for the properties of the hot and dense QCD matter formed in high-energy nuclear collisions. In this study, we utilized the <italic toggle="yes">p+p</italic> events produced by SHERPA as input of the transport model driven by the modified Langevin equations [<xref ref-type="bibr" rid="cpc_49_6_064101_bib99">99</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib104">104</xref>] to estimate the nuclear modification effect of the HQ jet production in <italic toggle="yes">A+A</italic> collisions.</p><p>
            <disp-formula>
               <label>1</label>
               <tex-math id="cpc_49_6_064101_E1"> <?CDATA $ {\rm d}x_j=\dfrac{p_j}{E}{\rm d} t, $?> </tex-math>
               <graphic xlink:href="cpc_49_6_064101_E1.jpg" orientation="portrait" position="float" xlink:type="simple"/>
            </disp-formula>
         </p><p>
            <disp-formula>
               <label>2</label>
               <tex-math id="cpc_49_6_064101_E2"> <?CDATA $ {\rm d}p_j=-\Gamma p_j{\rm d} t+\sqrt{{\rm d} t}C_{jk}(|\boldsymbol{p}+\xi{\rm d}\boldsymbol{p}|)\rho_k-p^{\rm g}_j .$?> </tex-math>
               <graphic xlink:href="cpc_49_6_064101_E2.jpg" orientation="portrait" position="float" xlink:type="simple"/>
            </disp-formula>
         </p><p>The spatial position update of the traversing heavy quarks in the medium is described in Eq. (1), where <inline-formula>
               <tex-math><?CDATA $ {\rm d} t=0.1 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M87.jpg" xlink:type="simple"/>
            </inline-formula>, and  fm is the time step of our simulation. Meanwhile, Eq. (2) expresses the in-medium energy loss with index <inline-formula>
               <tex-math><?CDATA $ j, k=1,2,3 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M88.jpg" xlink:type="simple"/>
            </inline-formula>, where the three terms on the right-hand side denote the drag,  thermal stochastic, and radiative correction terms, respectively. The drag term represents the collisional energy loss of heavy quarks, with the drag coefficient Γ controlling the strength of the energy loss. The thermal stochastic term indicates the mass of random kicks that heavy quarks suffer, caused by the thermal quasi-particles in the hot and dense QCD matter, where the white <inline-formula>
               <tex-math><?CDATA $ \rho_k $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M89.jpg" xlink:type="simple"/>
            </inline-formula> obeys the standard normal distribution, and <inline-formula>
               <tex-math><?CDATA $ P({\rho})=(2\pi)^{-3/2}{\rm e}^{\rho^2/2} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M90.jpg" xlink:type="simple"/>
            </inline-formula>. The momentum argument of the covariance matrix <inline-formula>
               <tex-math><?CDATA $ C_{jk} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M91.jpg" xlink:type="simple"/>
            </inline-formula> is a function of the momentum diffusion coefficients in the longitudinal (<inline-formula>
               <tex-math><?CDATA $ \kappa_{||} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M92.jpg" xlink:type="simple"/>
            </inline-formula>) and transverse (<inline-formula>
               <tex-math><?CDATA $ \kappa_{\perp} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M93.jpg" xlink:type="simple"/>
            </inline-formula>) directions [<xref ref-type="bibr" rid="cpc_49_6_064101_bib105">105</xref>].</p><p>
            <disp-formula>
               <label>3</label>
               <tex-math id="cpc_49_6_064101_E3"> <?CDATA $ C_{jk}=\sqrt{\kappa_{||}}\frac{p_jp_k}{\vec{p}^{\, 2}}+\sqrt{\kappa_{\perp}}\left(\delta_{jk}-\frac{p_jp_k}{\vec{p}^{\, 2}}\right). $?> </tex-math>
               <graphic xlink:href="cpc_49_6_064101_E3.jpg" orientation="portrait" position="float" xlink:type="simple"/>
            </disp-formula>
         </p><p>Note here we chose <inline-formula>
               <tex-math><?CDATA $ \xi=0 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M94.jpg" xlink:type="simple"/>
            </inline-formula> for the pre-point (Ito) realization of the stochastic integral of <inline-formula>
               <tex-math><?CDATA $C_{jk}(|\boldsymbol{p}+\xi{\rm d}\boldsymbol{p}|)$?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M95.jpg" xlink:type="simple"/>
            </inline-formula> [<xref ref-type="bibr" rid="cpc_49_6_064101_bib106">106</xref>]. Additionally, by assuming <italic toggle="yes">κ</italic> is isotropic for heavy quarks <inline-formula>
               <tex-math><?CDATA $ \kappa_{\perp}=\kappa_{||}=\kappa $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M96.jpg" xlink:type="simple"/>
            </inline-formula>, a simple expression <inline-formula>
               <tex-math><?CDATA $ C_{jk}=\sqrt{\kappa}\delta_{jk} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M97.jpg" xlink:type="simple"/>
            </inline-formula>can be obtained. Then the momentum diffusion coefficient <italic toggle="yes">κ</italic> can be related to the drag coefficient Γ by the relativistic Einstein relation <inline-formula>
               <tex-math><?CDATA $ \Gamma=\kappa/2ET $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M98.jpg" xlink:type="simple"/>
            </inline-formula>. Note that the momentum diffusion coefficient <italic toggle="yes">κ</italic> of heavy quarks can also be converted into another dimensionless form <inline-formula>
               <tex-math><?CDATA $ 2\pi TD_s $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M99.jpg" xlink:type="simple"/>
            </inline-formula> in coordinate space using the relation <inline-formula>
               <tex-math><?CDATA $ D_s=2T^2/\kappa $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M100.jpg" xlink:type="simple"/>
            </inline-formula>. Note that, to accurately determine the temperature and momentum dependence of the diffusion coefficient of heavy quarks (<italic toggle="yes">κ</italic> or <inline-formula>
               <tex-math><?CDATA $ D_s $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M101.jpg" xlink:type="simple"/>
            </inline-formula>), the heavy-ion community has  made some elaborate and sgnificant efforts in recent years [<xref ref-type="bibr" rid="cpc_49_6_064101_bib107">107</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib111">111</xref>]. More detailed reviews can be found in [<xref ref-type="bibr" rid="cpc_49_6_064101_bib112">112</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib113">113</xref>]. At each time step, the heavy quarks are boosted into the local rest frame of the expanding medium to update the four-momentum using the Lorentz transformation, boosting them back again to the laboratory frame to update the spatial position. The last correction term <inline-formula>
               <tex-math><?CDATA $ -p^g_j $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M102.jpg" xlink:type="simple"/>
            </inline-formula> corresponds to the momentum recoil of the medium-induced radiated gluon, based on the gluon spectrum calculated by the higher-twist approach [<xref ref-type="bibr" rid="cpc_49_6_064101_bib40">40</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib114">114</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib116">116</xref>],</p><p>
            <disp-formula>
               <label>4</label>
               <tex-math id="cpc_49_6_064101_E4"> <?CDATA $ \frac{{\rm d}N}{ {\rm d}x{\rm d}k^{2}_{\perp}{\rm d}t}=\frac{2\alpha_{s}C_sP\left(x\right)\hat{q}}{\pi k^{4}_{\perp}}\sin^2\left(\frac{t-t_i}{2\tau_f}\right)\left(\frac{k^2_{\perp}}{k^2_{\perp}+x^2M^2}\right)^4, $?> </tex-math>
               <graphic xlink:href="cpc_49_6_064101_E4.jpg" orientation="portrait" position="float" xlink:type="simple"/>
            </disp-formula>
         </p><p>where <italic toggle="yes">x</italic> and <inline-formula>
               <tex-math><?CDATA $ k_\perp $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M103.jpg" xlink:type="simple"/>
            </inline-formula> are the energy fraction and  transverse momentum carried by the radiated gluon. <inline-formula>
               <tex-math><?CDATA $ C_s $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M104.jpg" xlink:type="simple"/>
            </inline-formula> is the quadratic Casimir in the color representation, and <inline-formula>
               <tex-math><?CDATA $ P(x) $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M105.jpg" xlink:type="simple"/>
            </inline-formula> the splitting function; <inline-formula>
               <tex-math><?CDATA $ \tau_f=2Ex(1-x)/(k^2_\perp+x^2M^2) $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M106.jpg" xlink:type="simple"/>
            </inline-formula> denotes the gluon formation time to take into account the Landau-Pomeranchuk-Migdal (LPM) effects [<xref ref-type="bibr" rid="cpc_49_6_064101_bib117">117</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib118">118</xref>]. <inline-formula>
               <tex-math><?CDATA $\hat{q}=q_0 (T/T_0)^3 \cdot p_{\mu}u^{\mu}/E$?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M107.jpg" xlink:type="simple"/>
            </inline-formula> is the jet transport parameter [<xref ref-type="bibr" rid="cpc_49_6_064101_bib119">119</xref>], where <inline-formula>
               <tex-math><?CDATA $ T_0 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M108.jpg" xlink:type="simple"/>
            </inline-formula> is the highest temperature in the most central <italic toggle="yes">A+A</italic> collisions, and <inline-formula>
               <tex-math><?CDATA $ u^{\mu} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M109.jpg" xlink:type="simple"/>
            </inline-formula> the velocity of the medium cell where the heavy quark is located. In considering the fluctuation of medium-induced gluon radiation, we assumed that the number of the radiated gluon during a time step <inline-formula>
               <tex-math><?CDATA $ \Delta t $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M110.jpg" xlink:type="simple"/>
            </inline-formula> obeys the Possion distribution <inline-formula>
               <tex-math><?CDATA $f(n)=\lambda^{n}{\rm{e}}^{-\lambda}/{n!}$?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M111.jpg" xlink:type="simple"/>
            </inline-formula>, where the parameter <italic toggle="yes">λ</italic> denotes the mean number of the radiated gluon which can be calculated by integrating Eq. (4). Once the radiation number <italic toggle="yes">n</italic> is sampled, the radiated gluon's four-momentum can be further sampled by Eq. (4) one at a time. As discussed above, the momentum update of heavy quarks is driven by Eq. (2). Furthermore, considering the energy loss of the light partons (light quark and gluon) inside the jet cone is essential for the calculation of the full-jet observable. As an effective treatment, the elastic energy loss of light partons is estimated by the perturbative quantum chroodynamics (pQCD) calculations for the hard theral loops (HTL) approximation [<xref ref-type="bibr" rid="cpc_49_6_064101_bib120">120</xref>],  whereas for the inelastic part, the higher-twist formalism is adopted.</p><p>The initial spatial production vertex of jets in nucleus-nucleus collisions is sampled based on the Monte Carlo (MC)-Glauber model [<xref ref-type="bibr" rid="cpc_49_6_064101_bib121">121</xref>]. During jet propagation, the velocity and temperature of the expanding QGP medium are provided by the CLVisc hydrodynamic model [<xref ref-type="bibr" rid="cpc_49_6_064101_bib122">122</xref>]. In general,   the partonic energy loss is assumed to cease at the hadronic phase, namely at the local temperature below <inline-formula>
               <tex-math><?CDATA $ T_c=0.165 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M112.jpg" xlink:type="simple"/>
            </inline-formula> GeV. In this work, the initial fluctuation of the bulk medium was ignored due to its small influence on the average energy loss of high-<inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M113.jpg" xlink:type="simple"/>
            </inline-formula> jet [<xref ref-type="bibr" rid="cpc_49_6_064101_bib123">123</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib125">125</xref>]. However, such initial fluctuations of hydrodynamics may be critical for the simultaneous description of the <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M114.jpg" xlink:type="simple"/>
            </inline-formula> and <inline-formula>
               <tex-math><?CDATA $ v_2 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M115.jpg" xlink:type="simple"/>
            </inline-formula> of heavy-flavor hadrons at low <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M116.jpg" xlink:type="simple"/>
            </inline-formula> regions [<xref ref-type="bibr" rid="cpc_49_6_064101_bib126">126</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib127">127</xref>]. Notably, based on the isotropic approximation of the QGP medium, <italic toggle="yes">κ</italic> and <inline-formula>
               <tex-math><?CDATA $ \hat{q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M117.jpg" xlink:type="simple"/>
            </inline-formula> of a high-energy heavy quark can be related through a concise expression <inline-formula>
               <tex-math><?CDATA $ \kappa=\hat{q}/2 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M118.jpg" xlink:type="simple"/>
            </inline-formula> [<xref ref-type="bibr" rid="cpc_49_6_064101_bib102">102</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib112">112</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib128">128</xref>]. In recent years, the SHELL transport model has been successfully employed to study the medium modifications of both light- and heavy-flavor jet in high-energy nuclear collisions [<xref ref-type="bibr" rid="cpc_49_6_064101_bib52">52</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib61">61</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib63">63</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib76">76</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib80">80</xref>, <xref ref-type="bibr" rid="cpc_49_6_064101_bib129">129</xref>].</p></sec><sec id="cpc_49_6_064101_s04"><label>IV.</label><title>RESULTS AND DISCUSSIONS</title><p>Note that <inline-formula>
               <tex-math><?CDATA $ \hat{q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M119.jpg" xlink:type="simple"/>
            </inline-formula> is the only parameter in our framework that controls the interaction strength for both light and heavy-flavor partons. First, we performed a <inline-formula>
               <tex-math><?CDATA $ \chi^2 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M120.jpg" xlink:type="simple"/>
            </inline-formula> fit of the recent inclusive-jet and b-jet <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M121.jpg" xlink:type="simple"/>
            </inline-formula> data measured by the ATLAS collaboration [<xref ref-type="bibr" rid="cpc_49_6_064101_bib59">59</xref>] to fix the model parameter <inline-formula>
               <tex-math><?CDATA $ \hat{q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M122.jpg" xlink:type="simple"/>
            </inline-formula>, where the jet <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M123.jpg" xlink:type="simple"/>
            </inline-formula> is conventionally defined as,</p><p>
            <disp-formula>
               <label>5</label>
               <tex-math id="cpc_49_6_064101_E5"> <?CDATA $ R_{AA}=\frac{1}{\langle N_{\rm bin}^{\rm AA} \rangle}\frac{{\rm d}\sigma^{\rm AA}/ {\rm d}y{\rm d}p_T}{{\rm d}\sigma^{\rm pp}/ {\rm d}y{\rm d}p_T} . $?> </tex-math>
               <graphic xlink:href="cpc_49_6_064101_E5.jpg" orientation="portrait" position="float" xlink:type="simple"/>
            </disp-formula>
         </p><p>The scaling factor <inline-formula>
               <tex-math><?CDATA $ \langle N_{\rm bin}^{AA} \rangle $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M124.jpg" xlink:type="simple"/>
            </inline-formula> denotes the number of binary nucleon-nucleon collisions in <italic toggle="yes">A+A</italic> estimated using the Glauber model [<xref ref-type="bibr" rid="cpc_49_6_064101_bib121">121</xref>]. The <inline-formula>
               <tex-math><?CDATA $ \chi^2 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M125.jpg" xlink:type="simple"/>
            </inline-formula> fit of the ATLAS data [<xref ref-type="bibr" rid="cpc_49_6_064101_bib59">59</xref>] obtained the optimal value of <inline-formula>
               <tex-math><?CDATA $ q_0= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M126.jpg" xlink:type="simple"/>
            </inline-formula> 0.9 GeV<inline-formula>
               <tex-math><?CDATA $ ^2 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M127.jpg" xlink:type="simple"/>
            </inline-formula>/fm with <inline-formula>
               <tex-math><?CDATA $ \chi^2= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M128.jpg" xlink:type="simple"/>
            </inline-formula>1.29. Using this configuration,  the model calculations of <italic toggle="yes">b</italic>-jet and inclusive jet <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M129.jpg" xlink:type="simple"/>
            </inline-formula>are  compared with the data in <xref ref-type="fig" rid="cpc_49_6_064101_f6">Fig. 6</xref>, showing good agreement for both the <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M130.jpg" xlink:type="simple"/>
            </inline-formula> magnitudes and their ratio <inline-formula>
               <tex-math><?CDATA $ R_{AA}^{\rm b-jet}/R_{AA}^{\rm incl-jet} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M131.jpg" xlink:type="simple"/>
            </inline-formula> from central to peripheral Pb+Pb collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M132.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV. The <italic toggle="yes">b</italic>-jets experence a more moderate yield suppression than the inclusive jet, which may indicate that the <italic toggle="yes">b</italic>-jet loses less energy in QGP than the light-flavor jet. However, the HQ-initiated jet is not the dominant contribution for <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet samples, as discussed in Sec. II. The mixture of components in HQ jets complicates the understanding of the mass effect of jet energy loss. Shown in <xref ref-type="fig" rid="cpc_49_6_064101_f7">Fig. 7</xref>is the nuclear modification factor <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M133.jpg" xlink:type="simple"/>
            </inline-formula> of both <italic toggle="yes">c</italic>-jet, <italic toggle="yes">b</italic>-jet, and inclusive jet in central 0−10% Pb+Pb collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M135.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV for different jet-cone sizes (<italic toggle="yes">R</italic> = 0.2, 0.4), at <inline-formula>
               <tex-math><?CDATA $ 30 \lt p_T \lt 260 $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M136.jpg" xlink:type="simple"/>
            </inline-formula> GeV. These calculations were performed at the parton level, and HQ jets (<italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet) are defined as jets containing at least one heavy quark inside the jet cone with <inline-formula>
               <tex-math><?CDATA $ p_T^Q \gt $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M137.jpg" xlink:type="simple"/>
            </inline-formula> 3 GeV. As the <italic toggle="yes">b</italic>-jet has the largest <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M138.jpg" xlink:type="simple"/>
            </inline-formula>, it is surprising that the <italic toggle="yes">c</italic>-jet has <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M139.jpg" xlink:type="simple"/>
            </inline-formula> comparable with that of the inclusive jet for <italic toggle="yes">R</italic> = 0.2. In addition, for larger jet cone <italic toggle="yes">R</italic> = 0.4, the yield suppression of <italic toggle="yes">c</italic>-jet was found to be stronger than that of inclusive jet at <inline-formula>
               <tex-math><?CDATA $ p_T \gt $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M140.jpg" xlink:type="simple"/>
            </inline-formula> 150 GeV. Similar results were also obtained using the linearized patronic transport  LIDO model [<xref ref-type="bibr" rid="cpc_49_6_064101_bib130">130</xref>].</p><fig id="cpc_49_6_064101_f6" orientation="portrait" position="float"><label>Fig. 6</label><caption id="cpc_49_6_064101_fc6"><p>(color online) The nuclear modification factor <inline-formula>
                     <tex-math><?CDATA $ R_{AA} $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M141.jpg" xlink:type="simple"/>
                  </inline-formula> of b-jet and inclusive jet in 0%−20%, 20%−50% and 50%−80% Pb+Pb collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M145.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV compared with ATLAS data (upper panels), along with their ratio <inline-formula>
                     <tex-math><?CDATA $R_{AA}^{{\rm b}{\text{-}}{\rm jet}}/R_{AA}^{{\rm incl}{\text{-}}{\rm jet}}$?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M146.jpg" xlink:type="simple"/>
                  </inline-formula> (lower panels).</p></caption><graphic xlink:href="cpc_49_6_064101_f6.eps" content-type="print" id="cpc_49_6_064101_f6_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f6.jpg" content-type="online" id="cpc_49_6_064101_f6_online" orientation="portrait" position="float" xlink:type="simple"/></fig><fig id="cpc_49_6_064101_f7" orientation="portrait" position="float"><label>Fig. 7</label><caption id="cpc_49_6_064101_fc7"><p>(color online) The nuclear modification factor <inline-formula>
                     <tex-math><?CDATA $ R_{AA} $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M147.jpg" xlink:type="simple"/>
                  </inline-formula> of <italic toggle="yes">c</italic>-jet, <italic toggle="yes">b</italic>-jet, and inclusive jet in central 0−10% Pb+Pb collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M149.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV for different jet-cone sizes (<italic toggle="yes">R</italic> = 0.2, 0.4).</p></caption><graphic xlink:href="cpc_49_6_064101_f7.eps" content-type="print" id="cpc_49_6_064101_f7_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f7.jpg" content-type="online" id="cpc_49_6_064101_f7_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>In <xref ref-type="fig" rid="cpc_49_6_064101_f8">Fig. 8,</xref> the averaged jet energy loss (<inline-formula>
               <tex-math><?CDATA $ \Delta p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M150.jpg" xlink:type="simple"/>
            </inline-formula>) of <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M151.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M152.jpg" xlink:type="simple"/>
            </inline-formula>-jet were estimated by tracking their propagation in 0−10% Pb+Pb collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M154.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV for <italic toggle="yes">c</italic>-jet (upper) and <italic toggle="yes">b</italic>-jet (lower). First, the total <italic toggle="yes">c</italic>-jet <inline-formula>
               <tex-math><?CDATA $ \Delta p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M155.jpg" xlink:type="simple"/>
            </inline-formula> is more significant than that of <italic toggle="yes">b</italic>-jet with the same initial <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M156.jpg" xlink:type="simple"/>
            </inline-formula>. Second, by comparing the <inline-formula>
               <tex-math><?CDATA $ \Delta p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M157.jpg" xlink:type="simple"/>
            </inline-formula> of <inline-formula>
               <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M158.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M159.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <italic toggle="yes">Q</italic>-jets initiated by the bottom lose less energy than that by charm, which is the direct embodiment of the mass hierarchy of quark energy loss. Finally, we find that <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M160.jpg" xlink:type="simple"/>
            </inline-formula>-jet loses much more energy than <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M161.jpg" xlink:type="simple"/>
            </inline-formula>-jet for both <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet. This study employed the <italic toggle="yes">p+p</italic> events after a full vacuum parton shower as input to simulate the in-medium energy loss. This treatment assumes all heavy quarks were created before the QGP was formed. Hence, the different energy losses of <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M162.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M163.jpg" xlink:type="simple"/>
            </inline-formula>-jet may only result from their initial features. As presented in <xref ref-type="fig" rid="cpc_49_6_064101_f4">Figs. 4</xref> and <xref ref-type="fig" rid="cpc_49_6_064101_f5">5</xref> at the end of Sec. II, the <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M164.jpg" xlink:type="simple"/>
            </inline-formula>-jet generally has a more dispersive (<inline-formula>
               <tex-math><?CDATA $ z_Q, r_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M165.jpg" xlink:type="simple"/>
            </inline-formula>) distribution compared to <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M166.jpg" xlink:type="simple"/>
            </inline-formula>-jet, namely plenty of heavy quarks are located in smaller <inline-formula>
               <tex-math><?CDATA $ z_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M167.jpg" xlink:type="simple"/>
            </inline-formula> and larger <inline-formula>
               <tex-math><?CDATA $ r_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M168.jpg" xlink:type="simple"/>
            </inline-formula> regions. Larger <inline-formula>
               <tex-math><?CDATA $ r_Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M169.jpg" xlink:type="simple"/>
            </inline-formula> facilitates the dissipation of lost energy from heavy quarks  outside the jet cone, which is consistent with the results of the recent measurements of the ATLAS, ALICE, and CMS collaborations [<xref ref-type="bibr" rid="cpc_49_6_064101_bib131">131</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib136">136</xref>], indicating that the more dispersive the jet structure is, the more energy is lost in the QGP. Moreover, the jets produced by <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q\bar{Q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M170.jpg" xlink:type="simple"/>
            </inline-formula> processes usually contain two heavy quarks inside the jet cone, and energy dissipation in the QGP is more efficient compared to the <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M171.jpg" xlink:type="simple"/>
            </inline-formula>-jet.</p><fig id="cpc_49_6_064101_f8" orientation="portrait" position="float"><label>Fig. 8</label><caption id="cpc_49_6_064101_fc8"><p>(color online) The averaged transverse jet energy loss (<inline-formula>
                     <tex-math><?CDATA $ \langle\Delta p_T\rangle $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M172.jpg" xlink:type="simple"/>
                  </inline-formula>) of <inline-formula>
                     <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M173.jpg" xlink:type="simple"/>
                  </inline-formula>-jet and <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M174.jpg" xlink:type="simple"/>
                  </inline-formula>-jet in 0−10% Pb+Pb collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M176.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV, both for <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet.</p></caption><graphic xlink:href="cpc_49_6_064101_f8.eps" content-type="print" id="cpc_49_6_064101_f8_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f8.jpg" content-type="online" id="cpc_49_6_064101_f8_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>An overall comparison of the <inline-formula>
               <tex-math><?CDATA $ \langle\Delta p_T\rangle $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M177.jpg" xlink:type="simple"/>
            </inline-formula> for the six kinds of jets (<inline-formula>
               <tex-math><?CDATA $ q \rightarrow \rm incl $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M178.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ g \rightarrow \rm incl $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M179.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M180.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M181.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M182.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M183.jpg" xlink:type="simple"/>
            </inline-formula>-jet) in 0−10% Pb+Pb collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M185.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV is shown in <xref ref-type="fig" rid="cpc_49_6_064101_f9">Fig. 9</xref>, to compare the flavor dependence of jet energy loss intuitively and systematically. First, it is essential that the energy loss of the jet initiated by the parton with different flavors be compared. Excluding the contribution from gluon splitting processes, we find that the jet energy loss obeys the order <inline-formula>
               <tex-math><?CDATA $ \Delta E_{g\rightarrow \rm incl-jet} \gt \Delta E_{q\rightarrow \rm incl-jet}\gtrsim \Delta E_{c\rightarrow c-\rm jet} \gt \Delta E_{b\rightarrow b-\rm jet} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M186.jpg" xlink:type="simple"/>
            </inline-formula>, in line with the flavor-dependent parton energy loss expectation. The <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M187.jpg" xlink:type="simple"/>
            </inline-formula>-jet shows a noticeable mass effect of energy loss compared to the <inline-formula>
               <tex-math><?CDATA $ q \rightarrow $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M188.jpg" xlink:type="simple"/>
            </inline-formula>incl-jet, whereas the <inline-formula>
               <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M189.jpg" xlink:type="simple"/>
            </inline-formula>-jet behaves more like a light quark jet at <inline-formula>
               <tex-math><?CDATA $ p_T \gt $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M190.jpg" xlink:type="simple"/>
            </inline-formula> 50 GeV. Comparing the energy loss of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M191.jpg" xlink:type="simple"/>
            </inline-formula>incl-jet with that of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M192.jpg" xlink:type="simple"/>
            </inline-formula>-jet is also interesting. They are all initiated by the high-energy gluon; however, the latter traverses the QGP as a <inline-formula>
               <tex-math><?CDATA $ Q\bar{Q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M193.jpg" xlink:type="simple"/>
            </inline-formula> pair inside the jet. The energy loss of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M194.jpg" xlink:type="simple"/>
            </inline-formula>-jet is smaller than that of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow \rm jet $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M195.jpg" xlink:type="simple"/>
            </inline-formula> but visibly larger than that of the <inline-formula>
               <tex-math><?CDATA $ q \rightarrow \rm incl $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M196.jpg" xlink:type="simple"/>
            </inline-formula>-jet, which indicates that the HQ jets from the gluon splitting lose more energy in the QGP than the light-quark jets. Therefore, the significant contribution of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M197.jpg" xlink:type="simple"/>
            </inline-formula>-jet may be the critical point for understanding the similar <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M198.jpg" xlink:type="simple"/>
            </inline-formula> of <italic toggle="yes">c</italic>-jet and inclusive jet shown in <xref ref-type="fig" rid="cpc_49_6_064101_f7">Fig. 7</xref>. In other words, due to the large fraction of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M199.jpg" xlink:type="simple"/>
            </inline-formula>-jet components, the averaged energy loss of <italic toggle="yes">c</italic>-jet is comparable to that of the inclusive jet. <xref ref-type="fig" rid="cpc_49_6_064101_f10">Fig. 10</xref> displays the fractions of <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M200.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M201.jpg" xlink:type="simple"/>
            </inline-formula>-jet for <italic toggle="yes">c</italic>-jet (left panel) and <italic toggle="yes">b</italic>-jet (middle panel) versus jet <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M202.jpg" xlink:type="simple"/>
            </inline-formula> (left panel) with <italic toggle="yes">R</italic> = 0.2 and <italic toggle="yes">R</italic> = 0.4. The fractions of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M203.jpg" xlink:type="simple"/>
            </inline-formula>-jet increase as <italic toggle="yes">R</italic> varies from 0.2 to 0.4, and accordingly, that of <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M204.jpg" xlink:type="simple"/>
            </inline-formula>-jet decreases for both <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet. For larger jet cones, the enhanced fraction of <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M205.jpg" xlink:type="simple"/>
            </inline-formula>-jet increases the average energy loss of HQ jets. The fractions of quark- and gluon-jet in the inclusive jet sample are shown in the right panel, and they are observed to be insensitive to the jet-cone size. This can explain why the <italic toggle="yes">c</italic>-jet <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M206.jpg" xlink:type="simple"/>
            </inline-formula>is smaller than that of the inclusive jet for <italic toggle="yes">R</italic> = 0.4, as shown in <xref ref-type="fig" rid="cpc_49_6_064101_f7">Fig. 7</xref>.</p><fig id="cpc_49_6_064101_f9" orientation="portrait" position="float"><label>Fig. 9</label><caption id="cpc_49_6_064101_fc9"><p>(color online) The averaged transverse energy loss (<inline-formula>
                     <tex-math><?CDATA $ \langle\Delta p_T\rangle $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M207.jpg" xlink:type="simple"/>
                  </inline-formula>) for the six kinds of jets, <inline-formula>
                     <tex-math><?CDATA $ q \rightarrow \rm incl $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M208.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow \rm incl $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M209.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, <inline-formula>
                     <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M210.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M211.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, <inline-formula>
                     <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M212.jpg" xlink:type="simple"/>
                  </inline-formula>-jet and <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M213.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, in 0−10% Pb+Pb collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M215.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV.</p></caption><graphic xlink:href="cpc_49_6_064101_f9.eps" content-type="print" id="cpc_49_6_064101_f9_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f9.jpg" content-type="online" id="cpc_49_6_064101_f9_online" orientation="portrait" position="float" xlink:type="simple"/></fig><fig id="cpc_49_6_064101_f10" orientation="portrait" position="float"><label>Fig. 10</label><caption id="cpc_49_6_064101_fc10"><p>(color online) The fractional contributions of <inline-formula>
                     <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M216.jpg" xlink:type="simple"/>
                  </inline-formula>-jet and <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M217.jpg" xlink:type="simple"/>
                  </inline-formula>-jet to the total <italic toggle="yes">c</italic>-jet; <inline-formula>
                     <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M218.jpg" xlink:type="simple"/>
                  </inline-formula>-jet and <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M219.jpg" xlink:type="simple"/>
                  </inline-formula>-jet to the total <italic toggle="yes">b</italic>-jet; <inline-formula>
                     <tex-math><?CDATA $ q \rightarrow \rm incl $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M220.jpg" xlink:type="simple"/>
                  </inline-formula>-jet and <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow \rm incl $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M221.jpg" xlink:type="simple"/>
                  </inline-formula>-jet to the inclusive jet; differential cross section versus <inline-formula>
                     <tex-math><?CDATA $ p_T $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M222.jpg" xlink:type="simple"/>
                  </inline-formula> in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M223.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV, as jet-cone size varies from 0.2 to 0.4.</p></caption><graphic xlink:href="cpc_49_6_064101_f10.eps" content-type="print" id="cpc_49_6_064101_f10_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f10.jpg" content-type="online" id="cpc_49_6_064101_f10_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>So far, we have discussed the jet energy loss of <italic toggle="yes">c</italic>-jet, <italic toggle="yes">b</italic>-jet, and inclusive jet by systematically analyzing their component features and fraction variations. Notably, the energy loss of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M224.jpg" xlink:type="simple"/>
            </inline-formula>-jet is significantly more pronounced than that of the <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M225.jpg" xlink:type="simple"/>
            </inline-formula>-jet in nucleus-nucleus collisions. Our calculations indicate that <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M226.jpg" xlink:type="simple"/>
            </inline-formula>-jet behaves like a gluon-jet but not a heavy quark jet. More efforts in future experimental measurements on <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M227.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M228.jpg" xlink:type="simple"/>
            </inline-formula>-jet can be helpful  in addressing the flavor/mass dependence of jet energy loss. However, these measurements assume that the reconstructed Q-jets from different channels (<inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M229.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M230.jpg" xlink:type="simple"/>
            </inline-formula>-jet) can be identified effectively in the experiment. For this reason, we present the selection methods for separating the two processes <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M231.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M232.jpg" xlink:type="simple"/>
            </inline-formula>-jet and also estimate the purity of the jet sample selected by these strategies.</p><p>As mentioned in Sec. II, the <inline-formula>
               <tex-math><?CDATA $ Q\bar{Q} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M233.jpg" xlink:type="simple"/>
            </inline-formula> pairs produced by <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M234.jpg" xlink:type="simple"/>
            </inline-formula>-jet usually have a narrow opening angle, whereas the one from hard scattering is usually "back-to-back" in the azimuthal plane. We designed the following strategies to select the high-purity sample of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M235.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M236.jpg" xlink:type="simple"/>
            </inline-formula>-jet, respectively.</p><p>● <bold>Strategy-1</bold> for <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M237.jpg" xlink:type="simple"/>
            </inline-formula>-jet: Selecting jets containing two heavy quarks inside the jet-cone. The heavy quark should have <inline-formula>
               <tex-math><?CDATA $ p_T^Q \gt $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M238.jpg" xlink:type="simple"/>
            </inline-formula>2 GeV.</p><p>● <bold>Strategy-2</bold> for <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M239.jpg" xlink:type="simple"/>
            </inline-formula>-jet: Selecting jets containing only one heavy quark inside the jet-cone. Moreover, the selected candidates should have a recoiled HQ jet partner with <inline-formula>
               <tex-math><?CDATA $ p_T \gt $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M240.jpg" xlink:type="simple"/>
            </inline-formula>10 GeV, and their angle of separation in azimuth plane should satisfy <inline-formula>
               <tex-math><?CDATA $ \Delta \phi_{12} \gt 2/3\pi $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M241.jpg" xlink:type="simple"/>
            </inline-formula>.</p><p>To test the performance of the selection strategies, in <xref ref-type="fig" rid="cpc_49_6_064101_f11">Fig. 11</xref> we show the purities of the selected <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M242.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M243.jpg" xlink:type="simple"/>
            </inline-formula>-jet samples in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M244.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV for both <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet, where purity is defined as the fraction of the target process in the total selected jet sample,</p><fig id="cpc_49_6_064101_f11" orientation="portrait" position="float"><label>Fig. 11</label><caption id="cpc_49_6_064101_fc11"><p>(color online) Purities of the selected of <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M245.jpg" xlink:type="simple"/>
                  </inline-formula>-jet and <inline-formula>
                     <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M246.jpg" xlink:type="simple"/>
                  </inline-formula>-jet samples for <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet in <italic toggle="yes">p+p</italic> collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M247.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV.</p></caption><graphic xlink:href="cpc_49_6_064101_f11.eps" content-type="print" id="cpc_49_6_064101_f11_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f11.jpg" content-type="online" id="cpc_49_6_064101_f11_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>
            <disp-formula>
               <label>6</label>
               <tex-math id="cpc_49_6_064101_E6"> <?CDATA $ {\rm Purity}=\frac{{\rm d}\sigma/{\rm d}p_T[{\rm target \: process}]}{{\rm d}\sigma/{\rm d}p_T[{\rm selected \: jet \: sample}]}. $?> </tex-math>
               <graphic xlink:href="cpc_49_6_064101_E6.jpg" orientation="portrait" position="float" xlink:type="simple"/>
            </disp-formula>
         </p><p>In the upper panel of <xref ref-type="fig" rid="cpc_49_6_064101_f11">Fig. 11</xref>, the purity of the selected <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M248.jpg" xlink:type="simple"/>
            </inline-formula>-jet sample is above 0.9 for both <italic toggle="yes">c</italic>-jet and <italic toggle="yes">b</italic>-jet. In the lower panel, the purity of the selected <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M249.jpg" xlink:type="simple"/>
            </inline-formula>-jet sample is above 0.8 for <italic toggle="yes">c</italic>-jet and 0.9 for <italic toggle="yes">b</italic>-jet. The selection strategies tested in <italic toggle="yes">A+A</italic> collisions also show similar satisfactory performance.</p><p>After establishing the effective strategies for selecting the <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M250.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M251.jpg" xlink:type="simple"/>
            </inline-formula>-jet, we can directly compare their yield suppression in <italic toggle="yes">A+A</italic> collisions with the inclusive jet. Although isolating the gluon jet and quark jet in the experiment is difficult, the comparison between <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M252.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M253.jpg" xlink:type="simple"/>
            </inline-formula>-jet, and inclusive jet may provide a unique opportunity for capturing the flavor/mass dependence of jet quenching, which can be used to test the experiments. <xref ref-type="fig" rid="cpc_49_6_064101_f12">Fig. 12</xref> compares the calculated<inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M254.jpg" xlink:type="simple"/>
            </inline-formula> of selected <inline-formula>
               <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M255.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M256.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M257.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M258.jpg" xlink:type="simple"/>
            </inline-formula>-jet with that of inclusive jet in 0−10% Pb+Pb collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M260.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV. Note that <inline-formula>
               <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M261.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M262.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M263.jpg" xlink:type="simple"/>
            </inline-formula>-jet, and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M264.jpg" xlink:type="simple"/>
            </inline-formula>-jet denote the selected samples with the above mentioned strategies. Clearly, the jets initiated by heavy quarks obey the order <inline-formula>
               <tex-math><?CDATA $ R_{AA}^{\rm b-jet} \gt R_{AA}^{\rm c-jet} \gt R_{AA}^{\rm incl-jet} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M265.jpg" xlink:type="simple"/>
            </inline-formula>. Namely, by effectively isolating the <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M266.jpg" xlink:type="simple"/>
            </inline-formula>-jet processes, the mass hierarchy of energy loss at jet level (<inline-formula>
               <tex-math><?CDATA $\Delta E_{\rm incl-jet} \gt \Delta E_{\rm c-jet} \gt \Delta E_{\rm b-jet}$?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M267.jpg" xlink:type="simple"/>
            </inline-formula>) is predicted in nucleus-nucleus collisions. We observe that the yield suppression of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M268.jpg" xlink:type="simple"/>
            </inline-formula>-jet is much stronger than that of inclusive jet. As for the <inline-formula>
               <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M269.jpg" xlink:type="simple"/>
            </inline-formula>-jet, its yield suppression is obviously stronger than that of <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M270.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M271.jpg" xlink:type="simple"/>
            </inline-formula>-jet. At high <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M272.jpg" xlink:type="simple"/>
            </inline-formula>, <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M273.jpg" xlink:type="simple"/>
            </inline-formula> of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M274.jpg" xlink:type="simple"/>
            </inline-formula>-jet is slightly lower than that of inclusive jet whereas their values are close at lower <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M275.jpg" xlink:type="simple"/>
            </inline-formula>. This may result from the dispersive structure of the <italic toggle="yes">b</italic>-jets generated by the <inline-formula>
               <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M276.jpg" xlink:type="simple"/>
            </inline-formula>-jet process, which can lead to more energy loss in the QGP compared to the <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M277.jpg" xlink:type="simple"/>
            </inline-formula>-jet, similar to the case of the <italic toggle="yes">c</italic>-jet.</p><fig id="cpc_49_6_064101_f12" orientation="portrait" position="float"><label>Fig. 12</label><caption id="cpc_49_6_064101_fc12"><p>(color online) <inline-formula>
                     <tex-math><?CDATA $ R_{AA} $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M278.jpg" xlink:type="simple"/>
                  </inline-formula> of the selected <inline-formula>
                     <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M279.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M280.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, <inline-formula>
                     <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M281.jpg" xlink:type="simple"/>
                  </inline-formula>-jet, and <inline-formula>
                     <tex-math><?CDATA $ g \rightarrow b $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M282.jpg" xlink:type="simple"/>
                  </inline-formula>-jet compared to that of the inclusive jet in 0−10% Pb+Pb collisions at <inline-formula>
                     <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
                     <inline-graphic xlink:href="cpc_49_6_064101_M284.jpg" xlink:type="simple"/>
                  </inline-formula> 5.02 TeV.</p></caption><graphic xlink:href="cpc_49_6_064101_f12.eps" content-type="print" id="cpc_49_6_064101_f12_eps" orientation="portrait" position="float" xlink:type="simple"/><graphic xlink:href="cpc_49_6_064101_f12.jpg" content-type="online" id="cpc_49_6_064101_f12_online" orientation="portrait" position="float" xlink:type="simple"/></fig><p>Unlike the treatment in [<xref ref-type="bibr" rid="cpc_49_6_064101_bib50">50</xref>], which considers the fragmentation function of high-energy gluon into the heavy-flavor hadron in the hadronization process, in this study, the vacuum splitting of <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M285.jpg" xlink:type="simple"/>
            </inline-formula>-jet was simulated before the formation of the QGP medium. The results obtained from different treatments are consistent, indicating that the heavy flavors from gluon splitting suffer a stronger quenching effect than those from the hard scattering in heavy-ion collisions. We next plan to investigate the influence of considering the concrete <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M286.jpg" xlink:type="simple"/>
            </inline-formula>-jet splitting time in the QGP medium on the energy loss and substructure modifications of HQ jets, and some recent exploratory studies in this direction are expected to be helpful [<xref ref-type="bibr" rid="cpc_49_6_064101_bib137">137</xref>−<xref ref-type="bibr" rid="cpc_49_6_064101_bib139">139</xref>]. Moreover, the recent studies have extracted the gluon energy loss by <inline-formula>
               <tex-math><?CDATA $ J/\Psi $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M287.jpg" xlink:type="simple"/>
            </inline-formula> production in Pb+Pb collisions [<xref ref-type="bibr" rid="cpc_49_6_064101_bib51">51</xref>] because over 80% <inline-formula>
               <tex-math><?CDATA $ J/\Psi $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M289.jpg" xlink:type="simple"/>
            </inline-formula> is mainly produced by the gluon fragmentation at high <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M290.jpg" xlink:type="simple"/>
            </inline-formula>. From this point of view, measurement on the <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M291.jpg" xlink:type="simple"/>
            </inline-formula>-jet production in <italic toggle="yes">A+A</italic> collisions can similarly build a bridge for understanding the energy loss of the gluon jet.</p></sec><sec id="cpc_49_6_064101_s05"><label>V.</label><title>SUMMARY</title><p>This paper systematically studies the yield suppression of HQ jets in nucleus-nucleus collisions relative to the <italic toggle="yes">p+p,</italic> focusing on the energy loss of HQ jets produced by different production mechanisms. The Monte Carlo event generator SHERPA was used to generate the p+p baseline, which matches the NLO hard QCD processes with the resummation of the parton shower. The in-medium evolution of the HQ jets was described by the SHELL transport model, which considers the elastic and inelastic energy loss. The <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M292.jpg" xlink:type="simple"/>
            </inline-formula>-jet process significantly contributed to the HQ jet production at high <inline-formula>
               <tex-math><?CDATA $ p_T $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M293.jpg" xlink:type="simple"/>
            </inline-formula> and showed more dispersive structures compared to the <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M294.jpg" xlink:type="simple"/>
            </inline-formula>-jet in <italic toggle="yes">p+p</italic> collisions. In Pb+Pb collisions at <inline-formula>
               <tex-math><?CDATA $ \sqrt{s_{NN}}= $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M295.jpg" xlink:type="simple"/>
            </inline-formula> 5.02 TeV, our calculations provide descriptions of the inclusive jet and b-jet <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M296.jpg" xlink:type="simple"/>
            </inline-formula> as measured by the ATLAS collaboration, which remarkably point to the mass effect of jet energy loss. Due to its dispersive substructure, <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M297.jpg" xlink:type="simple"/>
            </inline-formula>-jet lost more energy than the <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M298.jpg" xlink:type="simple"/>
            </inline-formula>-jet in the same collision system. Furthermore, because of the dominant contribution of the <inline-formula>
               <tex-math><?CDATA $ g \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M299.jpg" xlink:type="simple"/>
            </inline-formula>-jet, the <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M300.jpg" xlink:type="simple"/>
            </inline-formula> of <italic toggle="yes">c</italic>-jet was comparable or even smaller than that of inclusive jet. We proposed event selection strategies based on their topological features and tested their performances, which allowed us to distinguish the two processes <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M301.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M302.jpg" xlink:type="simple"/>
            </inline-formula>-jet according to the final-state jet particle information. By isolating the <inline-formula>
               <tex-math><?CDATA $ c \rightarrow c $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M303.jpg" xlink:type="simple"/>
            </inline-formula>-jet, <inline-formula>
               <tex-math><?CDATA $ b \rightarrow b $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M304.jpg" xlink:type="simple"/>
            </inline-formula>-jet, and the jets initiated by heavy quarks, we predicted that the order of their <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M305.jpg" xlink:type="simple"/>
            </inline-formula> aligns with the mass hierarchy of energy loss. Measurements on the <inline-formula>
               <tex-math><?CDATA $ R_{AA} $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M306.jpg" xlink:type="simple"/>
            </inline-formula> of <inline-formula>
               <tex-math><?CDATA $ Q \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M307.jpg" xlink:type="simple"/>
            </inline-formula>-jet and <inline-formula>
               <tex-math><?CDATA $ g \rightarrow Q $?></tex-math>
               <inline-graphic xlink:href="cpc_49_6_064101_M308.jpg" xlink:type="simple"/>
            </inline-formula>-jet in heavy-ion collisions provide a unique opportunity for testing the flavor/mass dependence of energy loss at the jet level.</p></sec></body><back><ref-list><title>References</title><ref id="cpc_49_6_064101_bib1"><label>[1]</label><element-citation publication-type="other" xlink:type="simple"><comment>M. Gyulassy, I. Vitev, X. N. Wang <italic toggle="yes">et al</italic>., In <italic toggle="yes">Quark Gluon Plasma</italic>, edited by Hwa R.C <italic toggle="yes">et al</italic>. (Singapore: World Scientific, 2010), p.123-191</comment></element-citation></ref><ref id="cpc_49_6_064101_bib2"><label>[2]</label><element-citation publication-type="journal" xlink:type="simple"><person-group person-group-type="author">
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