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<article article-type="research-article" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:oasis="http://www.niso.org/standards/z39-96/ns/oasis-exchange/table"><front><journal-meta><journal-id journal-id-type="publisher-id">PRL</journal-id><journal-id journal-id-type="coden">PRLTAO</journal-id><journal-title-group><journal-title>Physical Review Letters</journal-title><abbrev-journal-title>Phys. Rev. Lett.</abbrev-journal-title></journal-title-group><issn pub-type="ppub">0031-9007</issn><issn pub-type="epub">1079-7114</issn><publisher><publisher-name>American Physical Society</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.1103/PhysRevLett.124.221801</article-id><article-categories><subj-group subj-group-type="toc-major"><subject>LETTERS</subject></subj-group><subj-group subj-group-type="toc-minor"><subject>Elementary Particles and Fields</subject></subj-group></article-categories><title-group><article-title>High Quality QCD Axion and the LHC</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>Hook</surname><given-names>Anson</given-names></name><xref ref-type="aff" rid="a1"/><xref ref-type="author-notes" rid="n2"><sup>†</sup></xref></contrib><contrib contrib-type="author"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-6924-3375</contrib-id><name><surname>Kumar</surname><given-names>Soubhik</given-names></name><xref ref-type="aff" rid="a1"/><xref ref-type="author-notes" rid="n1"><sup>*</sup></xref></contrib><contrib contrib-type="author"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-3143-1976</contrib-id><name><surname>Liu</surname><given-names>Zhen</given-names></name><xref ref-type="aff" rid="a1"/><xref ref-type="author-notes" rid="n3"><sup>‡</sup></xref></contrib><contrib contrib-type="author"><name><surname>Sundrum</surname><given-names>Raman</given-names></name><xref ref-type="aff" rid="a1"/><xref ref-type="author-notes" rid="n4"><sup>§</sup></xref></contrib><aff id="a1">Maryland Center for Fundamental Physics, Department of Physics, <institution>University of Maryland</institution>, College Park, Maryland 20742, USA</aff></contrib-group><author-notes><fn id="n1"><label><sup>*</sup></label><p>Corresponding author.</p><p><email>soubhik@terpmail.umd.edu</email></p></fn><fn id="n2"><label><sup>†</sup></label><p><email>hook@umd.edu</email></p></fn><fn id="n3"><label><sup>‡</sup></label><p><email>zliuphys@umd.edu</email></p></fn><fn id="n4"><label><sup>§</sup></label><p><email>raman@umd.edu</email></p></fn></author-notes><pub-date iso-8601-date="2020-06-01" date-type="pub" publication-format="electronic"><day>1</day><month>June</month><year>2020</year></pub-date><pub-date iso-8601-date="2020-06-05" date-type="pub" publication-format="print"><day>5</day><month>June</month><year>2020</year></pub-date><volume>124</volume><issue>22</issue><elocation-id>221801</elocation-id><pub-history><event><date iso-8601-date="2019-12-23" date-type="received"><day>23</day><month>December</month><year>2019</year></date></event><event><date iso-8601-date="2020-04-29" date-type="accepted"><day>29</day><month>April</month><year>2020</year></date></event></pub-history><permissions><copyright-statement>Published by the American Physical Society</copyright-statement><copyright-year>2020</copyright-year><copyright-holder>authors</copyright-holder><license license-type="creative-commons" xlink:href="https://creativecommons.org/licenses/by/4.0/"><license-p content-type="usage-statement">Published by the American Physical Society under the terms of the <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution 4.0 International</ext-link> license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP<sup>3</sup>.</license-p></license></permissions><abstract><p>The QCD axion provides an elegant solution to the strong <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> problem. While the minimal realization is vulnerable to the so-called “axion quality problem,” we will consider a more robust realization in the presence of a mirror sector related to the standard model by a (softly broken) <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> symmetry. We point out that the resulting “heavy” axion, while satisfying all theoretical and observational constraints, has a large and uncharted parameter space, which allows it to be probed at the LHC as a long-lived particle (LLP). The small defining axionic coupling to gluons results in a challenging hadronic decay signal which we argue can be distinguished against the background in such a long-lived regime, and yet, the same coupling allows for sufficient production at the hadron colliders thanks to the large gluon-parton luminosity. Our study opens up a new window towards accelerator observable axions and, more generally, singly produced LLPs.</p></abstract><funding-group><award-group award-type="grant"><funding-source country="US"><institution-wrap><institution>National Science Foundation</institution><institution-id institution-id-type="doi" vocab="open-funder-registry" vocab-identifier="10.13039/open-funder-registry">10.13039/100000001</institution-id></institution-wrap></funding-source><award-id>PHY-1620074</award-id><award-id>PHY-1914480</award-id><award-id>PHY-1914731</award-id><award-id>PHY-174958</award-id><award-id>PHY-1607611</award-id></award-group><award-group award-type="unspecified"><funding-source country="US"><institution-wrap><institution>Maryland Center for Fundamental Physics</institution><institution-id institution-id-type="doi" vocab="open-funder-registry" vocab-identifier="10.13039/open-funder-registry">10.13039/100008510</institution-id></institution-wrap></funding-source></award-group><award-group award-type="unspecified"><funding-source country="US"><institution-wrap><institution>University of Pittsburgh</institution><institution-id institution-id-type="doi" vocab="open-funder-registry" vocab-identifier="10.13039/open-funder-registry">10.13039/100007921</institution-id></institution-wrap></funding-source></award-group><award-group award-type="unspecified"><funding-source country=""><institution-wrap><institution>MIAPP</institution><institution-id institution-id-type="doi" vocab="open-funder-registry" vocab-identifier="10.13039/open-funder-registry">10.13039/501100012162</institution-id></institution-wrap></funding-source></award-group><award-group award-type="unspecified"><funding-source country="US"><institution-wrap><institution>Aspen Center for Physics</institution><institution-id institution-id-type="doi" vocab="open-funder-registry" vocab-identifier="10.13039/open-funder-registry">10.13039/100007739</institution-id></institution-wrap></funding-source></award-group></funding-group><counts><page-count count="7"/></counts></article-meta></front><body><sec id="s1"><title specific-use="run-in">Introduction.—</title><p>The strong <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> problem is the puzzle of why the strong interactions are <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> symmetric, even though the standard model (SM) as a whole is not. Technically, the question centers on the vanishingly small value of the one <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula>-violating coupling of QCD, <inline-formula><mml:math display="inline"><mml:mi>θ</mml:mi></mml:math></inline-formula>. An elegant solution is provided by elevating <inline-formula><mml:math display="inline"><mml:mi>θ</mml:mi></mml:math></inline-formula> to a fully dynamical pseudoscalar “axion” field. If the axion gets its potential entirely through QCD effects, then remarkably its ground state automatically corresponds to <inline-formula><mml:math display="inline"><mml:mi>θ</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula> <xref ref-type="bibr" rid="c1 c2 c3 c4">[1–4]</xref>.</p><p>Despite this bottom-up simplicity, the QCD axion mechanism has a top-down flaw: the axion quality problem <xref ref-type="bibr" rid="c5 c6 c7 c8">[5–8]</xref>. This arises because there can be other UV contributions to the axion potential that can push the minimum away from <inline-formula><mml:math display="inline"><mml:mi>θ</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>. We consider a mirror sector in the UV related to the SM by a <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> symmetry, generalizing on Refs. <xref ref-type="bibr" rid="c9 c10 c11 c12 c13">[9–13]</xref>, coupled to the same axion, such that its contribution to the axion potential is much larger than QCD’s but aligned with it in having its minimum at <inline-formula><mml:math display="inline"><mml:mi>θ</mml:mi><mml:mo>=</mml:mo><mml:mn>0</mml:mn></mml:math></inline-formula>. This results in an axion mechanism which is vastly more robust against other uncorrelated UV effects. See Refs. <xref ref-type="bibr" rid="c14 c15 c16 c17">[14–17]</xref> (also recent work Refs. <xref ref-type="bibr" rid="c18 c19 c20">[18–20]</xref>) for special UV structures that mitigate the quality problem, and Refs. <xref ref-type="bibr" rid="c21 c22 c23 c24 c25 c26 c27 c28">[21–28]</xref> for alternate mechanisms for having a heavy QCD axion.</p><p>Our general solution to the quality problem places us in a very different and interesting region in axion mass-coupling parameter space (for reviews of the standard regimes, see Refs. <xref ref-type="bibr" rid="c29 c30">[29,30]</xref>), in which the axion can be probed as a quantum particle at cutting-edge collider experiments. While there are a number of axion(-like) particle collider studies <xref ref-type="bibr" rid="c31 c32 c33 c34 c35 c36 c37 c38 c39 c40 c41 c42 c43 c44 c45 c46 c47 c48 c49 c50 c51 c52 c53 c54 c55 c56 c57 c58 c59 c60 c61 c62 c63 c64 c65">[31–65]</xref>, we will show that this high quality axion search presents an experimentally novel but challenging target for singly produced long-lived particles (LLPs) at the LHC main detectors.</p></sec><sec id="s2"><title specific-use="run-in">Axion mechanism and the quality problem.—</title><p>The QCD axion field <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>x</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> is coupled to QCD by promoting <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo stretchy="false">→</mml:mo><mml:mspace linebreak="goodbreak"/><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mi>a</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>x</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo stretchy="false">/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula>: <disp-formula id="d1"><mml:math display="block"><mml:mrow><mml:mi mathvariant="script">L</mml:mi><mml:mo>⊃</mml:mo><mml:mfrac><mml:mrow><mml:msub><mml:mrow><mml:mi>α</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mn>8</mml:mn><mml:mi>π</mml:mi></mml:mrow></mml:mfrac><mml:mrow><mml:mo>(</mml:mo><mml:mover accent="true"><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:mi>a</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>x</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo>)</mml:mo></mml:mrow><mml:msubsup><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mi>μ</mml:mi><mml:mi>ν</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msubsup><mml:msup><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">˜</mml:mo></mml:mrow></mml:mover></mml:mrow><mml:mrow><mml:mi>a</mml:mi><mml:mo>,</mml:mo><mml:mi>μ</mml:mi><mml:mi>ν</mml:mi></mml:mrow></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math><label>(1)</label></disp-formula>In the absence of the axion, <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula> represents the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula>-odd gauge invariant QCD coupling, constrained by bounds on the neutron electric dipole moment (EDM) to be <inline-formula><mml:math display="inline"><mml:mrow><mml:mo stretchy="false">|</mml:mo><mml:mover accent="true"><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mo>-</mml:mo><mml:mn>10</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="c66">[66]</xref>. In the above, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>α</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mrow><mml:mi>g</mml:mi></mml:mrow><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo stretchy="false">/</mml:mo><mml:mn>4</mml:mn><mml:mi>π</mml:mi></mml:mrow></mml:math></inline-formula> is given in terms of the QCD gauge coupling <inline-formula><mml:math display="inline"><mml:msub><mml:mi>g</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>G</mml:mi><mml:mo accent="true" stretchy="false">˜</mml:mo></mml:mover></mml:math></inline-formula> denotes the dual of the gluon field strength, <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">˜</mml:mo></mml:mrow></mml:mover></mml:mrow><mml:mrow><mml:mi>a</mml:mi><mml:mo>,</mml:mo><mml:mi>μ</mml:mi><mml:mi>ν</mml:mi></mml:mrow></mml:msup><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mn>1</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mfrac><mml:msup><mml:mrow><mml:mi>ε</mml:mi></mml:mrow><mml:mrow><mml:mi>μ</mml:mi><mml:mi>ν</mml:mi><mml:mi>ρ</mml:mi><mml:mi>σ</mml:mi></mml:mrow></mml:msup><mml:msubsup><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mi>ρ</mml:mi><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> with <inline-formula><mml:math display="inline"><mml:msup><mml:mi>ε</mml:mi><mml:mn>0123</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula>; and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula> denotes the axion “decay constant.” The parameter <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula> is the <italic>effective</italic> <inline-formula><mml:math display="inline"><mml:mi>θ</mml:mi></mml:math></inline-formula> parameter obtained after diagonalizing the Yukawa matrices via chiral rotations, and is given by <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo>≡</mml:mo><mml:mspace linebreak="goodbreak"/><mml:mi>θ</mml:mi><mml:mo>+</mml:mo><mml:mi>arg</mml:mi><mml:mtext> </mml:mtext><mml:mi>det</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>Y</mml:mi></mml:mrow><mml:mrow><mml:mi>u</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mrow><mml:mi>Y</mml:mi></mml:mrow><mml:mrow><mml:mi>d</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:msub><mml:mi>Y</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>d</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:msub></mml:math></inline-formula> is the up (down) type Yukawa matrix with complex entries and <inline-formula><mml:math display="inline"><mml:mi>θ</mml:mi></mml:math></inline-formula> is a <italic>bare</italic> Lagrangian parameter.</p><p>The nonperturbative QCD axion potential resulting from Eq. <xref ref-type="disp-formula" rid="d1">(1)</xref> can be calculated using chiral perturbation theory <xref ref-type="bibr" rid="c3 c67">[3,67]</xref>, <disp-formula id="d2"><mml:math display="block"><mml:mrow><mml:mi mathvariant="script">V</mml:mi><mml:mo>≈</mml:mo><mml:mo>-</mml:mo><mml:msubsup><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:msubsup><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:msqrt><mml:mrow><mml:mn>1</mml:mn><mml:mo>-</mml:mo><mml:mfrac><mml:mrow><mml:mn>4</mml:mn><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>u</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>d</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>u</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>d</mml:mi></mml:mrow></mml:msub><mml:msup><mml:mrow><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mfrac><mml:msup><mml:mrow><mml:mi>sin</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:mi>a</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>x</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">¯</mml:mo></mml:mrow></mml:mover></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mfrac><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:msqrt><mml:mo>,</mml:mo></mml:mrow></mml:math><label>(2)</label></disp-formula>where <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>π</mml:mi></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>π</mml:mi></mml:msub></mml:math></inline-formula> are, respectively, the mass and the decay constant of the pion, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>d</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:msub></mml:math></inline-formula> is the up (down) quark mass. Given the potential in Eq. <xref ref-type="disp-formula" rid="d2">(2)</xref> (and its refinements), the axion acquires a vacuum expectation value (VEV), <inline-formula><mml:math display="inline"><mml:mo stretchy="false">⟨</mml:mo><mml:mi>a</mml:mi><mml:mo stretchy="false">⟩</mml:mo><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula>. Plugging this into Eq. <xref ref-type="disp-formula" rid="d1">(1)</xref> we see at low energies that the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> violation in QCD is eliminated—solving the strong <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> problem.</p><p>Clearly, if there is any other contribution to the axion potential from beyond QCD, the resulting axion ground state need no longer screen the QCD <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> violation. One can realize the axion as a Nambu-Goldstone boson of a <inline-formula><mml:math display="inline"><mml:mi>U</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>1</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> Peccei-Quinn (PQ) symmetry, <inline-formula><mml:math display="inline"><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>a</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>ϕ</mml:mi></mml:mrow></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>a</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:msup></mml:math></inline-formula>, which would forbid any axion potential. But such a symmetry cannot be exact because it is broken by QCD (chiral anomaly) effects, and further in the far UV quantum gravity is expected to explicitly break all global symmetries <xref ref-type="bibr" rid="c68 c69">[68,69]</xref>. At best, PQ must be an accidental symmetry of the leading couplings. For example, the UV violation of PQ symmetry may take the form of a higher-dimensional composite operator <inline-formula><mml:math display="inline"><mml:mi mathvariant="script">O</mml:mi></mml:math></inline-formula> with scaling dimension <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn>4</mml:mn></mml:math></inline-formula> and PQ charge <inline-formula><mml:math display="inline"><mml:mi>q</mml:mi></mml:math></inline-formula>, <disp-formula id="d3"><mml:math display="block"><mml:mrow><mml:mi mathvariant="script">L</mml:mi><mml:mo>⊃</mml:mo><mml:mfrac><mml:mrow><mml:mi mathvariant="script">O</mml:mi></mml:mrow><mml:mrow><mml:msubsup><mml:mrow><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>-</mml:mo><mml:mn>4</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac><mml:munder><mml:mrow><mml:mo>∼</mml:mo></mml:mrow><mml:mrow><mml:mtext>low energies</mml:mtext></mml:mrow></mml:munder><mml:mfrac><mml:mrow><mml:msubsup><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi></mml:mrow></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mrow><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>-</mml:mo><mml:mn>4</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac><mml:msup><mml:mrow><mml:mi>e</mml:mi></mml:mrow><mml:mrow><mml:mi>i</mml:mi><mml:mi>q</mml:mi><mml:mi>a</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math><label>(3)</label></disp-formula>where <inline-formula><mml:math display="inline"><mml:msub><mml:mi>M</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>∼</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>19</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula> is the Planck scale. Naively, one would expect that Planck-suppressed PQ violation would have negligible effects on the axion mechanism. However, given the experimental or astrophysical constraint <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub><mml:mo>&gt;</mml:mo><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>9</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="c30">[30]</xref> and the very delicate QCD potential of Eq. <xref ref-type="disp-formula" rid="d2">(2)</xref>, the axion mechanism is spoiled (for <inline-formula><mml:math display="inline"><mml:mi>q</mml:mi><mml:mo>∼</mml:mo><mml:mn>1</mml:mn></mml:math></inline-formula>) out to very high scaling dimension unless <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>≥</mml:mo><mml:mn>9</mml:mn></mml:math></inline-formula>. This extreme fragility of the axion mechanism is the so-called “quality problem” <xref ref-type="bibr" rid="c5 c6 c7 c8">[5–8]</xref>.</p></sec><sec id="s3"><title specific-use="run-in">Model construction.—</title><p>While it is possible, but demanding, that the UV structure does strongly suppress PQ violation at this level, in this Letter, we study a different approach: we strengthen the IR axion mechanism itself. We will consider a <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> symmetry that exchanges the fields of the SM and matching fields of a mirror sector. This replication includes the SM gauge structure, so that the entire mirror sector carries no SM charges and vice versa. All the marginal (dimensionless) couplings of the two sectors are identical, including <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula>. However <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is softly broken in the one relevant operator by having two distinct tachyonic Higgs mass terms, <inline-formula><mml:math display="inline"><mml:msup><mml:mi>μ</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:msup><mml:mi>H</mml:mi><mml:mi>†</mml:mi></mml:msup><mml:mi>H</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msup><mml:mi>μ</mml:mi><mml:mrow><mml:mo>′</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mi>H</mml:mi><mml:mrow><mml:mo>′</mml:mo><mml:mi>†</mml:mi></mml:mrow></mml:msup><mml:msup><mml:mi>H</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>. We will consider <inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mrow><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup><mml:mo>≫</mml:mo><mml:msup><mml:mrow><mml:mi>μ</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>≫</mml:mo><mml:msup><mml:mrow><mml:mi>μ</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. One can view <inline-formula><mml:math display="inline"><mml:msup><mml:mi>μ</mml:mi><mml:mrow><mml:mo>′</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>-</mml:mo><mml:msup><mml:mi>μ</mml:mi><mml:mn>2</mml:mn></mml:msup></mml:math></inline-formula> as arising from the VEV of a <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>-odd scalar coupled to the Higgs fields in the far UV. It is then plausible that the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> breaking in the marginal couplings is as small as <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:msup><mml:mi>μ</mml:mi><mml:mrow><mml:mo>′</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo stretchy="false">/</mml:mo><mml:msubsup><mml:mi>M</mml:mi><mml:mi>p</mml:mi><mml:mn>2</mml:mn></mml:msubsup></mml:math></inline-formula>.</p><p>We now introduce a <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>-invariant QCD axion coupling, <disp-formula id="d4"><mml:math display="block"><mml:mrow><mml:mfrac><mml:mrow><mml:msub><mml:mrow><mml:mi>α</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mn>8</mml:mn><mml:mi>π</mml:mi></mml:mrow></mml:mfrac><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:mi>G</mml:mi><mml:mover accent="true"><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">˜</mml:mo></mml:mrow></mml:mover><mml:mo>+</mml:mo><mml:msup><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">˜</mml:mo></mml:mrow></mml:mover></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mo>.</mml:mo></mml:mrow></mml:math><label>(4)</label></disp-formula>The equality of the strong couplings indicated above is true in the far UV, by <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, but can run differently below <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:msup><mml:mi>μ</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>. For <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>μ</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:mo>&gt;</mml:mo><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">Λ</mml:mi></mml:mrow><mml:mrow><mml:mi>QCD</mml:mi></mml:mrow></mml:msub><mml:mo>≪</mml:mo><mml:msubsup><mml:mrow><mml:mi mathvariant="normal">Λ</mml:mi></mml:mrow><mml:mrow><mml:mi>QCD</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:msup><mml:mrow><mml:mi>q</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for all mirror quarks <inline-formula><mml:math display="inline"><mml:msup><mml:mi>q</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>. We can estimate the strong coupling scale <inline-formula><mml:math display="inline"><mml:msubsup><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>QCD</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:math></inline-formula> given <inline-formula><mml:math display="inline"><mml:msub><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>QCD</mml:mi></mml:msub></mml:math></inline-formula> using the 1-loop renormalization group (RG). The differential running at 1 loop depends on the quark and mirror quark masses in terms of <inline-formula><mml:math display="inline"><mml:mi>μ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msup><mml:mi>μ</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> but is insensitive to new model-dependent thresholds involving colored degrees of freedom needed to UV complete the nonrenormalizable axionic couplings, which do not get mass through electroweak symmetry breaking.</p><p>In the above regime the nonperturbative <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>QCD</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (pure glue) contribution to the axion potential near its minimum is given by lattice computation <xref ref-type="bibr" rid="c70">[70]</xref>, and continuum (<inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>MS</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="true">¯</mml:mo></mml:mrow></mml:mover></mml:mrow></mml:math></inline-formula>) matching <xref ref-type="bibr" rid="c71">[71]</xref>: <disp-formula id="d5"><mml:math display="block"><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="script">V</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:mo>=</mml:mo><mml:mn>0.3</mml:mn><mml:mtext> </mml:mtext><mml:mo stretchy="false">(</mml:mo><mml:mi>few</mml:mi><mml:mo>×</mml:mo><mml:msubsup><mml:mrow><mml:mi mathvariant="normal">Λ</mml:mi></mml:mrow><mml:mrow><mml:mi>QCD</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msubsup><mml:msup><mml:mrow><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:mi mathvariant="script">O</mml:mi><mml:mrow><mml:mo>[</mml:mo><mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:mi>a</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mo stretchy="false">¯</mml:mo></mml:mrow></mml:mover><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow></mml:msup><mml:mo>]</mml:mo></mml:mrow><mml:mo>,</mml:mo></mml:mrow></mml:math><label>(5)</label></disp-formula>where “few” <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:msubsup><mml:mi>α</mml:mi><mml:mn>3</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>0.4</mml:mn></mml:mrow></mml:msubsup></mml:math></inline-formula> is in detail the model-dependent conversion factor between the 1 loop and 2 loop estimates of the strong coupling scales.</p><p>Considering Eq. <xref ref-type="disp-formula" rid="d4">(4)</xref>, this immediately shows that the single QCD axion <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> solves the strong <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> problems of both the sectors at the same time by having the VEV <inline-formula><mml:math display="inline"><mml:mo stretchy="false">⟨</mml:mo><mml:mi>a</mml:mi><mml:mo stretchy="false">⟩</mml:mo><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula>. Although the two values of <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula> are identical for the two sectors in the UV, the breaking of the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> symmetry can make the two <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula>’s different below <inline-formula><mml:math display="inline"><mml:msup><mml:mi>μ</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>. However, RG running of <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover></mml:math></inline-formula> occurs at seven loops, and contributions from threshold corrections arise at four loops <xref ref-type="bibr" rid="c72">[72]</xref>. Thus, both of these effects, arising from renormalizable operators in SM and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>SM</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, are too small to be significant, even given the tight neutron EDM constraints.</p><p>However, higher dimensional operators, suppressed by the Planck scale, can make the two angles different. For example, the interactions <disp-formula id="d6"><mml:math display="block"><mml:mrow><mml:mfrac><mml:mrow><mml:msub><mml:mrow><mml:mi>α</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mn>8</mml:mn><mml:mi>π</mml:mi></mml:mrow></mml:mfrac><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:msup><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mi>†</mml:mi></mml:mrow></mml:msup><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:msubsup><mml:mrow><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac><mml:mi>G</mml:mi><mml:mover accent="true"><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">˜</mml:mo></mml:mrow></mml:mover><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:msup><mml:mrow><mml:msup><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow><mml:mrow><mml:mi>†</mml:mi></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow><mml:mrow><mml:msubsup><mml:mrow><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac><mml:msup><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mover accent="true"><mml:mrow><mml:mi>G</mml:mi></mml:mrow><mml:mrow><mml:mo accent="true" stretchy="false">˜</mml:mo></mml:mrow></mml:mover></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math><label>(6)</label></disp-formula>can give <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo>≠</mml:mo><mml:msup><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> upon the breaking of the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="double-struck">Z</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> symmetry. We need the splitting <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:msup><mml:mover accent="true"><mml:mi>θ</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo>′</mml:mo></mml:msup><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>10</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in order to maintain the axion mechanism to within current neutron EDM constraint. This implies <inline-formula><mml:math display="inline"><mml:msup><mml:mi>μ</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>&lt;</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>14</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>, and thus there is a maximal amount by which <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> can be made heavier. For further theoretical considerations see the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref>, which contains Refs. <xref ref-type="bibr" rid="c74 c75 c76">[74–76]</xref>.</p><p>From Eq. <xref ref-type="disp-formula" rid="d5">(5)</xref>, we see that the resulting axion mass is much larger than in the SM alone (for a given <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula>) so that it can be heavier than <inline-formula><mml:math display="inline"><mml:msub><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>QCD</mml:mi></mml:msub></mml:math></inline-formula>. This significantly weakens the existing experimental constraints and allows stronger couplings, <inline-formula><mml:math display="inline"><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula>, to the SM. The raising of the axion mass and lowering of <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula> clearly reduces the severity of the quality problem. This opens up a strongly motivated and new experimentally testable regime for the QCD axion, which we identify now.</p></sec><sec id="s4"><title specific-use="run-in">Constraints on parameter space.—</title><p>In Fig. <xref ref-type="fig" rid="f1">1</xref> we show the preferred parameter space for our model. We begin with the quality problem. We will choose as a benchmark a composite axion model for which PQ symmetry holds at the renormalizable level but can be violated at <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>=</mml:mo><mml:mn>6</mml:mn></mml:math></inline-formula>. Given Eq. <xref ref-type="disp-formula" rid="d3">(3)</xref>, this reintroduces the strong <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> problem in the region labeled “PQ Quality Problem” in Fig. <xref ref-type="fig" rid="f1">1</xref>. We cannot populate the area labeled “Below the QCD Axion line” as our mechanism can only make the axion heavier, and not lighter. In the area labeled “Higgs VEV Quality Problem,” <inline-formula><mml:math display="inline"><mml:mrow><mml:mo stretchy="false">⟨</mml:mo><mml:msup><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:mo stretchy="false">⟩</mml:mo><mml:mo>∼</mml:mo><mml:msup><mml:mrow><mml:mi>μ</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup><mml:mo>&gt;</mml:mo><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>14</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:mrow></mml:math></inline-formula> and Planck suppressed operators spoil the axion mechanism, as explained around Eq. <xref ref-type="disp-formula" rid="d6">(6)</xref>. Our effective field theory is only valid if <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:msubsup><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>QCD</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:math></inline-formula> which excludes the region shaded in cyan in Fig. <xref ref-type="fig" rid="f1">1</xref>. We are being agnostic about the origin of the axion coupling to QCD. Typically, the coupling is generated by integrating out colored fundamental fermions who get a mass <inline-formula><mml:math display="inline"><mml:mi>y</mml:mi><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>a</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="c77">[77]</xref>. Requiring that the Yukawa coupling <inline-formula><mml:math display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> of these fermions is smaller than <inline-formula><mml:math display="inline"><mml:mn>4</mml:mn><mml:mi>π</mml:mi></mml:math></inline-formula>, we have new colored particles below <inline-formula><mml:math display="inline"><mml:mn>4</mml:mn><mml:mi>π</mml:mi><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula>. Requiring that these colored fermions satisfy LHC constraints <xref ref-type="bibr" rid="c78 c79 c80 c81">[78–81]</xref> and are heavier than <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:mn>2</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi></mml:math></inline-formula> disfavors the region shown in Fig. <xref ref-type="fig" rid="f1">1</xref>. The regions labeled “<inline-formula><mml:math display="inline"><mml:mrow><mml:mtext>Astro</mml:mtext><mml:mo>+</mml:mo><mml:mtext>Cosmo</mml:mtext><mml:mo>+</mml:mo><mml:mtext>Beam</mml:mtext></mml:mrow></mml:math></inline-formula> Dump” and “Collider Searches” are ruled out due to a variety of supernova, stellar cooling, beam dump, collider, and cosmology constraints. All these constraints, along with original references, can be found in the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref> and references therein <xref ref-type="bibr" rid="c36 c82 c83 c84 c85 c86 c87 c88 c89 c90 c91 c92 c93 c94">[36,82–94]</xref>. We see then that the most favored region is given by <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub><mml:mo>∼</mml:mo><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi><mml:mtext>-</mml:mtext><mml:mi>TeV</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub><mml:mo>∼</mml:mo><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi><mml:mtext>-</mml:mtext><mml:mi>PeV</mml:mi></mml:mrow></mml:math></inline-formula>, ripe for collider exploration.</p><fig id="f1"><object-id>1</object-id><object-id pub-id-type="doi">10.1103/PhysRevLett.124.221801.f1</object-id><label>FIG. 1.</label><caption><p>The preferred model parameter regions for our high quality axion model. We require that no new colored particles exist with a mass below 2 TeV; higher dimensional operators involving the axion or the Higgs do not reintroduce the strong <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> problem, as well as several astrophysical, cosmological, and collider constraints.</p></caption><graphic xlink:href="e221801_1.eps"/></fig></sec><sec id="s5"><title specific-use="run-in">Phenomenology.—</title><p>We present a search strategy and discuss its feasibility for massive axions in the GeV to tens of GeV range, with decay constants ranging between 100 TeV and PeV, thereby covering a sizable portion of the open regime seen in Fig. <xref ref-type="fig" rid="f1">1</xref>. We note here that the axion predominantly decays into gluons which give rise to hadronic final states. Hence, with the production mode we consider below, the signal will be a displaced jet recoiling against prompt jet(s), where the displaced jet should contain at least three tracks from axion decay with the properties described below. The presence of a displaced vertex gives us a powerful discriminator against hadronic backgrounds while still having a sizable production rate. The existence of such a parameter regime, where the signal is produced with both a significant rate and with significant displacement, is nontrivial for the GeV-scale axion, or, in general, for any singly produced long-lived particles, given that the same small coupling controls the production rate and upper limit of the proper lifetime. The lever arm that offsets the small production coupling is provided by the immense gluon-parton luminosity at the LHC and other proton accelerator experiments.</p><p>The production rate of the axion at the 13 TeV LHC is <disp-formula id="und1"><mml:math display="block"><mml:mrow><mml:mi>σ</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>p</mml:mi><mml:mi>p</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:mi>a</mml:mi><mml:mo>+</mml:mo><mml:mi>X</mml:mi><mml:mo>;</mml:mo><mml:msub><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mi>T</mml:mi></mml:mrow></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mo>≃</mml:mo><mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:mo>×</mml:mo><mml:mn>0.7</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>fb</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>Here we have imposed a cut on the sum of transverse energy of hadronic activity, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula> and hence, the axion mass (<inline-formula><mml:math display="inline"><mml:mo>≲</mml:mo><mml:mn>20</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>) does not significantly affect the cross section. If one instead requires a leading (prompt) jet minimal <inline-formula><mml:math display="inline"><mml:msub><mml:mi>p</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:math></inline-formula> cut of 30 GeV, the cross section increases by around a factor of 3. For further details of the cross section calculation, done using <sc>m</sc>ad<sc>g</sc>raph5@<sc>nlo</sc> <xref ref-type="bibr" rid="c95">[95]</xref>, <sc>pythia</sc>8 <xref ref-type="bibr" rid="c96 c97">[96,97]</xref>, and <sc>delphes</sc>3 <xref ref-type="bibr" rid="c98">[98]</xref>, see the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref>. The lifetime of the axion can be approximated by <disp-formula id="d7"><mml:math display="block"><mml:mrow><mml:mi>c</mml:mi><mml:mi>τ</mml:mi><mml:mo>≃</mml:mo><mml:mn>0.8</mml:mn><mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:msub><mml:mrow><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi></mml:mrow></mml:mfrac><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mfrac><mml:mrow><mml:mn>2</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>a</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>mm</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math><label>(7)</label></disp-formula></p><p>A good signal trigger efficiency is critical given the above cross section, which can be achieved using the displaced track trigger discussed in Refs. <xref ref-type="bibr" rid="c99 c100">[99,100]</xref>. We follow this construction with conservative modifications to accommodate our signal. In detail, we require (i) At least three <inline-formula><mml:math display="inline"><mml:msub><mml:mi>p</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>2</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula> tracks within an Level-1 (L1) trigger jet, (ii) Among the above tracks, at least three of them have the transverse impact parameter <inline-formula><mml:math display="inline"><mml:msub><mml:mi>d</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>1</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>mm</mml:mi></mml:math></inline-formula>, (iii) The pseudorapidity of the tracks to be <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mi>η</mml:mi><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>2.4</mml:mn></mml:math></inline-formula>, (iv) The event has <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>. Additionally, in our analysis, we require decay location of axion candidates in the transverse plane with displacement <inline-formula><mml:math display="inline"><mml:msub><mml:mi>d</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>35</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi></mml:math></inline-formula> to have more than five hits in the trackers. This requirement of the number of hits for a displaced track has already been folded into to the L1 trigger rates dominated by the “fake-track” backgrounds, coming from misconnections of the tracker hits or instrumental noise. These requirements are sufficient to pass the L1 trigger with affordable rates below <inline-formula><mml:math display="inline"><mml:mo>≲</mml:mo><mml:mn>10</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>kHz</mml:mi></mml:math></inline-formula>. Such an L1 rate is dominated by backgrounds from fake tracks as per the displaced track trigger in Refs. <xref ref-type="bibr" rid="c99 c100">[99,100]</xref>. The requirement of three or more tracks can be passed quite easily for axion masses <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≳</mml:mo><mml:mi>few</mml:mi><mml:mtext>  </mml:mtext><mml:mi>GeV</mml:mi></mml:mrow></mml:math></inline-formula>. Other SM background from metastable SM hadron decays can be effectively vetoed with the number of displaced tracks and vertexing requirements; for more detailed considerations, see the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref> including Refs. <xref ref-type="bibr" rid="c101 c102 c103 c104">[101–104]</xref>.</p><p>The fake-track background is one of the most crucial for displaced vertex searches at the LHC at every stage of experimental analysis and is very large. We will use conservative estimates to suggest that this background can be cut to a small enough size to reveal the signal. Our estimates are not, however, a substitute for a full experimental analysis, which we hope to inspire. The key feature of these fake tracks is that they allow for a much larger reconstructed impact parameter than the SM background. Empirically, one can model them as tracks with flat distributions in the finite range in the following dimensions: track impact parameter (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>d</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>15</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi></mml:mrow></mml:math></inline-formula>), track curvature [<inline-formula><mml:math display="inline"><mml:mrow><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>∝</mml:mo><mml:mi>q</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi>T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:mn>1.8</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi mathvariant="normal">m</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math></inline-formula>], track eta <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:mi>η</mml:mi><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>2.4</mml:mn></mml:math></inline-formula>, track time <inline-formula><mml:math display="inline"><mml:msub><mml:mi>t</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>ns</mml:mi></mml:math></inline-formula>), and track <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> coordinate (<inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mi>z</mml:mi><mml:mn>0</mml:mn></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>15</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi></mml:math></inline-formula>). These definitions of L1 fake-track parameters are mainly based upon Ref. <xref ref-type="bibr" rid="c105">[105]</xref>. We note that these assumptions are rough and can vary based upon detector performance and collider environments, however, they can serve as a good benchmark to start the discussion of such LLP search strategies.</p><p>Nevertheless, the fake tracks that pass the above L1 trigger constitute huge background, amounting to about <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>10</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>kHz</mml:mi><mml:mo>×</mml:mo><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>8</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>sec</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>12</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> triples of fake tracks (in jets) at the HL-LHC. Combinations of SM displaced tracks and fake tracks are expected to give a subdominant background; for more discussions, see the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref>. At higher level triggers and in the analysis, one needs to suppress the background much further, to below a Hz while maintaining a high signal efficiency. Beyond all existing displaced trigger studies, we further demonstrate that it is possible to suppress these backgrounds using a 2D-4D displaced vertexing selection at a high-level trigger. We first solve for a 2D vertex by finding the best-fit point that minimizes the distances between the vertex and the tracks. Then we construct the 4D vertex of the system by extrapolating the 2D point in the transverse plane to the <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> direction and time direction by propagating the tracks. The time direction is defined as the timing information of each track with respect to the reference time, e.g., the beam-crossing time <xref ref-type="bibr" rid="c106">[106]</xref>.</p><p>Our 2D-4D displaced vertexing selection is defined as follows: (1) The 2D tracks fit a common vertex with standard deviation <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>d</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>1</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi></mml:math></inline-formula>; (2) The 2D common vertex has a minimal distance to the interaction point of 0.5 cm and maximal distance of 35 cm, <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>0.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>d</mml:mi></mml:mrow><mml:mrow><mml:mi>T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>35</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi></mml:mrow></mml:math></inline-formula>; (3) The 2D common vertex is significantly displaced away from the interaction point, <inline-formula><mml:math display="inline"><mml:msub><mml:mi>d</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>d</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>5</mml:mn></mml:math></inline-formula>; (4) The corresponding 4D vertex has a standard deviation in the <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> direction <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>d</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>5</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi></mml:math></inline-formula>; (5) The corresponding 4D vertex has a <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> direction location <inline-formula><mml:math display="inline"><mml:msub><mml:mi>d</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>20</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>cm</mml:mi></mml:math></inline-formula>; (6) The corresponding 4D vertex has a standard deviation in time <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>d</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>500</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>ps</mml:mi></mml:math></inline-formula>; (7) The corresponding 4D vertex has a time <inline-formula><mml:math display="inline"><mml:msub><mml:mi>d</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>1000</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>ps</mml:mi></mml:math></inline-formula>; (8) The tracks are within 0.4 in pseudorapidity of the reconstructed displaced jet direction <inline-formula><mml:math display="inline"><mml:mrow><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi>V</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>0.4</mml:mn></mml:mrow></mml:math></inline-formula> for all the three tracks; (9) The tracks are within 0.4 in azimuthal angle of the reconstructed displaced jet direction <inline-formula><mml:math display="inline"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mi>ϕ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>ϕ</mml:mi><mml:mi>V</mml:mi></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>0.4</mml:mn></mml:math></inline-formula> for all the three tracks, where <inline-formula><mml:math display="inline"><mml:msub><mml:mi>η</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:msub><mml:mi>ϕ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:math></inline-formula>) and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>η</mml:mi><mml:mi>V</mml:mi></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:msub><mml:mi>ϕ</mml:mi><mml:mi>V</mml:mi></mml:msub></mml:math></inline-formula>) are the pseudorapidity (azimuthal angle) of the displaced tracks and primary vertex, respectively.</p><p>Following the empirical model of fake-track distribution discussed above, we find that the combination of the transverse plane vertex fitting (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Cut</mml:mi><mml:mn>1</mml:mn><mml:mo>+</mml:mo><mml:mi>Cut</mml:mi><mml:mn>2</mml:mn><mml:mo>+</mml:mo><mml:mi>Cut</mml:mi><mml:mn>3</mml:mn></mml:mrow></mml:math></inline-formula>) provides a suppression factor of <inline-formula><mml:math display="inline"><mml:mn>8.2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Note, cuts 2 and 3 remove prompt SM backgrounds and processes involving shorter decay lengths, while Cut1 removes fake tracks. The combination of <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>-direction consistency (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Cut</mml:mi><mml:mn>4</mml:mn><mml:mo>+</mml:mo><mml:mi>Cut</mml:mi><mml:mn>5</mml:mn></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-direction consistency (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Cut</mml:mi><mml:mn>6</mml:mn><mml:mo>+</mml:mo><mml:mi>Cut</mml:mi><mml:mn>7</mml:mn></mml:mrow></mml:math></inline-formula>) provides <inline-formula><mml:math display="inline"><mml:mn>4.9</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mn>3.0</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> background suppression, respectively. Furthermore, the requirement for the displaced tracks pointing back to the primary vertex (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Cut</mml:mi><mml:mn>8</mml:mn><mml:mo>+</mml:mo><mml:mi>Cut</mml:mi><mml:mn>9</mml:mn></mml:mrow></mml:math></inline-formula>) provides <inline-formula><mml:math display="inline"><mml:mn>4.9</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>4</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> suppression. After taking into account the correlations between the selection cuts (see the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref>), the resulting overall suppression factor of the fake-track background from this 2D-4D vertex fitting procedure is <inline-formula><mml:math display="inline"><mml:mn>2.9</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>9</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. This means the background is reduced to <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>12</mml:mn></mml:mrow></mml:msup><mml:mo>×</mml:mo><mml:mn>2.9</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mo>-</mml:mo><mml:mn>9</mml:mn></mml:mrow></mml:msup><mml:mo>=</mml:mo><mml:mn>2900</mml:mn></mml:mrow></mml:math></inline-formula> events. A crucial consideration on top of the above background estimation is that it is using outer layers of the tracking information only. For the signal, there would be consistent energy deposition in the electromagnetic calorimeter and hadronic calorimeter, as well as inner tracker information, which will improve the spatial resolution of the displaced tracks and constitute a powerful consistency check and discrimination of signal from fake-track background. We further assume, but leave for the experiments to demonstrate, that the matching of the information between different subdetectors for all the tracks and as well the neutral hadrons, should be able to at least provide 1 order of magnitude fake-track background suppression per track, reducing our background estimate to <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>2900</mml:mn><mml:mo>×</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mo>-</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mo stretchy="false">)</mml:mo></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msup><mml:mo>≃</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:math></inline-formula> events. Hence, it is plausible that the fake-track background can be suppressed to negligible levels.</p><p>Depending on the detector performance at the HL-LHC, one can have 10–30 fake tracks per collision and the ranges in the fake-track distribution model may vary. The study in Ref. <xref ref-type="bibr" rid="c100">[100]</xref> showed that by requiring two fake tracks, one can have <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> background rate suppression and the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:math></inline-formula> cut provides <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> suppression, so the overall rate at L1 is around 10 kHz. Here the fake tracks are those which pass the L1 track fitting procedure as described in Ref. <xref ref-type="bibr" rid="c100">[100]</xref>, which requires the consistency between the track hits in the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>p</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:math></inline-formula> modules for the CMS detector. Our evaluation here conservatively assumes that the same level of suppression can be achieved by requiring three fake tracks. As shown in the discussion of the cross section in the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref>, such an <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:math></inline-formula> cut reduces the inclusive cross section by more than 2 orders of magnitude for the axion mass regions of interest. To show what one can achieve with a slightly less conservative trigger consideration, in the next section, we also consider a trigger with a leading-jet minimal <inline-formula><mml:math display="inline"><mml:msub><mml:mi>p</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:math></inline-formula> of 30 GeV, instead of the minimal <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:math></inline-formula> of 100 GeV, plus three displaced tracks. We assume the same level of the L1 rate and background can be maintained using advanced trigger developments such as matching information between different subdetectors.</p></sec><sec id="s6"><title specific-use="run-in">Results.—</title><p>After these considerations where we show that it is at least plausible to suppress the background to <inline-formula><mml:math display="inline"><mml:mi mathvariant="script">O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>10</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> level using vertex fitting and information matching between detectors, we give the estimated sensitivities for our signals at the HL-LHC with <inline-formula><mml:math display="inline"><mml:mn>3000</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msup><mml:mi>fb</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> integrated luminosity. We show in Fig. <xref ref-type="fig" rid="f2">2</xref> the reach of the proposed search with 3 and 10 signal events. These correspond to the required number of signal events for 95% C.L. exclusions for the two assumptions of 0 and 25 background events, respectively. As can be seen from Fig. <xref ref-type="fig" rid="f2">2</xref> the importance of experiments in actually reducing the background to <inline-formula><mml:math display="inline"><mml:mi mathvariant="script">O</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>10</mml:mn><mml:mo stretchy="false">)</mml:mo></mml:math></inline-formula> level is crucial to conduct such a high-quality axion search.</p><fig id="f2"><object-id>2</object-id><object-id pub-id-type="doi">10.1103/PhysRevLett.124.221801.f2</object-id><label>FIG. 2.</label><caption><p>The signal coverage in the <inline-formula><mml:math display="inline"><mml:msub><mml:mi>m</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>f</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:math></inline-formula> plane where the red and green contours correspond to requiring a leading jet with <inline-formula><mml:math display="inline"><mml:msub><mml:mi>p</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>30</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>, respectively. For both the red and green contours, we show 10 and 3 signal event regions that can be covered following the present work. The reference lines for various ALP proper lifetimes are shown in solid gray.</p></caption><graphic xlink:href="e221801_2.eps"/></fig><p>There are several unique features of the coverage plot in Fig. <xref ref-type="fig" rid="f2">2</xref>, which are different from the analogous results involving more common LLP searches where LLPs are pair produced. Understanding this will help in designing and optimizing future searches for GeV scale axions and, more generally, singly produced LLPs. First, the coverage has a strong dependence on the number of signal events needed, which is clearly shown by comparing the coverage between the shaded regions with different colors. The reason behind the strong dependence comes from our trigger requirement <inline-formula><mml:math display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>100</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula> or leading-jet <inline-formula><mml:math display="inline"><mml:msub><mml:mi>p</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>30</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math></inline-formula>. Given that the axion mass we are probing is much smaller than these scales, the production cross section remains approximately constant, as discussed around Eq. <xref ref-type="disp-formula" rid="d7">(7)</xref> and shown clearly in the Supplemental Material <xref ref-type="bibr" rid="c73">[73]</xref>. Second, the lower edge (low mass and low decay constant) of the coverage is determined by the minimal displacement requirement, below which the probability becomes too low for a GeV axion to be sufficiently displaced. Third, unlike most LLPs that are produced by stronger interactions than those involved in their decays, the upper edge (high mass and high decay constants) for our search is limited by the production rate of the axion.</p></sec><sec id="s7"><title specific-use="run-in">Discussion and outlook.—</title><p>The quest for axions is pressing. We have put forward a general theoretical structure involving a mirror sector in which a true QCD axion solves the strong <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math></inline-formula> problem while being very robust against the axion quality problem. We find that <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:mi>GeV</mml:mi></mml:math></inline-formula> axions with <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:mi>PeV</mml:mi></mml:math></inline-formula> decay constants lie at the heart of the motivated parameter space (see Fig. <xref ref-type="fig" rid="f1">1</xref>).</p><p>For <inline-formula><mml:math display="inline"><mml:mrow><mml:mo stretchy="false">∼</mml:mo><mml:mi>GeV</mml:mi></mml:mrow></mml:math></inline-formula> axions with <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo><mml:mi>PeV</mml:mi></mml:math></inline-formula> decay constants, the axion can be produced and detected at the LHC as a long-lived particle. This is a challenging long-lived particle search at the LHC. The production rate is highly suppressed by the same small coupling that leads to the displaced decay, implying that for reasonable rates, most decays will take place inside the LHC main detectors. Furthermore, there is only one low-mass displaced vertex in the event, while most other searches are for pair production of massive long-lived particles. We explored the dominant background of fake tracks and proposed a three-displaced-track strategy with 2D-4D displaced vertex reconstruction, demonstrating that the background can be feasibly suppressed. We believe that this makes the case for experimental exploration. An LLP search along the lines described in this Letter will require creative designs of the triggers and analysis at the LHC main detectors.</p><p>The codes for this Letter are available at Axion@LHC <xref ref-type="bibr" rid="c107">[107]</xref>.</p></sec></body><back><ack><p>We would like to thank Matthew Daniel Citron, Jared Evans, Yuri Gershtein, Simon Knapen, and Diego Redigolo for very useful comments on the draft. We would also like to thank Prateek Agrawal, Evan Berkowitz, Zohreh Davoudi, and Simone Pagan Griso for helpful discussions. This research was supported in part by the NSF Grants No. PHY-1620074, No. PHY-1914480, and No. PHY-1914731, and by the Maryland Center for Fundamental Physics (MCFP). A. H., Z. L., and R. S. acknowledge the hospitality of the Kavli Institute for Theoretical Physics, UC Santa Barbara, during the “Origin of the Vacuum Energy and Electroweak Scales” workshop, and the support by the NSF Grant No. PHY-174958. A. H. and Z. L. would also like to thank Pittsburgh Particle Physics Astrophysics and Cosmology Center (PITT-PACC), The Munich Institute for Astro- and Particle Physics (MIAPP), and Aspen Center for Physics (supported by NSF Grant No. PHY-1607611) for support from their programs and providing the environment for collaboration during various stages of this work.</p></ack><ref-list><ref id="c1"><label>[1]</label><mixed-citation publication-type="journal"><object-id>1</object-id><person-group person-group-type="author"><string-name>R. D. Peccei</string-name> and <string-name>H. R. 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