High-quality composite Pati-Salam axion

We present a composite QCD axion model where the Peccei-Quinn symmetry emerges as a high-quality, accidental symmetry. The axion potential is only modified by eight-fermion, dimension-12 operators, which if present at the Planck scale, allow for axion dark matter from misalignment while solving the strong <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mi>C</a:mi> <a:mi>P</a:mi> </a:math> problem. The model is an <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mi>SU</c:mi> <c:mo stretchy="false">(</c:mo> <c:msub> <c:mi>N</c:mi> <c:mi>c</c:mi> </c:msub> <c:mo stretchy="false">)</c:mo> </c:math> gauge theory with ten flavors where the Pati-Salam unified subgroup <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"> <g:mi>SO</g:mi> <g:mo stretchy="false">(</g:mo> <g:mn>6</g:mn> <g:mo stretchy="false">)</g:mo> <g:mo>×</g:mo> <g:mi>SO</g:mi> <g:mo stretchy="false">(</g:mo> <g:mn>4</g:mn> <g:mo stretchy="false">)</g:mo> <g:mo>⊂</g:mo> <g:mi>SU</g:mi> <g:mo stretchy="false">(</g:mo> <g:mn>10</g:mn> <g:msub> <g:mo stretchy="false">)</g:mo> <g:mi>L</g:mi> </g:msub> </g:math> and <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"> <o:mi>Sp</o:mi> <o:mo stretchy="false">(</o:mo> <o:mn>10</o:mn> <o:mo stretchy="false">)</o:mo> <o:mo>⊂</o:mo> <o:mi>SU</o:mi> <o:mo stretchy="false">(</o:mo> <o:mn>10</o:mn> <o:msub> <o:mo stretchy="false">)</o:mo> <o:mi>R</o:mi> </o:msub> </o:math> are weakly gauged. The dynamics breaks <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:mi>SU</u:mi> <u:mo stretchy="false">(</u:mo> <u:mn>10</u:mn> <u:msub> <u:mo stretchy="false">)</u:mo> <u:mi>L</u:mi> </u:msub> <u:mo>×</u:mo> <u:mi>SU</u:mi> <u:mo stretchy="false">(</u:mo> <u:mn>10</u:mn> <u:msub> <u:mo stretchy="false">)</u:mo> <u:mi>R</u:mi> </u:msub> <u:mo stretchy="false">→</u:mo> <u:mi>SU</u:mi> <u:mo stretchy="false">(</u:mo> <u:mn>10</u:mn> <u:msub> <u:mo stretchy="false">)</u:mo> <u:mi>V</u:mi> </u:msub> </u:math> and the weakly gauged groups to <db:math xmlns:db="http://www.w3.org/1998/Math/MathML" display="inline"> <db:mi mathvariant="normal">U</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>3</db:mn> <db:mo stretchy="false">)</db:mo> <db:mo>×</db:mo> <db:mi mathvariant="normal">U</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>2</db:mn> <db:mo stretchy="false">)</db:mo> <db:mo>⊃</db:mo> <db:mi>SU</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>3</db:mn> <db:msub> <db:mo stretchy="false">)</db:mo> <db:mi>c</db:mi> </db:msub> <db:mo>×</db:mo> <db:mi>SU</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>2</db:mn> <db:msub> <db:mo stretchy="false">)</db:mo> <db:mi>L</db:mi> </db:msub> <db:mo>×</db:mo> <db:mi mathvariant="normal">U</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>1</db:mn> <db:msub> <db:mo stretchy="false">)</db:mo> <db:mi>Y</db:mi> </db:msub> </db:math> , with the QCD axion identified as one of the Nambu-Goldstone bosons. This axion has a relatively large coupling to photons while a residual <sb:math xmlns:sb="http://www.w3.org/1998/Math/MathML" display="inline"> <sb:msub> <sb:mover accent="true"> <sb:mi>θ</sb:mi> <sb:mo stretchy="false">¯</sb:mo> </sb:mover> <sb:mi>eff</sb:mi> </sb:msub> </sb:math> may be just below the current limit on the neutron electric dipole moment. If the dimension-12 operators are present near the grand unified theory scale, they can cause domain wall networks to decay, allowing for axion dark matter even for the postinflationary scenario.

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Journal
Physical review. D/Physical review. D.
Published
2025-10-14
DOI
https://doi.org/10.1103/f1dg-n9h7
Citations
4
Primary Topic
Dark Matter and Cosmic Phenomena
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article
Field-Weighted Citation Impact
7.48

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article

High-quality composite Pati-Salam axion

Tony Gherghetta A, Hitoshi Murayama, Pablo Quílez
4 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
7.48
article

High-quality composite Pati-Salam axion

Tony Gherghetta A, Hitoshi Murayama, Pablo Quílez
article en
4 citations

Abstract

We present a composite QCD axion model where the Peccei-Quinn symmetry emerges as a high-quality, accidental symmetry. The axion potential is only modified by eight-fermion, dimension-12 operators, which if present at the Planck scale, allow for axion dark matter from misalignment while solving the strong <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mi>C</a:mi> <a:mi>P</a:mi> </a:math> problem. The model is an <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mi>SU</c:mi> <c:mo stretchy="false">(</c:mo> <c:msub> <c:mi>N</c:mi> <c:mi>c</c:mi> </c:msub> <c:mo stretchy="false">)</c:mo> </c:math> gauge theory with ten flavors where the Pati-Salam unified subgroup <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"> <g:mi>SO</g:mi> <g:mo stretchy="false">(</g:mo> <g:mn>6</g:mn> <g:mo stretchy="false">)</g:mo> <g:mo>×</g:mo> <g:mi>SO</g:mi> <g:mo stretchy="false">(</g:mo> <g:mn>4</g:mn> <g:mo stretchy="false">)</g:mo> <g:mo>⊂</g:mo> <g:mi>SU</g:mi> <g:mo stretchy="false">(</g:mo> <g:mn>10</g:mn> <g:msub> <g:mo stretchy="false">)</g:mo> <g:mi>L</g:mi> </g:msub> </g:math> and <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"> <o:mi>Sp</o:mi> <o:mo stretchy="false">(</o:mo> <o:mn>10</o:mn> <o:mo stretchy="false">)</o:mo> <o:mo>⊂</o:mo> <o:mi>SU</o:mi> <o:mo stretchy="false">(</o:mo> <o:mn>10</o:mn> <o:msub> <o:mo stretchy="false">)</o:mo> <o:mi>R</o:mi> </o:msub> </o:math> are weakly gauged. The dynamics breaks <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:mi>SU</u:mi> <u:mo stretchy="false">(</u:mo> <u:mn>10</u:mn> <u:msub> <u:mo stretchy="false">)</u:mo> <u:mi>L</u:mi> </u:msub> <u:mo>×</u:mo> <u:mi>SU</u:mi> <u:mo stretchy="false">(</u:mo> <u:mn>10</u:mn> <u:msub> <u:mo stretchy="false">)</u:mo> <u:mi>R</u:mi> </u:msub> <u:mo stretchy="false">→</u:mo> <u:mi>SU</u:mi> <u:mo stretchy="false">(</u:mo> <u:mn>10</u:mn> <u:msub> <u:mo stretchy="false">)</u:mo> <u:mi>V</u:mi> </u:msub> </u:math> and the weakly gauged groups to <db:math xmlns:db="http://www.w3.org/1998/Math/MathML" display="inline"> <db:mi mathvariant="normal">U</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>3</db:mn> <db:mo stretchy="false">)</db:mo> <db:mo>×</db:mo> <db:mi mathvariant="normal">U</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>2</db:mn> <db:mo stretchy="false">)</db:mo> <db:mo>⊃</db:mo> <db:mi>SU</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>3</db:mn> <db:msub> <db:mo stretchy="false">)</db:mo> <db:mi>c</db:mi> </db:msub> <db:mo>×</db:mo> <db:mi>SU</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>2</db:mn> <db:msub> <db:mo stretchy="false">)</db:mo> <db:mi>L</db:mi> </db:msub> <db:mo>×</db:mo> <db:mi mathvariant="normal">U</db:mi> <db:mo stretchy="false">(</db:mo> <db:mn>1</db:mn> <db:msub> <db:mo stretchy="false">)</db:mo> <db:mi>Y</db:mi> </db:msub> </db:math> , with the QCD axion identified as one of the Nambu-Goldstone bosons. This axion has a relatively large coupling to photons while a residual <sb:math xmlns:sb="http://www.w3.org/1998/Math/MathML" display="inline"> <sb:msub> <sb:mover accent="true"> <sb:mi>θ</sb:mi> <sb:mo stretchy="false">¯</sb:mo> </sb:mover> <sb:mi>eff</sb:mi> </sb:msub> </sb:math> may be just below the current limit on the neutron electric dipole moment. If the dimension-12 operators are present near the grand unified theory scale, they can cause domain wall networks to decay, allowing for axion dark matter even for the postinflationary scenario.

Physical review. D/Physical review. D.Vol. 112(9)
University of Minnesota (US), Lawrence Berkeley National Laboratory (US), Kavli Institute for the Physics and Mathematics of the Universe (JP), University of Minnesota System (US), University of California System (US), University of California San Diego (US), The University of Tokyo (JP), University of California, Berkeley (US)
National Science Foundation, U.S. Department of Energy, University of Minnesota, CERN, European Commission, Ministry of Education, Culture, Sports, Science and Technology, Office of Science, Japan Society for the Promotion of Science, High Energy Physics
Openalex Percentile: Top 3%
Dark Matter and Cosmic Phenomena
7.48
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