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We present a QCD axion model where the couplings of the axion to nucleons, electrons, and muons are naturally suppressed because of the appropriate choice of the Peccei-Quinn charges of the Standard Model fermions.
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K. Harigaya and J. M. Leedom, QCD Axion Dark Matter from a Late Time Phase Transition , JHEP 06
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M. Dine, Problems of naturalness: Some lessons from string theory , in Conference on Topics in Quantum Gravity , 7, 1992, hep-th/9207045
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1994
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1999
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2017
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N. Iwamoto, Nucleon-nucleon bremsstrahlung of axions and pseudoscalar particles from neutron star matter , Phys. Rev. D 64
2001
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2001
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2002
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2018
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L. Di Luzio, F. Mescia, E. Nardi, P. Panci and R. Ziegler, Astrophobic Axions , Phys. Rev. Lett. 120
2018
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2018
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2018
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A. Sedrakian, Axion cooling of neutron stars. II. Beyond hadronic axions , Phys. Rev. D 99
2019
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2019
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L. B. Leinson, Impact of axions on the Cassiopea A neutron star cooling , JCAP 09
2021
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2021
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2021
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2021
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K. Harigaya and I. R. Wang, Axiogenesis from S U ( 2 ) R SU(2)_{R} phase transition , JHEP 10
2021
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R. T. Co, K. Harigaya, Z. Johnson and A. Pierce, R-parity violation axiogenesis , JHEP 11
2021
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K. Nakayama and W. Yin, Hidden photon and axion dark matter from symmetry breaking , JHEP 10
2021
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R. T. Co, T. Gherghetta and K. Harigaya, Axiogenesis with a heavy QCD axion , JHEP 10
2022
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F. D’Eramo and S. Yun, Flavor violating axions in the early Universe , Phys. Rev. D 105
2022
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J. Kawamura and S. Raby, Lepto-axiogenesis in minimal SUSY KSVZ model , JHEP 04
2022
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