Naturally astrophobic QCD axion

被引:0
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作者
Marcin Badziak
Keisuke Harigaya
机构
[1] University of Warsaw,Institute of Theoretical Physics, Faculty of Physics
[2] University of Chicago,Department of Physics
[3] University of Chicago,Enrico Fermi Institute
[4] University of Chicago,Kavli Institute for Cosmological Physics
[5] The University of Tokyo Institutes for Advanced Study,Kavli Institute for the Physics and Mathematics of the Universe (WPI)
[6] The University of Tokyo,undefined
关键词
Axions and ALPs; Rare Decays;
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摘要
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. We reexamine next-to-leading order corrections to the couplings of the axion with nucleons and photons and show that the axion decay constant may be as small as 107 GeV. It is also possible to suppress the coupling with the photon so that the decay constant is even smaller and minimal axiogenesis works. In this scenario, the axion has a mass above 1 eV and may be directly detected via absorption of axion dark matter. Flavor-violating axion couplings are generically predicted in our model, but we show that they may be naturally and sufficiently suppressed. We discuss the implications of the hints for anomalous cooling in several stellar environments to our model.
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