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Light axions can potentially leave a cosmic background, just like neutrinos.
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D. Baumann, D. Green and B. Wallisch, New Target for Cosmic Axion Searches , Phys. Rev. Lett. 117
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2001
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E. Masso, F. Rota and G. Zsembinszki, On axion thermalization in the early universe , Phys. Rev. D66
2002
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2002
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G. D’Ambrosio, G. Giudice, G. Isidori and A. Strumia, Minimal flavor violation: An Effective field theory approach , Nucl. Phys. B 645
2002
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C.A. Baker et al., An Improved Experimental Limit on the Electric Dipole Moment of the Neutron , Phys. Rev. Lett. 97
2006
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2007
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M. Gorghetto, E. Hardy and G. Villadoro, More Axions from Strings , 2007.04990
2007
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2016
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J.L. Bernal, L. Verde and A.G. Riess, The trouble with H 0 H_{0} , JCAP 1610
2016
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A. Sedrakian, Axion Cooling of Neutron Stars , Phys. Rev. D93
2016
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2016
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2017
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M. Bauer, M. Neubert and A. Thamm, Collider Probes of Axion-Like Particles , JHEP 12
2017
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F. Arias-Aragon and L. Merlo, The Minimal Flavour Violating Axion , JHEP 10
2017
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2017
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2017
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2017
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2018
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2018
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2018
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M. Gorghetto, E. Hardy and G. Villadoro, Axions from Strings: the Attractive Solution , JHEP 07
2018
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T. Vachaspati, A.E. Everett and A. Vilenkin, Radiation From Vacuum Strings and Domain Walls , Phys. Rev. D 30
2046
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