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We strengthen the cosmological bound on the axion mass, by solving the momentum-dependent Boltzmann equations for axion-pion scatterings and by using a phenomenological production rate derived from pion-pion scattering data, overcoming the breakdown of chiral perturbation theory.
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1999
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E. Masso, F. Rota, and G. Zsembinszki, On axion thermalization in the early universe, Phys. Rev. D 66
2002
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J. R. Pelaez and F. J. Yndurain, The Pion-pion scattering amplitude, Phys. Rev. D 71
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2016
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N. Aghanim et al. (Planck), Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641
2021
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2021
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