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Thermal axion production at low temperatures: a smooth treatment of the QCD phase transition

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arxiv 2108.04259 v3 pith:GNQMTPVE submitted 2021-08-09 hep-ph astro-ph.CO

Thermal axion production at low temperatures: a smooth treatment of the QCD phase transition

classification hep-ph astro-ph.CO
keywords axionproductiontemperaturesphasequantifyratethermaltransition
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study thermal axion production around the confinement scale. At higher temperatures, we extend current calculations to account for the masses of heavy quarks, whereas we quantify production via hadron scattering at lower temperatures. Matching our results between the two opposite regimes provides us with a continuous axion production rate across the QCD phase transition. We employ such a rate to quantify the axion contribution to the effective number of neutrino species.

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Cited by 3 Pith papers

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    For axion masses above 0.1 eV, cosmology provides the strongest known limits on axion couplings to muons, taus, and flavor-violating tau channels, excluding decay constants up to 10^8 GeV.

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    HTL computation of soft axion rates shows interpolation between k=0 and k≈ω, raising ΔN_eff from ~0.03 to ~0.04 for light QCD axions at fa=4×10^8 GeV.

  3. Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments

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    The meV axion window is presented as a coherent, cross-validated search program in which string theory, stellar cooling, dark matter, and new detector concepts converge on the same mass range.