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Nucleon-Nucleon Bremsstrahlung emission of massive Axion
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We consider the problem of axion production by bremsstrahlung emission in a nuclear medium. The usual assumption of a massless axion is replaced by more general hypotheses, so that we can describe the emission process for axions with mass up to a few MeV. We point out that in certain physical situations the contribution from non-zero mass is non-negligible. In particular, in the mechanism for the production of Gamma Ray Bursts via emission of heavy axions the axion mass m_a ~ 1MeV is comparable with the temperature of the nuclear medium and thus can not be disregarded. Looking at our results we find, in fact, a fairly considerable reduction of the axion luminosity in that mechanism.
Forward citations
Cited by 2 Pith papers
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Disentangling axion-like particle couplings to nucleons via a delayed signal in Super-Kamiokande from a future supernova
A future nearby supernova could reveal sub-MeV axion-like particles through a delayed ~30 MeV photon signal in Super-Kamiokande and Hyper-Kamiokande, probing couplings down to about 3 x 10^-6.
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Probing a diffuse flux of axion-like particles from galactic supernovae with neutrino water Cherenkov detectors
MeV-mass axion-like particles from galactic supernovae can form a diffuse flux detectable via a p -> p gamma in water Cherenkov detectors, and Super-Kamiokande data exclude a new region of the ALP parameter space.
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