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Comment on axion emission rates in stars
Phys. Rev. D 34, 3927 – Published 15 December, 1986
DOI: https://doi.org/10.1103/PhysRevD.34.3927
Abstract
It is pointed out that the emission of axions from stellar plasmas and their reabsorption is stimulated by the thermal radiation field in processes with final-state photons. An expression for the bremsstrahlung emissivity of a stellar plasma is given for the nonrelativistic, degenerate regime. Some other aspects of a recent calculation by Pantziris and Kang of stellar axion emissivities are discussed.
Original Article
Axion emission rates in stars and constraints on its mass
Phys. Rev. D 33, 3509 (1986)
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