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arXiv · hep-ph/0611350

Astrophysical Axion Bounds

Georg G. Raffelt
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Abstract

Axion emission by hot and dense plasmas is a new energy-loss channel for stars. Observational consequences include a modification of the solar sound-speed profile, an increase of the solar neutrino flux, a reduction of the helium-burning lifetime of globular-cluster stars, accelerated white-dwarf cooling, and a reduction of the supernova SN 1987A neutrino burst duration. We review and update these arguments and summarize the resulting axion constraints.

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Georg G. Raffelt. 2006-11-28. Astrophysical Axion Bounds. https://doi.org/10.1007/978-3-540-73518-2_3

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