Astrophysical Axion Bounds

Details Astrophysical Axion Bounds Astrophysical Axion Bounds

2006-11-28

arxiv.org/abs/hep-ph/0611350v1

Lect.Notes Phys.741:51-71,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

Contribution to Axion volume of Lecture Notes in Physics, 20 pages, 3 figures

Scientific paper

10.1007/978-3-540-73518-2_3

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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