Astrophysical axion bounds

被引：605

作者：

Raffelt, Georg G. ^{[1
]}

机构：

[1] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

来源：

AXIONS: THEORY, COSMOLOGY, AND EXPERIMENTAL SEARCHES | 2008年 / 741卷

关键词：

D O I：

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

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Axion emission by hot and dense plasmas is a new energy-loss channel for stars. Observable 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. I review and update these arguments and summarize the resulting axion constraints.

引用

页码：51 / 71

页数：21

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