Solar neutrino limit on axions and keV-mass bosons

被引：96

作者：

Gondolo, Paolo ^{[1
]}

Raffelt, Georg G. ^{[2
]}

机构：

[1] Univ Utah, Dept Phys, Salt Lake City, UT 84102 USA

[2] Max Planck Inst Phys Werner Heisenberg Inst, D-80805 Munich, Germany

来源：

PHYSICAL REVIEW D | 2009年 / 79卷 / 10期

关键词：

DARK-MATTER; SEARCH; CONVERSION; DETECTORS; BOUNDS;

D O I：

10.1103/PhysRevD.79.107301

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The all-flavor solar neutrino flux measured by the Sudbury Neutrino Observatory constrains nonstandard energy losses to less than about 10% of the Sun's photon luminosity, superseding a helioseismological argument and providing new limits on the interaction strength of low-mass particles. For the axion-photon coupling strength we find g(a gamma)< 7x10(-10) GeV-1. We also derive explicit limits on the Yukawa coupling to electrons of pseudoscalar, scalar, and vector bosons with keV-scale masses.

引用

页数：4

共 27 条

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