Sterile neutrinos in cosmology

被引:163
|
作者
Abazajian, Kevork N. [1 ]
机构
[1] Univ Calif Irvine, Ctr Cosmol, Dept Phys & Astron, Irvine, CA 92697 USA
基金
美国国家科学基金会;
关键词
WARM DARK-MATTER; 3.5 KEV LINE; ASYMMETRY GENERATION; FINITE-TEMPERATURE; POWER SPECTRUM; ALPHA FOREST; BETA-DECAY; MASS; OSCILLATIONS; SEARCH;
D O I
10.1016/j.physrep.2017.10.003
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Sterile neutrinos are natural extensions to the standard model of particle physics in neutrino mass generation mechanisms. If they are relatively light, less than approximately 10 keV, they can alter cosmology significantly, from the early Universe to the matter and radiation energy density today. Here, we review the cosmological role such light sterile neutrinos can play from the early Universe, including production of keV-scale sterile neutrinos as dark matter candidates, and dynamics of light eV-scale sterile neutrinos during the weakly-coupled active neutrino era. We review proposed signatures of light sterile neutrinos in cosmic microwave background and large scale structure data. We also discuss keV-scale sterile neutrino dark matter decay signatures in X-ray observations, including recent candidate 3.5 keV X-ray line detections consistent with the decay of a similar to 7 keV sterile neutrino dark matter particle. (C) 2017 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 28
页数:28
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