Minimal sterile neutrino dark matter

被引:28
|
作者
Bringmann, Torsten [1 ,2 ]
Depta, Paul Frederik [3 ]
Hufnagel, Marco [4 ]
Kersten, Joern [5 ,6 ]
Ruderman, Joshua T. [7 ]
Schmidt-Hoberg, Kai [8 ]
机构
[1] Univ Oslo, Dept Phys, POB 1048, N-0316 Oslo, Norway
[2] CERN, Theoret Phys Dept, Geneva 23, CH-1211 Geneva, Switzerland
[3] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany
[4] Univ Libre Bruxelles, Serv Phys Theor, Blvd Triomphe,CP225, B-1050 Brussels, Belgium
[5] Korea Inst Adv Study, Seoul 02455, South Korea
[6] Univ Bergen, Dept Phys & Technol, N-5020 Bergen, Norway
[7] NYU, Ctr Cosmol & Particle Phys, Dept Phys, New York, NY 10003 USA
[8] Deutsch Elektronen Synchrotron DESY, Notkestr 85, D-22607 Hamburg, Germany
基金
美国国家科学基金会; 新加坡国家研究基金会;
关键词
MASS; ETHOS;
D O I
10.1103/PhysRevD.107.L071702
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose a novel mechanism to generate sterile neutrinos vs in the early Universe, by converting ordinary neutrinos va in scattering processes vsva -> vsvs. After initial production by oscillations, this leads to an exponential growth in the vs abundance. We show that such a production regime naturally occurs for self-interacting vs, and that this opens up significant new parameter space where vs make up all of the observed dark matter. Our results provide strong motivation to further push the sensitivity of X-ray line searches, and to improve on constraints from structure formation.
引用
收藏
页数:8
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