Freeze-in and freeze-out of sterile neutrino dark matter

被引:0
|
作者
Coy, Rupert [1 ]
Schmidt, Michael A. [2 ]
机构
[1] Univ Libre Bruxelles, Serv Phys Theor, Blvd Triomphe,CP225, B-1050 Brussels, Belgium
[2] Univ New South Wales, Sch Phys, Sydney Consortium Particle Phys & Cosmol, Sydney, NSW 2052, Australia
基金
澳大利亚研究理事会;
关键词
dark matter theory; physics of the early universe; neutrino theory; FINITE-TEMPERATURE; GREEN-FUNCTIONS; FIELD-THEORY; DISCONTINUITIES; OSCILLATIONS;
D O I
10.1088/1475-7516/2022/08/070
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A sterile neutrino with a keV-scale mass is a compelling dark matter candidate. We propose a new production mechanism involving the decay and annihilation of a complex scalar singlet with a Higgs portal coupling which develops a vacuum expectation value. The interactions of the resulting pseudo Nambu-Goldstone boson may thermalise the dark sector. We determine the region of parameter space where dark sector thermalisation is reached and discuss the most relevant cosmological observables. The scenario can be considered as the combination of a freeze-in of the dark sector followed by relativistic freeze-out.
引用
收藏
页数:34
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