Sterile neutrino dark matter production in the neutrino-phillic two Higgs doublet model

被引:22
作者
Adulpravitchai, Adisorn [1 ]
Schmidt, Michael A. [2 ]
机构
[1] Chulalongkorn Univ, Dept Phys, Fac Sci, Bangkok 10330, Thailand
[2] Univ Sydney, Sch Phys, ARC Ctr Excellence Particle Phys Terascale, Sydney, NSW 2006, Australia
基金
澳大利亚研究理事会;
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM; Neutrino Physics; OSCILLATIONS; GALAXIES;
D O I
10.1007/JHEP12(2015)023
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Sterile Neutrinos with a mass in the keV range form a good candidate for dark matter. They are naturally produced from neutrino oscillations via their mixing with the active neutrinos. However the production via non-resonant neutrino oscillations has recently been ruled out. The alternative production via Higgs decay is negligibly small compared to neutrino oscillations. We show that in the neutrino-phillic two Higgs doublet model, the contribution from Higgs decay can dominate over the contribution from neutrino oscillations and evade all constraints. We also study the free-streaming horizon and find that a sterile neutrino mass in the range of 4 to 53 keV leads to warm dark matter.
引用
收藏
页码:1 / 21
页数:21
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