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Intimate Relationship between Sterile Neutrino Dark Matter andΔNeff
Physical Review Letters ( IF 8.1 ) Pub Date : 2021-07-20 , DOI: 10.1103/physrevlett.127.041101
Kevin J Kelly 1 , Manibrata Sen 2, 3 , Yue Zhang 4
Affiliation  

The self-interacting neutrino hypothesis is well motivated for addressing the tension between the origin of sterile neutrino dark matter and indirect detection constraints. It can also result in a number of testable signals from the laboratories to the cosmos. We show that, in a broad class of models, where the sterile neutrino dark matter relic density is generated by a light neutrinophilic mediator, there must be a lower bound on the amount of extra radiation in early Universe, in particular, ΔNeff>0.12 at the cosmic microwave background (CMB) epoch. This lower bound will be further strengthened with an improved x-ray search at the Athena observatory. Such an intimate relationship will be unambiguously tested by the upcoming CMB Stage 4 project.

中文翻译:

不育中微子暗物质与ΔNeff的密切关系

自相互作用中微子假说很好地解决了惰性中微子暗物质起源与间接检测约束之间的紧张关系。它还可以产生许多从实验室到宇宙的可测试信号。我们表明,在一大类模型中,无菌中微子暗物质残余密度是由轻中微子介质产生的,早期宇宙中的额外辐射量必须有一个下限,特别是,ΔN效果>0.12在宇宙微波背景 (CMB) 时代。随着雅典娜天文台 X 射线搜索的改进,这一下限将得到进一步加强。即将到来的CMB第四阶段项目将明确测试这种亲密关系。
更新日期:2021-07-20
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