Constraining dark matter-neutrino interactions with IceCube-170922A

被引：42

作者：

Choi, Ki-Young ^{[1
]}

Kim, Jongkuk ^{[1
]}

Rott, Carsten ^{[1
]}

机构：

[1] Sungkyunkwan Univ, Inst Basic Sci, Phys Res Div BK21, Dept Phys, 2066 Seobu Ro, Suwon 16419, Gyeong Gi Do, South Korea

来源：

PHYSICAL REVIEW D | 2019年 / 99卷 / 08期

基金：

新加坡国家研究基金会;

关键词：

D O I：

10.1103/PhysRevD.99.083018

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Astrophysical neutrinos travel long distances from their sources to the Earth traversing dark matter halos of clusters of galaxies and that of our own Milky Way. The interaction of neutrinos with dark matter may affect the flux of neutrinos. The recent multimessenger observation of a high energy neutrino, IceCubc-170922A, can give a robust upper bound sigma/M-dm less than or similar to 5.1 x 10(-23) cm(2)/GeV on the interaction between neutrino and dark matter at a neutrino energy of 290 TeV allowing 90% suppression. Combining the constraints from cosmic microwave background and Large Scale Structure at different neutrino energies, we can constrain models of dark matter-neutrino interactions.

引用

页数：5

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