Tidal disruption events and dark matter scatterings with neutrinos and photons

被引：6

作者：

Fujiwara, Motoko ^{[1
]}

Herrera, Gonzalo ^{[2
,3
]}

机构：

[1] Tech Univ Munich, Phys Dept, James Franck Str, D-85748 Garching, Germany

[2] Ctr Neutrino Phys, Phys Dept, Dept Phys, Munchen, Blacksburg, VA 24061 USA

[3] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Fohringer Ring 6, D-80805 Munich, Germany

来源：

PHYSICS LETTERS B | 2024年 / 851卷

关键词：

HIGH-ENERGY NEUTRINO; BLACK-HOLES; EMISSION; STARS; GALAXIES; PRODUCE; MASSES; RAYS;

D O I：

10.1016/j.physletb.2024.138573

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Stars can be tidally disrupted when passing near a black hole, and the debris can induce a flux of high-energy neutrinos. It has been discussed that there are hints in IceCube data of high-energy neutrinos produced in Tidal Disruption Events. The emitting region of neutrinos and photons in these astrophysical events is likely to be located in the vicinity of the central black hole, where the dark matter density might be significantly larger than in the outer regions of the galaxy. We explore the potential attenuation of the emitted neutrino and photon fluxes due to interactions with dark matter particles around the supermassive black hole of the host galaxies of AT2019dsg, AT2019fdr and AT2019aalc, and study the implications for some well-motivated models of dark matter-neutrino and dark matter-photon interactions. Furthermore, we discuss the complementarity of our constraints with values of the dark matter-neutrino scattering cross section proven to alleviate some cosmological tensions.

引用

页数：8

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