New constraints on the dark matter-neutrino and dark matter-photon scattering cross sections from TXS 0506+056

被引：17

作者：

Ferrer, Francesc ^{[1
,2
]}

Herrera, Gonzalo ^{[3
,4
]}

Ibarra, Alejandro ^{[3
]}

机构：

[1] Washington Univ, Dept Phys, St Louis, MO 63130 USA

[2] Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA

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

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

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2023年 / 05期

关键词：

astrophysical black holes; dark matter theory; ultra high energy photons and neutrinos; MODELS;

D O I：

10.1088/1475-7516/2023/05/057

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The flux of high energy neutrinos and photons produced in a blazar could get attenuated when they propagate through the dark matter spike around the central black hole and the halo of the host galaxy. Using the observation by IceCube of a few high-energy neutrino events from TXS 0506+056, and their coincident gamma ray events, we obtain new constraints on the dark matter-neutrino and dark matter-photon scattering cross sections. Our constraints are orders of magnitude more stringent than those derived from considering the attenuation through the intergalactic medium and the Milky Way dark matter halo. When the cross-section increases with energy, our constraints are also stronger than those derived from the CMB and large-scale structure.

引用

页数：13

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