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Astrophysics > High Energy Astrophysical Phenomena

Title: AGN constraints on neutrino-dark matter scattering

Abstract: The IceCube collaboration has identified neutrinos of energy $\sim 10-100$ TeV from the blazar TXS 0506+056 and the active galaxy NGC 1068, which must have traveled through a dense dark matter spike surrounding the supermassive black holes that power the galactic nuclei. We use this to set new constraints on dark matter-neutrino scattering, and interpret the results in terms of a dark photon that couples to baryon minus lepton number.
Comments: 4.1 pages, 4 figures. Talk given at Moriond VHEPU based on arXiv:2209.02713 and arXiv:2301.08756
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Phenomenology (hep-ph)
Report number: CERN-TH-2024-053
Cite as: arXiv:2404.19471 [astro-ph.HE]
  (or arXiv:2404.19471v1 [astro-ph.HE] for this version)

Submission history

From: James Cline [view email]
[v1] Tue, 30 Apr 2024 11:37:20 GMT (2144kb,D)

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