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AGN constraints on neutrino-dark matter scattering

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arxiv 2404.19471 v1 pith:5ICIT6C4 submitted 2024-04-30 astro-ph.HE hep-ph

James M. Cline This is my paper · ORCID
classification astro-ph.HEhep-ph
keywords darkconstraintsmatterscatteringactivebaryonblackblazar
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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.

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Cited by 1 Pith paper

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  1. Phenomenology of Neutrino-Dark Matter Interaction in DSNB and AGN

    hep-ph 2024-12 conditional novelty 5.0 of 10

    Upper limits on the scalar-dark-matter neutrino coupling are derived from DSNB attenuation projected for DUNE/Hyper-K and from IceCube data on NGC 1068 and TXS 0506+056, assuming DM spikes around AGN black holes.

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