TY - JOUR
T1 - Bounds on neutrino-DM interactions from TXS 0506+056 neutrino outburst
AU - Zapata, Gabriel D.
AU - Jones-Pérez, Joel
AU - Gago, Alberto M.
N1 - Publisher Copyright:
© 2025 The Author(s)
PY - 2025/7/1
Y1 - 2025/7/1
N2 - We constrain the neutrino-dark matter cross-section using the 13±5 neutrino event excess observed by IceCube in 2014-2015 from the direction of the blazar TXS 0506+056. Our analysis takes advantage of the dark matter overdensity spike surrounding the supermassive black hole at the center of the blazar. In our results, we take into account uncertainties related to the different types of neutrino emission models and the features of the dark matter spike, considering cross-sections that scale with energy as σ ∝ (Eν /E 0)n , for values of n = 1, 0, -1, -2. In our best-case scenario, we obtain limits competitive with those derived from other active galaxies, tidal disruption events (TDEs), and the IC-170922A event.
AB - We constrain the neutrino-dark matter cross-section using the 13±5 neutrino event excess observed by IceCube in 2014-2015 from the direction of the blazar TXS 0506+056. Our analysis takes advantage of the dark matter overdensity spike surrounding the supermassive black hole at the center of the blazar. In our results, we take into account uncertainties related to the different types of neutrino emission models and the features of the dark matter spike, considering cross-sections that scale with energy as σ ∝ (Eν /E 0)n , for values of n = 1, 0, -1, -2. In our best-case scenario, we obtain limits competitive with those derived from other active galaxies, tidal disruption events (TDEs), and the IC-170922A event.
KW - active galactic nuclei
KW - dark matter theory
KW - ultra high energy photons and neutrinos
UR - https://www.scopus.com/pages/publications/105010697714
U2 - 10.1088/1475-7516/2025/07/042
DO - 10.1088/1475-7516/2025/07/042
M3 - Article
AN - SCOPUS:105010697714
SN - 1475-7516
VL - 2025
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
IS - 7
M1 - 042
ER -