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All-sky limits on sterile neutrino galactic dark matter obtained with SRG/ART-XC after two years of operations

E. I. Zakharov1,2,3,*, V. V. Barinov4,3,†, R. A. Burenin1,2,‡, D. S. Gorbunov3,5,§, R. A. Krivonos1,3,∥, A. Yu. Tkachenko1, V. A. Arefiev1, E. V. Filippova1, S. A. Grebenev1 et al.

A. A. Lutovinov1, I. A. Mereminsky1, S. Yu. Sazonov1, A. N. Semena1, A. E. Shtykovsky1,2, and R. A. Sunyaev1

  • 1Space Research Institute of the Russian Academy of Sciences, Moscow 117997, Russia
  • 2National Research University Higher School of Economics, Moscow 101000, Russia
  • 3Institute for Nuclear Research of the Russian Academy of Sciences, Moscow 117312, Russia
  • 4Physics Department, M. V. Lomonosov Moscow State University, Leninskie Gory, Moscow 119991, Russia
  • 5Moscow Institute of Physics and Technology, Dolgoprudny 141700, Russia

  • *ezakharov@cosmos.ru
  • †barinov.vvl@gmail.com
  • ‡rodion@hea.iki.rssi.ru
  • §gorby@ms2.inr.ac.ru
  • ∥krivonos@cosmos.ru

Phys. Rev. D 109, L021301 – Published 2 January, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.L021301

Abstract

Dark matter sterile neutrinos radiatively decay in the Milky Way, which can be tested with searches for almost monochromatic photons in the x-ray cosmic spectrum. We analyse the data of SRG/ART-XC telescope operated for two years in the all-sky survey mode. With no significant hints in the Galactic diffuse x-ray spectrum we explore models with sterile neutrino masses in 12–40 keV range and exclude corresponding regions of sterile-active neutrino mixing.

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