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• W3100507440 endingPage "L134" @default.
• W3100507440 startingPage "L131" @default.
• W3100507440 abstract "The standard model of particle physics assumes that neutrinos are massless, although adding non-zeros is required by the experimentally established phenomenon of neutrino oscillations requires neutrinos to have non-zero mass. Sterile neutrinos (or right-handed neutrinos) are a good warm dark matter candidate. We find that the excess of the intensity in the 8.7 keV line (at the energy of the FeXXVI Ly$gamma$ line) in the spectrum of the Galactic center observed by the Suzaku X-ray mission cannot be explained by standard ionization and recombination processes. We suggest that the origin of this excess is via decays of sterile neutrinos with a mass of 17.4 keV and estimate the value of the mixing angle. The estimated value of the mixing angle $sin^2(2theta)=(4.1 pm 2.2)times10^{-12}$ lies in the allowed region of the mixing angle of dark matter sterile neutrino with a mass of 17-18 keV." @default.
• W3100507440 created "2020-11-23" @default.
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• W3100507440 date "2010-11-24" @default.
• W3100507440 modified "2023-10-18" @default.
• W3100507440 title "CAN THE EXCESS IN THE Fe XXVI Lyγ LINE FROM THE GALACTIC CENTER PROVIDE EVIDENCE FOR 17 keV STERILE NEUTRINOS?" @default.
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• W3100507440 doi "https://doi.org/10.1088/2041-8205/725/2/l131" @default.
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