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Strategy for Searching for a Dark Matter Sterile Neutrino
Author(s) -
Alexey Boyarsky,
A. Neronov,
Oleg Ruchayskiy,
Mikhail Shaposhnikov,
I. Tkachev
Publication year - 2006
Publication title -
physical review letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.688
H-Index - 673
eISSN - 1079-7114
pISSN - 0031-9007
DOI - 10.1103/physrevlett.97.261302
Subject(s) - sterile neutrino , physics , dark matter , neutrino , warm dark matter , galaxy , radiative transfer , astrophysics , range (aeronautics) , particle physics , dwarf galaxy , hot dark matter , neutrino oscillation , cosmology , dark energy , optics , materials science , composite material
We propose a strategy of how to look for dark matter (DM) particlespossessing a radiative decay channel and derive constraints on their parametersfrom observations of X-rays from our own Galaxy and its dwarf satellites. Whenapplied to the sterile neutrinos in keV mass range, it allows a significantimprovement of restrictions to its parameters, as compared with previous works.Comment: 5 pp, revtex; v3: 1-sigma limits have been replaced by more conservative 3-sigma limits, a picture illustrating the data analysis methods has been ade

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