2015/04/30 by Kenny C. Y. Ng, Shunsaku Horiuchi, Jennifer Gaskins +4 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Fermi Gamma-ray Space Telescope #Gamma ray #Gamma-ray burst #Neutrino #Neutrino detector #Neutrino oscillation #Particle Detector Development and Performance #Particle physics #Physics #Sterile neutrino #astro-ph.CO #hep-ph
paper · pdf · doi:10.1103/physrevd.92.043503
published as Phys. Rev. D 92, 043503 (2015) · 16 pages, 11 figures, references added, discussion expanded, some typos fixed, matches the published version
openalex publication_date 2015/08/04 · arxiv created 2015/08/06 · arxiv updated 2015/08/07 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
Surprisingly stringent bounds on sterile neutrino dark matter are obtained by searching for spectral lines from sterile neutrino dark matter in the 25---40 keV mass range using data from Fermi Gamma-ray Burst Monitor (GBM). The constraints represent an order of magnitude improvement over previous results.