NuSTAR Tests of Sterile-Neutrino Dark Matter: New Galactic Bulge Observations and Combined Impact

Aug 23, 2019
16 pages
Published in:
  • Phys.Rev.D 101 (2020) 10, 103011
  • Published: May 9, 2020
e-Print:

Citations per year

2019202120232025202505101520
Abstract: (APS)
We analyze two dedicated NuSTAR observations with exposure ∼190  ks located ∼10° from the Galactic plane, one above and the other below, to search for x-ray lines from the radiative decay of sterile-neutrino dark matter. These fields were chosen to minimize astrophysical x-ray backgrounds while remaining near the densest region of the dark matter halo. We find no evidence of anomalous x-ray lines in the energy range 5–20 keV, corresponding to sterile neutrino masses 10–40 keV. Interpreted in the context of sterile neutrinos produced via neutrino mixing, these observations provide the leading constraints in the mass range 10–12 keV, improving upon previous constraints in this range by a factor ∼2. We also compare our results to Monte Carlo simulations, showing that the fluctuations in our derived limit are not dominated by systematic effects. An updated model of the instrumental background, which is currently under development, will improve NuSTAR’s sensitivity to anomalous x-ray lines, particularly for energies 3–5 keV.
Note:
  • 16 pages, 5 figures. Text updated to match published version in PRD. Conclusions unchanged
  • Astrophysics and astroparticle physics
  • neutrino: sterile: mass
  • dark matter: halo
  • dark matter: annihilation
  • dark matter: decay
  • neutrino: mixing
  • numerical calculations: Monte Carlo
  • electron positron
  • energy resolution
  • anti-p