pith. sign in

arxiv: astro-ph/0106108 · v3 · submitted 2001-06-06 · 🌌 astro-ph · hep-ph

Constraining the window on sterile neutrinos as warm dark matter

classification 🌌 astro-ph hep-ph
keywords steriledarkmatterneutrinoneutrinoswarmallowedastronomical
0
0 comments X
read the original abstract

Sterile neutrinos may be one of the best Warm Dark Matter candidates we have today. Both lower and upper bounds on the mass of the sterile neutrino come from astronomical observations. We show that the proper inclusion of the neutrino momentum distribution reduces the allowed region to be 2.6 keV < m < 5 keV for the simplest models. A search for a spectral line with E=m/2 is thus more interesting than ever before.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Early Growth of Structure in Warm Wave Dark Matter

    astro-ph.CO 2025-06 conditional novelty 6.0

    Derives suppression of adiabatic perturbations and scale-dependent growth of isocurvature power in warm wave dark matter, verifies with Schrödinger-Poisson simulations, and proposes an analytic halo mass function.