Detecting sterile dark matter in space
Abstract
Space-based instruments provide new and, in some cases, unique opportunities to search for dark matter. In particular, if dark matter comprises sterile neutrinos, the x ray detection of their decay line is the most promising strategy for discovery. Sterile neutrinos with masses in the keV range could solve several long-standing astrophysical puzzles, from supernova asymmetries and the pulsar kicks to star formation, reionization, and baryogenesis. The best current limits on sterile neutrinos come from Chandra and XMM-Newton. Future advances can be achieved with a high-resolution x-ray spectrometry in space.
Cite
@article{arxiv.astro-ph/0608096,
title = {Detecting sterile dark matter in space},
author = {Alexander Kusenko},
journal= {arXiv preprint arXiv:astro-ph/0608096},
year = {2008}
}
Comments
11 pages, 1 figure, to appear in proceedings "From Quantum to Cosmos: fundametal physics research in space", Washington, DC, May 22-24, 2006