A Dark Matter Signature for Condensed Neutrinos
High Energy Astrophysical Phenomena
2016-08-31 v1
Abstract
We derive the signature for condensed neutrino objects (CNOs) as the primary source of Dark Matter. Restricting our source data to minimize systematic errors, we find that by just using weak lensing data and Sunyaev-Zel'dovich data, that there may be a weak CNO signature.
Keywords
Cite
@article{arxiv.1604.05716,
title = {A Dark Matter Signature for Condensed Neutrinos},
author = {P. D. Morley and D. J. Buettner},
journal= {arXiv preprint arXiv:1604.05716},
year = {2016}
}
Comments
21 pages, 5 figures. Accepted for publication in the International Journal of Modern Physics D (IJMPD)