http://arxiv.org/abs/1604.05716
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.
P. Morley and D. Buettner
Thu, 21 Apr 16
23/61
Comments: 21 pages, 5 figures. Accepted for publication in the International Journal of Modern Physics D (IJMPD)
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