Latest Cosmological Constraints on the Densities of Hot and Cold Dark Matter

Author
Abstract

As experimentalists step up their pursuit of cold dark matter particles and neutrino masses, cosmological constraints are tightening. We compute the joint constraints on 11 cosmological parameters from cosmic microwave background and large scale structure data, and find that at 95\% confidence, the total (cold+hot) dark matter density is h2$\Omega$dm = 0.20+.12−.10 with at most 38\% of it being hot (due to neutrinos). A few assumptions, including negligible neutrinos, tighten this measurement to h2$\Omega$dm = 0.13+0.04−0.02, i, e., 2.4 \texttimes 10−27kg/m3 give or take 20\%.

Year of Conference
2001
Volume
409
Start Page or Article ID
128-137
Date Published
2001-01
Publisher
Springer Berlin Heidelberg
Conference Location
Berlin, Heidelberg
ISBN Number
978-3-662-04587-9
DOI
10.1007/978-3-662-04587-9_12
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Publication Status
JILA PI
JILA Topics
Conference Proceedings