期刊
ASTROPARTICLE PHYSICS
卷 30, 期 4, 页码 192-195出版社
ELSEVIER
DOI: 10.1016/j.astropartphys.2008.09.005
关键词
Cosmology; Cosmic microwave background anisotropies; Hot dark matter; Inflation
We report new constraints on the reheating temperature of the universe by analyzing the recent cosmic microwave background (CMB) data from the WMAP five year survey. From WMAP-5 data alone we found an upper limit at 95% c.l. of T-rh > 2 MeV, while including external priors from the SDSS red luminous galaxy survey and age constraints improves the limit to T-rh > 3.2 MeV (again at 95% c.l.). Future analysis from combined CMB and weak lensing surveys as Planck and DUNE will improve the the constraints by a factor similar to 2. We test the stability of the current upper limits on neutrino masses from cosmology under the hypothesis of non-standard thermal neutrino background. (C) 2008 Elsevier B.V. All rights reserved.
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