期刊
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS
卷 145, 期 -, 页码 313-318出版社
ELSEVIER
DOI: 10.1016/j.nuclphysbps.2005.04.029
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Cosmology is at present one of the most powerful probes of neutrino properties. The advent of precision data from the cosmic microwave background and large scale structure has allowed for a very strong bound on the neutrino mass. Here, I review the status of cosmological bounds on neutrino properties with emphasis on mass bounds on light neutrinos.
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