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Cosmological and astrophysical neutrino mass measurements

Abazajian, K.N., Calabrese, Erminia, Cooray, A., De Bernardis, F., Dodelson, S., Friedland, A., Fuller, G.M., Hannestad, S., Keating, B.G., Linder, E.V., Lunardini, C., Melchiorri, A., Miquel, R., Pierpaoli, E., Pritchard, J., Serra, P., Takada, M. and Wong, Y.Y.Y. 2011. Cosmological and astrophysical neutrino mass measurements. Astroparticle Physics 35 (4) , pp. 177-184. 10.1016/j.astropartphys.2011.07.002

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Abstract

Cosmological and astrophysical measurements provide powerful constraints on neutrino masses complementary to those from accelerators and reactors. Here we provide a guide to these different probes, for each explaining its physical basis, underlying assumptions, current and future reach. Highlights ► Neutrinos leave a distinct imprint on the large scale structure of the Universe. ► Large surveys are sensitive to the sum of the neutrino masses. ► We collect and explain current and future constraints from different probes of the structure of the Universe.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: Elsevier
ISSN: 0927-6505
Date of First Compliant Deposit: 9 October 2017
Date of Acceptance: 12 July 2011
Last Modified: 16 Oct 2017 11:17
URI: http://orca-mwe.cf.ac.uk/id/eprint/105340

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