Cosmological and astrophysical neutrino mass measurements

Abazajian, K.N., Calabrese, Erminia ORCID: https://orcid.org/0000-0003-0837-0068, 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:	24 Nov 2024 18:30
URI:	https://orca.cardiff.ac.uk/id/eprint/105340

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