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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Official URL: http://dx.doi.org/10.1016/j.astropartphys.2011.07....
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 |
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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: | 07 Nov 2023 12:58 |
URI: | https://orca.cardiff.ac.uk/id/eprint/105340 |
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