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.
- Wong, Y.Y.Y.
DOIAbstract
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
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