Cosmological neutrinos

By S. Hannestad. 2004

463 citations recorded by the source corpus.

The current status of neutrino cosmology is reviewed, from the question of neutrino decoupling and the presence of sterile neutrinos to the effects of neutrinos on the cosmic microwave background and large scale structure. Particular emphasis is put on cosmological neutrino mass measurements.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/6a7225e58503ad034aa999063b768ed883df18c9

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Nuclear and High Energy Physics

Citations in the corpus

Thermalisation of light sterile neutrinos in the early universe (2012, background): “an Affleck-Dine mechanism [58] or other models that are able to produce large lepton asymmetries and small baryonic ones [59, 60].”
The Search for Heavy Majorana Neutrinos (2009, unknown): “[48]).”
Global constraints on absolute neutrino masses and their ordering (2017, background): “[16, 63–67]), letting cosmology to strongly bound the neutrino mass scale, indeed providing the current strongest (albeit model dependent) bounds on Σ.”
A facility to search for hidden particles at the CERN SPS: the SHiP physics case (2015, background): “Since rp is directly linked to the observable deuterium and helium abundances, this gives us the possibility of testing the existence of HNL using observations of the light elements [619].”
The Hubble Constant (2010, background): “Star Evolution, p. 11 New York: Academic Press Sandage(1968)Sandage AR, Tammann GA. 1968.”
Relic backgrounds of gravitational waves from cosmic turbulence (2002, background): “[ 16 ]). The seeds of the neutrino domains are tiny fluctuations in the baryon num-”