Neutrino Mass from Cosmology

Neutrinos can play an important role in the evolution of the universe, modifying some of the cosmological observables. In this contribution we summarize the main aspects of cosmological relic neutrinos, and we describe how the precision of present cosmological data can be used to learn about neutrin...

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Main Authors: Julien Lesgourgues, Sergio Pastor
Format: Article
Language:English
Published: Wiley 2012-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2012/608515
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author Julien Lesgourgues
Sergio Pastor
author_facet Julien Lesgourgues
Sergio Pastor
author_sort Julien Lesgourgues
collection DOAJ
description Neutrinos can play an important role in the evolution of the universe, modifying some of the cosmological observables. In this contribution we summarize the main aspects of cosmological relic neutrinos, and we describe how the precision of present cosmological data can be used to learn about neutrino properties, in particular their mass, providing complementary information to beta decay and neutrinoless double-beta decay experiments. We show how the analysis of current cosmological observations, such as the anisotropies of the cosmic microwave background or the distribution of large-scale structure, provides an upper bound on the sum of neutrino masses of order 1 eV or less, with very good perspectives from future cosmological measurements which are expected to be sensitive to neutrino masses well into the sub-eV range.
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institution Kabale University
issn 1687-7357
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series Advances in High Energy Physics
spelling doaj-art-48c106ae684140afa2dd7b759f4ddf382025-02-03T05:51:52ZengWileyAdvances in High Energy Physics1687-73571687-73652012-01-01201210.1155/2012/608515608515Neutrino Mass from CosmologyJulien Lesgourgues0Sergio Pastor1Theory Division, CERN, 1211 Geneva 23, SwitzerlandInstituto de Física Corpuscular, CSIC-Universitat de València, Apartado de Correos 22085, 46071 Valencia, SpainNeutrinos can play an important role in the evolution of the universe, modifying some of the cosmological observables. In this contribution we summarize the main aspects of cosmological relic neutrinos, and we describe how the precision of present cosmological data can be used to learn about neutrino properties, in particular their mass, providing complementary information to beta decay and neutrinoless double-beta decay experiments. We show how the analysis of current cosmological observations, such as the anisotropies of the cosmic microwave background or the distribution of large-scale structure, provides an upper bound on the sum of neutrino masses of order 1 eV or less, with very good perspectives from future cosmological measurements which are expected to be sensitive to neutrino masses well into the sub-eV range.http://dx.doi.org/10.1155/2012/608515
spellingShingle Julien Lesgourgues
Sergio Pastor
Neutrino Mass from Cosmology
Advances in High Energy Physics
title Neutrino Mass from Cosmology
title_full Neutrino Mass from Cosmology
title_fullStr Neutrino Mass from Cosmology
title_full_unstemmed Neutrino Mass from Cosmology
title_short Neutrino Mass from Cosmology
title_sort neutrino mass from cosmology
url http://dx.doi.org/10.1155/2012/608515
work_keys_str_mv AT julienlesgourgues neutrinomassfromcosmology
AT sergiopastor neutrinomassfromcosmology