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Neutrinos in astrophysics

The amount of 4He synthesised in the "big bang" is sensitive to the early particle content and to the expansion rate. If there was indeed a "big bang", surprisingly strong conclusions can be drawn about the number of species of neutrinos, and about the possibility that such parti...

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Detalles Bibliográficos
Autor principal: Rees, Martin J
Lenguaje:eng
Publicado: CERN 1979
Materias:
Acceso en línea:http://cds.cern.ch/record/2239320
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author Rees, Martin J
author_facet Rees, Martin J
author_sort Rees, Martin J
collection CERN
description The amount of 4He synthesised in the "big bang" is sensitive to the early particle content and to the expansion rate. If there was indeed a "big bang", surprisingly strong conclusions can be drawn about the number of species of neutrinos, and about the possibility that such particles have non-zero rest mass. The dynamics of supernovae are sensitive to the det~ils of neutrino physics; such explosions would yield IO L-1053 ergs of -v IO Mev neutrinos, in a burst lasting a few milliseconds. Galactic nuclei, cosmic ray sources and other high energy cosmic phenomena could yield a low background of~ 10 Gev neutrinos.
id oai-inspirehep.net-148972
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1979
publisher CERN
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spelling oai-inspirehep.net-1489722019-09-30T06:29:59Zhttp://cds.cern.ch/record/2239320engRees, Martin JNeutrinos in astrophysicsAstrophysics and AstronomyThe amount of 4He synthesised in the "big bang" is sensitive to the early particle content and to the expansion rate. If there was indeed a "big bang", surprisingly strong conclusions can be drawn about the number of species of neutrinos, and about the possibility that such particles have non-zero rest mass. The dynamics of supernovae are sensitive to the det~ils of neutrino physics; such explosions would yield IO L-1053 ergs of -v IO Mev neutrinos, in a burst lasting a few milliseconds. Galactic nuclei, cosmic ray sources and other high energy cosmic phenomena could yield a low background of~ 10 Gev neutrinos.CERNoai:inspirehep.net:1489721979
spellingShingle Astrophysics and Astronomy
Rees, Martin J
Neutrinos in astrophysics
title Neutrinos in astrophysics
title_full Neutrinos in astrophysics
title_fullStr Neutrinos in astrophysics
title_full_unstemmed Neutrinos in astrophysics
title_short Neutrinos in astrophysics
title_sort neutrinos in astrophysics
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/2239320
work_keys_str_mv AT reesmartinj neutrinosinastrophysics