Particle Physics from Stars

dc.creatorRaffelt, G.
dc.date1999-03-24
dc.date.accessioned2026-07-07T10:33:50Z
dc.date.available2026-07-07T10:33:50Z
dc.descriptionLow-mass particles such as neutrinos, axions, other Nambu-Goldstone bosons and gravitons are produced in the hot and dense interior of stars. Therefore, astrophysical arguments constrain the properties of these particles in ways which are often complementary to cosmological arguments and to laboratory experiments. This review provides an update on the most important stellar-evolution limits and discusses them in the context of other information from cosmology and laboratory experiments.
dc.description46 pages, including 14 eps figures, prepared for vol.49 of the Annual Review of Nuclear and Particle Science (1999)
dc.identifierhttps://arxiv.org/abs/hep-ph/9903472
dc.identifierhttp://arxiv.org/abs/hep-ph/9903472
dc.identifierAnn.Rev.Nucl.Part.Sci.49:163-216,1999
dc.identifierdoi:10.1146/annurev.nucl.49.1.163
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179262
dc.subjectHigh Energy Physics - Phenomenology
dc.titleParticle Physics from Stars
dc.typetext

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