Neutrino Physics and the Primordial Elemental Abundances

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dc.creatorCardall, Christian Y.
dc.creatorFuller, George M.
dc.date1997-01-31
dc.date.accessioned2026-07-07T02:22:51Z
dc.date.available2026-07-07T02:22:51Z
dc.descriptionLimits can be placed on nonstandard neutrino physics when big bang nucleosynthesis (BBN) calculations employing standard neutrino physics agree with the observationally inferred primordial abundances of deuterium (D), $^3$He, $^4$He, and $^7$Li. These constraints depend most sensitively on the abundances of D and $^4$He. New observational determinations of the primordial D and/or $^4$He abundances could force revisions in BBN constraints on nonstandard neutrino physics.
dc.descriptionTo appear in the proceedings of the Texas Symposium on Relativistic Astrophysics held in Chicago, Dec. 15-20 1996. 3 pages, latex, uses included style file sprocl.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9702001
dc.identifierhttp://arxiv.org/abs/astro-ph/9702001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11028
dc.subjectAstrophysics
dc.titleNeutrino Physics and the Primordial Elemental Abundances
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