Big Bang Nucleosynthesis and the Observed Abundances of Light Elements

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dc.creatorHogan, Craig J.
dc.date1996-09-19
dc.date.accessioned2026-07-07T02:21:56Z
dc.date.available2026-07-07T02:21:56Z
dc.descriptionThe predictions of Standard Big Bang Nucleosynthesis are summarized and compared with observations of abundances of helium in HII regions, deuterium in quasar absorbers, deuterium and helium-3 in the Galaxy, and lithium in metal-poor stars. It is concluded that the prospects are good for a precise test of the theory.
dc.description13 pages, Latex. Contribution to the Princeton meeting, ``Critical Dialogues in Cosmology''
dc.identifierhttps://arxiv.org/abs/astro-ph/9609138
dc.identifierhttp://arxiv.org/abs/astro-ph/9609138
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10691
dc.subjectAstrophysics
dc.titleBig Bang Nucleosynthesis and the Observed Abundances of Light Elements
dc.typetext

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