Light element synthesis in baryon isocurvature models

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dc.creatorLohiya, D.
dc.creatorKumar, P.
dc.date2006-02-20
dc.date.accessioned2026-07-07T07:00:47Z
dc.date.available2026-07-07T07:00:47Z
dc.descriptionThe prejudice against baryon isocurvature models is primarily because of their inconsistency with early universe light element nucleosynthesis results. We propose that incipient low metallicity (Pop II) star forming regions can be expected to have environments conducive to Deuterium production by spallation, up to levels observed in the universe.
dc.description10 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0602425
dc.identifierhttp://arxiv.org/abs/astro-ph/0602425
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108085
dc.subjectAstrophysics
dc.titleLight element synthesis in baryon isocurvature models
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