Comment on "Heavy element production in inhomogeneous big bang nucleosynthesis"

Simple item page
dc.creatorRauscher, T.
dc.date2006-04-12
dc.date.accessioned2026-07-07T10:23:00Z
dc.date.available2026-07-07T10:23:00Z
dc.descriptionThe work of Matsuura et al. [Phys. Rev. D 72, 123505 (2005); astro-ph/0507439] claims that heavy nuclei could have been produced in a combined p- and r-process in very high baryon density regions of an inhomogeneous big bang. However, they do not account for observational constraints and previous studies which show that such high baryon density regions did not significantly contribute to big bang abundances.
dc.description2 pages, submitted to Phys. Rev. D on Feb 23, 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0604264
dc.identifierhttp://arxiv.org/abs/astro-ph/0604264
dc.identifierPhys.Rev.D75:068301,2007
dc.identifierdoi:10.1103/PhysRevD.75.068301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175673
dc.subjectAstrophysics
dc.titleComment on "Heavy element production in inhomogeneous big bang nucleosynthesis"
dc.typetext

Files

Collections

arXiv