Cosmic Matter Distribution: Cosmic Baryon Budget Revisited

Simple item page
dc.creatorFukugita, Masataka
dc.date2003-12-19
dc.date.accessioned2026-07-07T02:11:40Z
dc.date.available2026-07-07T02:11:40Z
dc.descriptionThe cosmic baryon budget is revisited using modern observations that have become available since our first publication. I also present an estimate for the heavy element abundance. An increased accuracy in the accounting of the baryon budget reveals `missing baryons', which amount to $\approx 35$% of the total. This would provide an interesting test for models of the cosmic structure formation.
dc.descriptionInvited Talk given at IAU Symposium 220, "Dark Matter in Galaxies", Sydney, 21-25 July, 2003. To be published in the Proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0312517
dc.identifierhttp://arxiv.org/abs/astro-ph/0312517
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7174
dc.subjectAstrophysics
dc.titleCosmic Matter Distribution: Cosmic Baryon Budget Revisited
dc.typetext

Files

Collections

arXiv