From nuclear multifragmentation reactions to supernova explosions

Simple item page
dc.creatorMishustin, Igor N.
dc.date2008-03-10
dc.date.accessioned2026-07-07T09:26:06Z
dc.date.available2026-07-07T09:26:06Z
dc.descriptionIn this talk I discuss properties of hot stellar matter at sub-nuclear densities which is formed in supernova explosions. I emphasize that thermodynamic conditions there are rather similar to those created in the laboratory by intermediate-energy heavy-ion collisions. Theoretical methods developed for the description of multi-fragment final states in such reactions can be used also for description of the stellar matter. I present main steps of the statistical approach to the equation of state and nuclear composition, dealing with an ensemble of nuclear species instead of one "average" nucleus.
dc.description11 pages, 5 figures, invited talk at the International Workshop on Multifragmentation (GANIL, Caen, France, November 4-7, 2007)
dc.identifierhttps://arxiv.org/abs/0803.1388
dc.identifierhttp://arxiv.org/abs/0803.1388
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/156633
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleFrom nuclear multifragmentation reactions to supernova explosions
dc.typetext

Files

Collections

arXiv