Properties of stellar matter in supernova explosions and nuclear multifragmentation

Simple item page
dc.creatorBotvina, A. S.
dc.creatorMishustin, I. N.
dc.creatorTrautmann, W.
dc.date2006-12-12
dc.date.accessioned2026-07-07T07:35:45Z
dc.date.available2026-07-07T07:35:45Z
dc.descriptionDuring the collapse of massive stars, and the supernova type-II explosions, stellar matter reaches densities and temperatures which are similar to the ones obtained in intermediate-energy nucleus-nucleus collisions. The nuclear multifragmentation reactions can be used for determination of properties of nuclear matter at subnuclear densities, in the region of the nuclear liquid-gas phase transition. It is demonstrated that the modified properties of hot nuclei (in particular, their symmetry energy) extracted from the multifragmentation data can essentially influence nuclear composition of stellar matter. The effects on weak processes, and on the nucleosynthesis are also discussed.
dc.description6 pages, 4 figures, a talk at the International Conference on Nucleus-Nucleus Collisions, Rio de Janeiro, Brazil, 2006
dc.identifierhttps://arxiv.org/abs/nucl-th/0612055
dc.identifierhttp://arxiv.org/abs/nucl-th/0612055
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120196
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleProperties of stellar matter in supernova explosions and nuclear multifragmentation
dc.typetext

Files

Collections

arXiv