Towards the Equation of State for Dense Stellar Matter

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dc.contributor.authorBuyukcizmeci, N.
dc.contributor.authorBotvina, A. S.
dc.contributor.authorMishustin, I. N.
dc.contributor.authorOgul, R.
dc.date.accessioned2020-03-26T18:05:28Z
dc.date.available2020-03-26T18:05:28Z
dc.date.issued2010
dc.departmentSelçuk Üniversitesien_US
dc.description4th International Conference on Nuclear Physics in Astrophysics -- JUN 08-12, 2009 -- Lab Nazl Frascati, Frascati, ITALYen_US
dc.description.abstractThe thermal nuclear multifragmentation reaction can be used to investigate the nuclear liquid-gas phase coexistence region and its relation to the astrophysical processes such as the collapse of massive stars, and the supernova type-II explosions. We have performed some calculations to estimate stellar equation of state (EOS) on the basis of statistical multifragmentation model.en_US
dc.description.sponsorshipBAP [09701267]; TUBITAK-BIDEBTurkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK)en_US
dc.description.sponsorshipN. Buyukcizmeci thanks BAP (Coord. of Scientific Research Projects of Selcuk University-09701267), and A. S. Botvina thanks TUBITAK-BIDEB for support that made his visit possible, to Selcuk University, Konya.en_US
dc.identifier.doi10.1088/1742-6596/202/1/012003en_US
dc.identifier.issn1742-6588en_US
dc.identifier.scopusqualityN/Aen_US
dc.identifier.urihttps://dx.doi.org/10.1088/1742-6596/202/1/012003
dc.identifier.urihttps://hdl.handle.net/20.500.12395/25436
dc.identifier.volume202en_US
dc.identifier.wosWOS:000287821100003en_US
dc.identifier.wosqualityN/Aen_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherIOP PUBLISHING LTDen_US
dc.relation.ispartofNUCLEAR PHYSICS IN ASTROPHYSICS IV (NPAIV 2009)en_US
dc.relation.ispartofseriesJournal of Physics Conference Series
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.selcuk20240510_oaigen_US
dc.titleTowards the Equation of State for Dense Stellar Matteren_US
dc.typeConference Objecten_US

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