Buyukcizmeci, N.Botvina, A. S.Mishustin, I. N.Ogul, R.2020-03-262020-03-2620101742-6588https://dx.doi.org/10.1088/1742-6596/202/1/012003https://hdl.handle.net/20.500.12395/254364th International Conference on Nuclear Physics in Astrophysics -- JUN 08-12, 2009 -- Lab Nazl Frascati, Frascati, ITALYThe 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.en10.1088/1742-6596/202/1/012003info:eu-repo/semantics/openAccessTowards the Equation of State for Dense Stellar MatterConference Object202N/AWOS:000287821100003N/A