Towards the Equation of State for Dense Stellar Matter

被引：1

作者：

Buyukcizmeci, N. ^{[1
]}

Botvina, A. S. ^{[2
]}

Mishustin, I. N. ^{[3
,4
]}

Ogul, R. ^{[1
]}

机构：

[1] Selcuk Univ, Dept Phys, TR-42079 Konya, Turkey

[2] Russian Acad Sci, Inst Nucl Res, Y Moscow 117312, Russia

[3] J W Geothe Univ, Frankfurt Inst Adv Studies, D-60438 Frankfurt, Germany

[4] Kurashov Inst, Russian Res Ctr, Moscow 123182, Russia

来源：

NUCLEAR PHYSICS IN ASTROPHYSICS IV (NPAIV 2009) | 2010年 / 202卷

关键词：

SUPERNOVA; NUCLEI;

D O I：

10.1088/1742-6596/202/1/012003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The 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.

引用

页数：4

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