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.
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页数：4
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