TABULATED EQUATION OF STATE FOR SUPERNOVA MATTER INCLUDING FULL NUCLEAR ENSEMBLE

被引：26
作者：
Buyukcizmeci, N. [1 ,2 ]
Botvina, A. S. [1 ,2 ,3 ,4 ]
Mishustin, I. N. [1 ,2 ,5 ]
机构：
[1] Goethe Univ Frankfurt, Frankfurt Inst Adv Studies, D-60438 Frankfurt, Germany
[2] Selcuk Univ, Dept Phys, TR-42079 Kampus, Konya, Turkey
[3] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia
[4] Johannes Gutenberg Univ Mainz, Inst Kernphys, D-55099 Mainz, Germany
[5] Russian Res Ctr, Kurchatov Inst, Moscow 123182, Russia
来源：
ASTROPHYSICAL JOURNAL | 2014年 / 789卷 / 01期
关键词：
dense matter; equation of state; nuclear reactions; nucleosynthesis; abundances; stars: neutron; supernovae: general; CORE-COLLAPSE SUPERNOVAE; GAS PHASE-TRANSITION; PLUS AU COLLISIONS; STATISTICAL MULTIFRAGMENTATION; DENSE MATTER; PHYSICAL-PROPERTIES; HEAVY-NUCLEI; HOT; MODEL; SIMULATIONS;
D O I：
10.1088/0004-637X/789/1/33
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This is an introduction to the tabulated database of stellar matter properties calculated within the framework of the Statistical Model for Supernova Matter (SMSM). The tables present thermodynamical characteristics and nuclear abundances for 31 values of baryon density (10(-8) < rho/rho(0) < 0.32, rho(0) = 0.15 fm(-3) is the normal nuclear matter density), 35 values of temperature (0.2MeV < T < 25 MeV), and 28 values of electron-to-baryon ratio (0.02 < Y-e < 0.56). The properties of stellar matter in beta equilibrium are also considered. The main ingredients of the SMSM are briefly outlined, and the data structure and content of the tables are explained.
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页数：12
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