Determination of the finite temperature equation of state of dense matter

被引：0
|
作者：
A. Yu. Illarionov
S. Fantoni
F. Pederiva
S. Gandolfi
K. E. Schmidt
机构：
[1] Dipartimento di Fisica dell’Universitá di Trento,International School for Advanced Studies
[2] SISSA Trieste,INFN
[3] Sezione di Trieste,INFN
[4] Gruppo Collegato di Trento,Theoretical Division
[5] Los Alamos National Laboratory,Department of Physics
[6] Arizona State University,undefined
来源：
Physics of Atomic Nuclei | 2012年 / 75卷
关键词：
Neutron Star; Atomic Nucleus; Nuclear Matter; Symmetry Energy; Saturation Density;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The equation of state is calculated for temperatures less than 30 MeV and densities less than four times the saturation density of nuclear matter using a combined analysis of Auxiliarly Fields Diffusion Monte Carlo and Fermi Hypernetted Change methods.
引用
收藏
页码：866 / 869
页数：3
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