Equation of state of protoneutron star matter

被引：10

作者：

Bordbar, GH ^{[1
]}

机构：

[1] Shiraz Univ, Dept Phys, Shiraz 71454, Iran

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2002年 / 41卷 / 02期

关键词：

D O I：

10.1023/A:1014063007618

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We have calculated the equation of state of protoneutron star matter by using the lowest order constrained variational method. In our calculations, the modern Argonne potential (AV(18)) together with its older model potential (AV(14)) are used. It is found that the equation of state for high lepton fraction is stiffer than for low lepton fraction. It is seen that the increasing effect of pressure due to high lepton fraction and due to entropy are comparable. It is shown that the temperature and adiabatic index depend on the values of both entropy and lepton fraction.

引用

页码：309 / 319

页数：11

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