Dense plasmas in astrophysics: from giant planets to neutron stars

被引：144

作者：

Chabrier, G. ^{[1
]}

Saumon, D.

Potekhin, A. Y.

机构：

[1] Ecole Normale Super Lyon, CNRS, CRAL, UMR 5574, F-69364 Lyon, France

[2] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

[3] AF Ioffe Phys Tech Inst, St Petersburg, Russia

来源：

JOURNAL OF PHYSICS A-MATHEMATICAL AND GENERAL | 2006年 / 39卷 / 17期

关键词：

D O I：

10.1088/0305-4470/39/17/S16

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We briefly examine the properties of the dense plasmas characteristic of the interior of giant planets and of the atmospheres of neutron stars. Special attention is devoted to the equation of state of hydrogen and helium at high density and to the effect of magnetic fields on the properties of dense matter.

引用

页码：4411 / 4419

页数：9

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