AN EQUATION OF STATE AT SUBNUCLEAR DENSITIES

被引：51

作者：

LANGER, WD

ROSEN, LC

COHEN, JM

CAMERON, AGW

机构：

[1] Goddard Institute for Space Studies, NASA, New York, N. Y.

[2] Belfer Graduate School of Science, Yeshiva University, New York, N. Y.

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1969年 / 5卷 / 03期

关键词：

D O I：

10.1007/BF00649994

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

An equation of state for cold matter above white dwarf densities is evaluated. The gas is considered to be a mixture of degenerate neutrons, protons and electrons combined with nuclei of one type (that is only one A and Z value). We derive the equilibrium equations for the mixture and calculate the number densities as well as the A and Z of the nucleus. Finally we calculate an equation of state, which smoothly goes over to that of a neutron, proton electron gas mixture at a density of ∼5×1013 g/cm3. © 1969 D. Reidel Publishing Company.

引用

页码：259 / &

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