Role of the interparticle interactions and axial rotation in the massive white dwarfs theory

被引：0

作者：

Dzikovskyi, D. V. ^{[1
]}

Vavrukh, M. V. ^{[1
]}

Smerechynskyi, S. V. ^{[1
]}

机构：

[1] Ivan Franko Natl Univ Lviv, Dept Astrophys, 8 Kyryla & Mephodiya Str, Lvov, Ukraine

来源：

ADVANCES IN ASTRONOMY AND SPACE PHYSICS | 2018年 / 8卷 / 01期

关键词：

stars: white dwarfs; rotation; equation of state;

D O I：

10.17721/2227-1481.8.9-15

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using the equation of state of electron-nuclear model at high densities and the mechanical equilibrium equation we have investigated the influence of interparticle interactions and axial rotation on the macroscopic characteristics of massive white dwarfs. The method of solving the equilibrium equation in the case of rotation, using the basis of universal functions of the radial variable has been proposed. The conditions in which the axial rotation can compensate for weight loss of mass due to the interparticle Coulomb interactions have been established.

引用

页码：9 / 15

页数：7

共 21 条

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