ROTATING INCOHERENT MATTER IN GENERAL RELATIVITY

被引:3
作者
PACHNER, J [1 ]
机构
[1] UNIV SASKATCHEWAN,DEPT PHYS & ASTRON,REGINA,SASKATCHEWAN,CANADA
关键词
D O I
10.1139/p73-061
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
引用
收藏
页码:477 / 490
页数:14
相关论文
共 33 条
[1]   STABILITY OF EQUILIBRIUM OF SUPERMASSIVE AND SUPERDENSE STARS [J].
CALAMAI, G .
ASTROPHYSICS AND SPACE SCIENCE, 1970, 6 (02) :240-&
[3]   POST-NEWTONIAN EQUATIONS OF HYDRODYNAMICS IN GENERAL RELATIVITY [J].
CHANDRASEKHAR, S .
ASTROPHYSICAL JOURNAL, 1965, 142 (04) :1488-+
[4]  
Chandrasekhar S., 1965, Astrophys. J., V142, P1519
[5]   NEUTRON STAR MODELS BASED ON AN IMPROVED EQUATION OF STATE [J].
COHEN, JM ;
LANGER, WD ;
ROSEN, LC ;
CAMERON, AGW .
ASTROPHYSICS AND SPACE SCIENCE, 1970, 6 (02) :228-&
[6]  
COURANT R, 1962, METHODS MATHEMATICAL, V2
[7]   Values of T and the christoffel symbols for a line element of considerable generality [J].
Dingle, H .
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1933, 19 :559-563
[9]  
Harrison B.K., 1965, Gravitational Theory and Gravitational Collapse
[10]   SLOWLY ROTATING RELATIVISTIC STARS .2. MODELS FOR NEUTRON STARS AND SUPERMASSIVE STARS [J].
HARTLE, JB ;
THORNE, KS .
ASTROPHYSICAL JOURNAL, 1968, 153 (3P1) :807-&