Some properties of static general relativistic stellar models

1980 ◽  
Vol 21 (6) ◽  
pp. 1455-1459 ◽  
Author(s):  
Lee Lindblom
1991 ◽  
Vol 44 (2) ◽  
pp. 307-313 ◽  
Author(s):  
Richard H. Price ◽  
James R. Ipser

1991 ◽  
Vol 376 ◽  
pp. 662
Author(s):  
J. M. Aguirregabiria ◽  
J. Ibanez ◽  
A. di Prisco ◽  
L. Herrera

The equilibrium states of isolated self-gravitating fluids (i.e. stellar models) always have a high degree of spatial symmetry. This paper reviews the current understanding of these symmetries in both the newtonian and the general relativistic theories. The arguments that establish (under various appropriate conditions) the necessity of spherical symmetry, axisymmetry, and reflection symmetry are summarized. The limitations of the present results and suggestions for further progress are outlined in the concluding remarks.


1985 ◽  
Vol 292 ◽  
pp. 12 ◽  
Author(s):  
S. Detweiler ◽  
L. Lindblom

Sign in / Sign up

Export Citation Format

Share Document