On the active gravitational mass of a non-spherical source leaving hydrostatic equilibrium

被引:19
|
作者
Herrera, L [1 ]
Di Prisco, A [1 ]
Fuenmayor, E [1 ]
机构
[1] Cent Univ Venezuela, Fac Ciencias, Escuela Fis, Caracas, Venezuela
关键词
D O I
10.1088/0264-9381/20/6/307
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We obtain an expression for the active gravitational mass (Tolman) of a source of the gamma metric, just after its departure from hydrostatic equilibrium, on a time scale of the order of (or smaller than) the hydrostatic time scale. It is shown that for very compact sources, even arbitrarily small departures from sphericity produce a significant decrease (increase) in the value of an active gravitational mass of collapsing (expanding) spheres, with respect to its value in equilibrium, enhancing thereby the stability of the system.
引用
收藏
页码:1125 / 1136
页数:12
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