Non spherical sources of strong gravitational fields out of hydrostatic equilibrium

Details Non spherical sources of strong gravitational fields out of hydrostatic equilibrium Non spherical sources of strong gravitational fields out of hydrostatic equilibrium

2000-10-19

arxiv.org/abs/gr-qc/0010066v1

Astrophys.Space Sci. 277 (2001) 447

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

26 pages Latex, a shortened version to appear in Astr.Space.Sci

Scientific paper

10.1023/A:1012592222758

We describe the departure from equilibrium of matter distributions representing sources for a class of Weyl metric. It is shown that, for extremely high gravitational fields, slight deviations from spherical symmetry may enhance the stability of the system weakening thereby its tendency to a catastrophic collapse. For critical values of surface gravitational potential, in contrast with the exactly spherically symmetric case, the speed of entering the collapse regime decreases substantially, at least for specific cases.

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