What role pressures play to determine the final end-state of gravitational collapse?

Details What role pressures play to determine the final end-state of gravitational collapse? What role pressures play to determine the final end-state of gravitational collapse?

2002-06-28

arxiv.org/abs/gr-qc/0206086v2

Class.Quant.Grav. 19 (2002) 5229-5234

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages Revtex4. Accepted by "Classical and Quantum Garavity"

Scientific paper

10.1088/0264-9381/19/20/314

We examine here in what way the pressures affect the final fate of a
continual gravitational collapse. It is shown that the presence of a
non-vanishing pressure gradient in the collapsing cloud determines directly the
epoch of formation of trapped surfaces and the apparent horizon, thus changing
the causal structure in the vicinity of singularity.

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