Relativistic gravitational collapse in non-comoving coordinates: The post-quasistatic approximation

Details Relativistic gravitational collapse in non-comoving coordinates: The post-quasistatic approximation Relativistic gravitational collapse in non-comoving coordinates: The post-quasistatic approximation

2002-02-14

arxiv.org/abs/gr-qc/0202051v1

Phys.Rev. D65 (2002) 104004

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

23 pages Latex, plus 12 ps. figures. To appear in Phys.Rev.D

Scientific paper

10.1103/PhysRevD.65.104004

A general, iterative, method for the description of evolving self-gravitating relativistic spheres is presented. Modeling is achieved by the introduction of an ansatz, whose rationale becomes intelligible and finds full justification within the context of a suitable definition of the post--quasistatic approximation. As examples of application of the method we discuss three models, in the adiabatic case.

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