Radiating fluid spheres in the effective variables approximation

Details Radiating fluid spheres in the effective variables approximation Radiating fluid spheres in the effective variables approximation

2002-11-10

arxiv.org/abs/gr-qc/0211033v1

Astrophys.Space Sci. 282 (2002) 581-593

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

15 pages, 6 eps figures, to appear in Ap. Sp. Sc

Scientific paper

10.1023/A:1020982504341

We study the evolution of spherically symmetric radiating fluid distributions using the effective variables method, implemented {\it ab initio} in Schwarzschild coordinates. To illustrate the procedure and to establish some comparison with the original method, we integrate numerically the set of equations at the surface for two different models. The first model is derived from the Schwarzschild interior solution. The second model is inspired in the Tolman VI solution.

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