Radiating fluid spheres in the effective variables approximation
General Relativity and Quantum Cosmology
2009-11-07 v1
Abstract
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.
Keywords
Cite
@article{arxiv.gr-qc/0211033,
title = {Radiating fluid spheres in the effective variables approximation},
author = {W. Barreto and B. Rodríguez and H. Martínez},
journal= {arXiv preprint arXiv:gr-qc/0211033},
year = {2009}
}
Comments
15 pages, 6 eps figures, to appear in Ap. Sp. Sc