Expansion-Free Evolving Spheres Must Have Inhomogeneous Energy Density Distributions
General Relativity and Quantum Cosmology
2015-05-13 v2 Cosmology and Nongalactic Astrophysics
Abstract
In a recent paper a systematic study on shearing expansion-free spherically symmetric distributions was presented. As a particular case of such systems, the Skripkin model was mentioned, which corresponds to a nondissipative perfect fluid with a constant energy density. Here we show that such a model is inconsistent with junction conditions. It is shown that in general for any nondissipative fluid distribution, the expansion-free condition requires the energy density to be inhomogeneous. As an example we consider the case of dust, which allows for a complete integration.
Keywords
Cite
@article{arxiv.0903.4774,
title = {Expansion-Free Evolving Spheres Must Have Inhomogeneous Energy Density Distributions},
author = {L. Herrera and G. Le Denmat and N. O. Santos},
journal= {arXiv preprint arXiv:0903.4774},
year = {2015}
}
Comments
8 pages, Latex. To appear in Phys. Rev.D. Typos corrected