Quintessence inhomogeneous cosmology
General Relativity and Quantum Cosmology
2007-05-23 v1
Abstract
The Einstein-Klein-Gordon field equations are solved in a inhomogeneous shear-free universe containing a material fluid, a self-interacting scalar field, a variable cosmological term, and a heat flux. A quintessence-dominated scenario arises with a power-law accelerated expansion compatible with the currently observed homogeneous universe.
Keywords
Cite
@article{arxiv.gr-qc/9911030,
title = {Quintessence inhomogeneous cosmology},
author = {Luis P. Chimento and Alejandro S. Jakubi and Diego Pavon},
journal= {arXiv preprint arXiv:gr-qc/9911030},
year = {2007}
}
Comments
8 pages, LaTeX 2.09. To appear in Proceedings of ERE-99