Full causal dissipative cosmologies with stiff matter
General Relativity and Quantum Cosmology
2008-11-26 v1
Abstract
The general solution of the gravitational field equations for a full causal bulk viscous stiff cosmological fluid, with bulk viscosity coefficient proportional to the energy density to the power 1/4, is obtained in the flat Friedmann-Robertson-Walker geometry. The solution describes a non-inflationary Universe, which starts its evolution from a singular state. The time variation of the scale factor, deceleration parameter, viscous pressure, viscous pressure-thermodynamic pressure ratio, comoving entropy and Ricci and Kretschmann invariants is considered in detail.
Keywords
Cite
@article{arxiv.gr-qc/0311050,
title = {Full causal dissipative cosmologies with stiff matter},
author = {M. K. Mak and T. Harko},
journal= {arXiv preprint arXiv:gr-qc/0311050},
year = {2008}
}
Comments
6 pages, 6 figures, to appear in Int. J. Mod. Phys. D