Quintessence inhomogeneous cosmology

Details Quintessence inhomogeneous cosmology Quintessence inhomogeneous cosmology

1999-11-09

arxiv.org/abs/gr-qc/9911030v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, LaTeX 2.09. To appear in Proceedings of ERE-99

Scientific paper

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.

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