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arXiv · gr-qc/9911030

Quintessence inhomogeneous cosmology

Luis P. Chimento·Alejandro S. Jakubi·Diego Pavon
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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.

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Luis P. Chimento, Alejandro S. Jakubi, Diego Pavon. 1999-11-09. Quintessence inhomogeneous cosmology. https://arxiv.org/abs/gr-qc/9911030

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