Quintessence inhomogeneous cosmology

Simple item page
dc.creatorChimento, Luis P.
dc.creatorJakubi, Alejandro S.
dc.creatorPavon, Diego
dc.date1999-11-09
dc.date.accessioned2026-07-07T03:33:41Z
dc.date.available2026-07-07T03:33:41Z
dc.descriptionThe 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.
dc.description8 pages, LaTeX 2.09. To appear in Proceedings of ERE-99
dc.identifierhttps://arxiv.org/abs/gr-qc/9911030
dc.identifierhttp://arxiv.org/abs/gr-qc/9911030
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36671
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuintessence inhomogeneous cosmology
dc.typetext

Files

Collections

arXiv