Dark energy, dark matter and the Chaplygin gas

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dc.creatorColistete Jr., R.
dc.creatorFabris, J. C.
dc.creatorGoncalves, S. V. B.
dc.creatorde Souza, P. E.
dc.date2002-10-23
dc.date.accessioned2026-07-07T03:27:16Z
dc.date.available2026-07-07T03:27:16Z
dc.descriptionThe possibility that the dark energy may be described by the Chaplygin gas is discussed. Some observational constraints are established. These observational constraints indicate that a unified model for dark energy and dark matter through the employement of the Chaplygin gas is favored.
dc.description5 pages, 2 EPS figures, LaTeX 2e, uses graphicx. To appear in the Proceedings of the XVIII IAP Colloquium `On the nature of dark energy', IAP, Paris, 1-5 July 2002
dc.identifierhttps://arxiv.org/abs/gr-qc/0210079
dc.identifierhttp://arxiv.org/abs/gr-qc/0210079
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34368
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDark energy, dark matter and the Chaplygin gas
dc.typetext

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