The vacuum energy density in the teleparallel equivalent of general relativity

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dc.creatorMaluf, J. W.
dc.creatorda Rocha-Neto, J. F.
dc.date2003-08-26
dc.date.accessioned2026-07-07T03:28:03Z
dc.date.available2026-07-07T03:28:03Z
dc.descriptionConsidering the vacuum as characterized by the presence of only the gravitational field, we show that the vacuum energy density of the de Sitter space, in the realm of the teleparallel equivalent of general relativity, can acquire arbitrarily high values. This feature is expected to hold in the consideration of realistic cosmological models, and may possibly provide a simple explanation to the cosmological constant problem.
dc.description11 pages, latex file, no figures, contribution to the tenth Marcel Grossmann Meeting (MG10), 20-26 July 2003, Rio de Janeiro, Brazil
dc.identifierhttps://arxiv.org/abs/gr-qc/0308084
dc.identifierhttp://arxiv.org/abs/gr-qc/0308084
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34678
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe vacuum energy density in the teleparallel equivalent of general relativity
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