The Energy of Bianchi Type I and II Universes in Teleparallel Gravity

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dc.creatorSo, Lau Loi
dc.creatorVargas, T.
dc.date2006-11-02
dc.date.accessioned2026-07-07T07:31:54Z
dc.date.available2026-07-07T07:31:54Z
dc.descriptionFor certain models, the energy of the universe which includes the energy of both the matter and the gravitational fields is obtained by using the quasilocal energy-momentum in teleparallel gravity. It is shown that in the case of the Bianchi type I and II universes, not only the total energy but also the quasilocal energy-momentum for any region vanishes independently of the three dimensionless coupling constants of teleparallel gravity.
dc.description9 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0611012
dc.identifierhttp://arxiv.org/abs/gr-qc/0611012
dc.identifierChin.J.Phys. 43 (2005) 901-908
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118918
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Energy of Bianchi Type I and II Universes in Teleparallel Gravity
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