Teleparallel Energy-Momentum Distribution of Lewis-Papapetrou Spacetimes

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dc.creatorSharif, M.
dc.creatorAmir, M Jamil
dc.date2006-07-20
dc.date.accessioned2026-07-07T12:40:44Z
dc.date.available2026-07-07T12:40:44Z
dc.descriptionIn this paper, we find the energy-momentum distribution of stationary axisymmetric spacetimes in the context of teleparallel theory by using M$\ddot{o}$ller prescription. The metric under consideration is the generalization of the Weyl metrics called the Lewis-Papapetrou metric. The class of stationary axisymmetric solutions of the Einstein field equations has been studied by Galtsov to include the gravitational effect of an {\it external} source. Such spacetimes are also astrophysically important as they describe the exterior of a body in equilibrium. The energy density turns out to be non-vanishing and well-defined and the momentum becomes constant except along $θ$-direction. It is interesting to mention that the results reduce to the already available results for the Weyl metrics when we take $ω=0$.
dc.description13 pages, accepted for publication in Modern Physics Letters A
dc.identifierhttps://arxiv.org/abs/gr-qc/0607077
dc.identifierhttp://arxiv.org/abs/gr-qc/0607077
dc.identifierMod.Phys.Lett.A22:425-434,2007; Addendum-ibid.A23:3431-3433,2009
dc.identifierdoi:10.1142/S0217732307021214 10.1142/S0217732308028156
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/219535
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTeleparallel Energy-Momentum Distribution of Lewis-Papapetrou Spacetimes
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