Energy of gravitational radiation in plane-symmetric space-times

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dc.creatorHayward, Sean A.
dc.date2008-05-19
dc.date.accessioned2026-07-07T11:50:54Z
dc.date.available2026-07-07T11:50:54Z
dc.descriptionGravitational radiation in plane-symmetric space-times can be encoded in a complex potential, satisfying a non-linear wave equation. An effective energy tensor for the radiation is given, taking a scalar-field form in terms of the potential, entering the field equations in the same way as the matter energy tensor. It reduces to the Isaacson energy tensor in the linearized, high-frequency approximation. An energy conservation equation is derived for a quasi-local energy, essentially the Hawking energy. A transverse pressure exerted by interacting low-frequency gravitational radiation is predicted.
dc.description7 REVTeX4 pages
dc.identifierhttps://arxiv.org/abs/0805.2813
dc.identifierhttp://arxiv.org/abs/0805.2813
dc.identifierPhys.Rev.D78:044027,2008
dc.identifierdoi:10.1103/PhysRevD.78.044027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203719
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEnergy of gravitational radiation in plane-symmetric space-times
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