Gravitational Waves from an Axi-symmetric Source in the Nonsymmetric Grav. Theory

dc.creatorMoffat, J. W.
dc.creatorTatarski, D. C.
dc.date1992-07-27
dc.date.accessioned2026-07-07T03:29:56Z
dc.date.available2026-07-07T03:29:56Z
dc.descriptionWe examine gravitational waves in an isolated axi--symmetric reflexion symmetric NGT system. The structure of the vacuum field equations is analyzed and the exact solutions for the field variables in the metric tensor are found in the form of expansions in powers of a radial coordinate. We find that in the NGT axially symmetric case the mass of the system remains constant only if the system is static (as it necessarily is in the case of spherical symmetry). If the system radiates, then the mass decreases monotonically and the energy flux associated with waves is positive.
dc.description26 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9207009
dc.identifierhttp://arxiv.org/abs/gr-qc/9207009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35381
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational Waves from an Axi-symmetric Source in the Nonsymmetric Grav. Theory
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