Gravitational radiation of accelerated sources

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dc.creatorMaluf, J. W.
dc.creatorde Andrade, V. C.
dc.creatorSteiner, J. R.
dc.date2006-10-20
dc.date.accessioned2026-07-07T11:04:32Z
dc.date.available2026-07-07T11:04:32Z
dc.descriptionWe investigate the gravitational radiation produced by a linearly accelerated source in general relativity. The investigation is performed by studying the vacuum C metric, which is interpreted as representing the exterior space-time of an uniformly accelerating spherically symmetric gravitational source, and is carried out in the context of the teleparallel equivalent of general relativity. For an observer sufficiently far from both the (modified) Schwarzschild and Rindler horizons, which is a realistic situation, we obtain a simple expression for the total emitted gravitational radiation. We also briefly discuss on the absolute or relative character of the accelerated motion.
dc.description21 pages, no figures, accepted for publication in the IJMPD
dc.identifierhttps://arxiv.org/abs/gr-qc/0610102
dc.identifierhttp://arxiv.org/abs/gr-qc/0610102
dc.identifierInt.J.Mod.Phys.D16:857-874,2007
dc.identifierdoi:10.1142/S0218271807010456
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188924
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational radiation of accelerated sources
dc.typetext

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