Gravitational waveforms from a Lense-Thirring system

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dc.creatorMajár, János
dc.creatorVasúth, Mátyás
dc.date2006-11-20
dc.date.accessioned2026-07-07T10:22:02Z
dc.date.available2026-07-07T10:22:02Z
dc.descriptionThe construction of ready to use templates for gravitational waves from spinning binaries is an important challenge in the investigation of detectable gravitational wave signals. Here we present a method to evaluate the gravitational wave polarization states for inspiralling compact binaries in the extreme mass ratio limit. We discuss the effects caused by the rotation of the central massive object for eccentric orbits in the Lense-Thirring approximation and give the formal expressions of the polarization states including higher order corrections. Our results are in agreement with existing calculations for the spinless and circular orbit limits.
dc.description11 pages, accepted for publication in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/gr-qc/0611105
dc.identifierhttp://arxiv.org/abs/gr-qc/0611105
dc.identifierPhys.Rev.D74:124007,2006
dc.identifierdoi:10.1103/PhysRevD.74.124007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175376
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational waveforms from a Lense-Thirring system
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