Gravitational waveforms for spinning compact binaries

dc.creatorMajár, János
dc.creatorVasúth, Mátyás
dc.date2008-06-13
dc.date.accessioned2026-07-07T11:33:55Z
dc.date.available2026-07-07T11:33:55Z
dc.descriptionThe rotation of the bodies and the eccentricity of the orbit have significant effects on the emitted gravitational radiation of binary systems. This work focuses on the evaluation of the gravitational wave polarization states for spinning compact binaries. We consider binaries on eccentric orbits and the spin-orbit interaction up to the 1.5 post-Newtonian order in a way which is independent of the parameterization of the orbit. The equations of motion for angular variables are included. The formal expressions of the polarization states are given with the inclusion of higher order corrections to the waveform.
dc.identifierhttps://arxiv.org/abs/0806.2273
dc.identifierhttp://arxiv.org/abs/0806.2273
dc.identifierPhys.Rev.D77:104005,2008
dc.identifierdoi:10.1103/PhysRevD.77.104005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198067
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational waveforms for spinning compact binaries
dc.typetext

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