Carter's constant revealed

dc.creatorRosquist, Kjell
dc.creatorBylund, Tomas
dc.creatorSamuelsson, Lars
dc.date2007-10-23
dc.date2009-03-19
dc.date.accessioned2026-07-07T13:13:15Z
dc.date.available2026-07-07T13:13:15Z
dc.descriptionA new formulation of Carter's constant for geodesic motion in Kerr black holes is given. It is shown that Carter's constant corresponds to the total angular momentum plus a precisely defined part which is quadratic in the linear momenta. The characterization is exact in the weak field limit obtained by letting the gravitational constant go to zero. It is suggested that the new form can be useful in current studies of the dynamics of extreme mass ratio inspiral (EMRI) systems emitting gravitational radiation.
dc.descriptionMinor changes to match published version
dc.identifierhttps://arxiv.org/abs/0710.4260
dc.identifierhttp://arxiv.org/abs/0710.4260
dc.identifierInt.J.Mod.Phys.D18:429-434,2009
dc.identifierdoi:10.1142/S0218271809014546
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229827
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleCarter's constant revealed
dc.typetext

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