Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8133
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dc.contributor.authorPrerna Rana-
dc.contributor.authorMangalam, A-
dc.date.accessioned2023-02-02T08:54:06Z-
dc.date.available2023-02-02T08:54:06Z-
dc.date.issued2022-
dc.identifier.citationThe Fifteenth Marcel Grossmann Meeting on General Relativity, edited by Elia S. Battistelli, Robert T. Jantzen and Remo Ruffini, pp. 858-864en_US
dc.identifier.isbn9789811258251-
dc.identifier.urihttp://hdl.handle.net/2248/8133-
dc.descriptionOpen Accessen_US
dc.descriptionThis is an Open Access volume published by World Scientific Publishing Company. It is distributed under the terms of the Creative Commons Attribution-Non Commercial 4.0 (CC BY-NC) License. Further distribution of this work is permitted, provided the original work is properly cited.-
dc.description.abstractWe derive the conditions for a non-equatorial eccentric bound orbit to exist around a Kerrblack hole in two-parameter spaces: the energy, angular momentum of the test particle,spin of the black hole, and Carter’s constant space (E,L,a,Q), and eccentricity, inverse-latus rectum space (e,μ,a,Q). These conditions distribute various kinds of bound orbitsin different regions of the (E,L)and(e,μ) planes, depending on which pair of rootsof the effective potential forms a bound orbit. We provide a prescription to select theseparameters for bound orbits, which are useful inputs to study bound trajectory evolutionin various astrophysical applications like simulations of gravitational wave emission fromextreme-mass ratio inspirals, relativistic precession around black holes, and the study ofgyroscope precession as a test of general relativityen_US
dc.language.isoenen_US
dc.publisherWorld Scientific Publishingen_US
dc.relation.urihttps://doi.org/10.1142/9789811258251_0116-
dc.rights© World Scientific Publishing-
dc.subjectClassical black holesen_US
dc.subjectRelativity and Gravitationen_US
dc.subjectBound orbit trajectoriesen_US
dc.titleBound orbit domains in the phase space of the Kerr geometryen_US
dc.typeArticleen_US
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