Equatorial circular motion in a Kerr-like spacetime

Fuente: arXiv
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Hauptverfasser: Solano-Alfaro, Diego, Frutos-Alfaro, Francisco
Format: Preprint
Veröffentlicht: 2024
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author Solano-Alfaro, Diego
Frutos-Alfaro, Francisco
author_facet Solano-Alfaro, Diego
Frutos-Alfaro, Francisco
contents An study of the equatorial circular motion of photons and massive particles around a rotating compact body like a neutron star is presented. For this goal, we use an approximate Kerr-like metric with mass quadrupole as perturbation. The effect of this deformation on the photon sphere, and the innermost stable circular orbit, is determined via an effective potential. Furthermore, a stability anaysis is shown, where we observed the same behavior of the effective potential for co-rotating and counter-rotating particles. A comparison with the results for the innermost stable circular orbit obtained for the Hartle-Thorne spacetime is also presented.
format Preprint
id arxiv_https___arxiv_org_abs_2404_19268
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Equatorial circular motion in a Kerr-like spacetime
Solano-Alfaro, Diego
Frutos-Alfaro, Francisco
General Relativity and Quantum Cosmology
An study of the equatorial circular motion of photons and massive particles around a rotating compact body like a neutron star is presented. For this goal, we use an approximate Kerr-like metric with mass quadrupole as perturbation. The effect of this deformation on the photon sphere, and the innermost stable circular orbit, is determined via an effective potential. Furthermore, a stability anaysis is shown, where we observed the same behavior of the effective potential for co-rotating and counter-rotating particles. A comparison with the results for the innermost stable circular orbit obtained for the Hartle-Thorne spacetime is also presented.
title Equatorial circular motion in a Kerr-like spacetime
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2404.19268