Extended bodies with spin induced quadrupoles on circular equatorial orbits in Kerr spacetime

Iason Timogiannis, Georgios Lukes-Gerakopoulos, and Theocharis A. Apostolatos
Phys. Rev. D 108, 084023 – Published 11 October 2023

Abstract

This work discusses the motion of extended test bodies as described by the Mathisson-Papapetrou-Dixon (MPD) equations in the pole-dipole-quadrupole approximation. We focus on the case that the quadrupole is solely induced by the spin of the body which is assumed to move on a circular equatorial orbit in a Kerr background. To fix the center of mass of the MPD body we use two different spin supplementary conditions (SSCs): the Tulczyjew-Dixon SSC and the Mathisson-Pirani SSC. We provide the frequencies of the circular equatorial orbits for the pole-dipole-(spin induced) quadrupole approximation of the body for both SSCs. In the process we develop an explicit four-velocity four-momentum relation for a pole-dipole-quadrupole body under the Mathisson-Pirani SSC.

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  • Received 21 June 2023
  • Accepted 11 September 2023

DOI:https://doi.org/10.1103/PhysRevD.108.084023

© 2023 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Iason Timogiannis1,*, Georgios Lukes-Gerakopoulos2,†, and Theocharis A. Apostolatos1,‡

  • 1Section of Astrophysics, Astronomy, and Mechanics, Department of Physics, University of Athens, Panepistimiopolis Zografos GR15783, Athens, Greece
  • 2Astronomical Institute of the Czech Academy of Sciences, Boční II 1401/1a, CZ-141 00 Prague, Czech Republic

  • *timogian@phys.uoa.gr
  • gglukes@gmail.com
  • thapostol@phys.uoa.gr

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Issue

Vol. 108, Iss. 8 — 15 October 2023

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