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Inner-most stable circular orbit in Kerr-MOG black hole

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arxiv 1704.02740 v2 pith:TCIAVZOK submitted 2017-04-10 gr-qc

Hyun-Chul Lee , Yong-Jin Han This is my paper · ORCID
classification gr-qc
keywords blackholegravitykerr-mogkerrcircularinner-mostmodified
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We study the inner-most stable circular orbit(ISCO) of Kerr black hole in MOdified gravity(Kerr-MOG black hole) which is one of the exact solution of the field equation of modified gravity in strong gravity regime. Kerr-MOG black hole is constructed commonly known kerr metric in Boyer-Lindquist coordinate by adding repulsive parameter like Yukawa force which explained in quantum gravity. We explore what is some differences of the ISCOs of Kerr-MOG black hole and kerr black hole.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Spherical photon orbits around Kerr-MOG black hole

    gr-qc 2024-12 conditional novelty 5.0 of 10

    Spherical photon orbits around Kerr-MOG black holes are classified, with a critical inclination angle switching the number of orbits from four to two.

  2. Chaotic motion of the charged test particle in a Kerr-MOG black hole with explicit symplectic algorithms

    gr-qc 2024-12 conditional novelty 4.0 of 10

    Chaos grows with energy, magnetic field, and the MOG parameter, and shrinks with spin and angular momentum, for a charged particle in a magnetized Kerr-MOG black hole.

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