Inner-most stable circular orbit in Kerr-MOG black hole
arXiv:1704.02740 · doi:10.1140/epjc/s10052-017-5152-7
Abstract
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.
arXiv comment5pages, 5figures
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- Scattering of quantum fields by a MOG Black Hole
- Shadow cast by a rotating black hole with anisotropic matter
- Relativistic Thermal Emission from Accretion Disks in Kerr-MOG Spacetimes