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We study tidal effects on self-gravitating Newtonian stars rotating around a Kerr black hole in stable circular orbits away from the equatorial plane.
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T. Bogdanović, M. Eracleous, S. Mahadevan, S. Sigurdsson, and P. Laguna, “Tidal disruption of a star by a black hole: Observational signature,” The Astrophysical Journal
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S. Ayal, M. Livio, and T. Piran, “Tidal disruption of a solar-type star by a supermassive black hole,” ApJ
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S. A. Hughes, “Evolution of circular, nonequatorial orbits of kerr black holes due to gravitational-wave emission,” Phys. Rev. D
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T. Karmakar and T. Sarkar, “Distinguishing between kerr and rotating jnw space-times via frame dragging and tidal effects,” General Relativity and Gravitation
2018
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