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- W2138718662 abstract "Based on a framework of the hydrodynamics for a fluid star of mass m orbiting a Kerr black hole of mass M ≫m, relativistic Roche-Riemann ellipsoids for incompressible fluids are considered. It is found that in the relativistic Roche-Riemann limit for the irrotational Roche-Riemann ellipsoid moving at the innermost stable circular orbit around Kerr black holes, the angular velocity, Ω, becomes Ω* ≃0.063637πρ. We also argue implications of present results on the final fate of black hole-neutron star binary systems." @default.
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- W2138718662 date "1996-11-01" @default.
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- W2138718662 title "Relativistic Roche-Riemann Problems around a Black Hole" @default.
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- W2138718662 doi "https://doi.org/10.1143/ptp.96.917" @default.
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