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• W2036090830 abstract "The tidal interaction of n = 1.5 polytropic stars with a massive rotating black hole is studied numerically. The general relativistic tidal potential for the Kerr metric is used to evaluate tidal forces exerted on a star. The hydrodynamic response of a star to these forces is treated in the Newtonian approximation using a three-dimensional, Eulerian, PPM hydrodynamical code. We compute the energy, ΔE, and angular momentum, ΔL, transferred into a star and the mass, ΔM, lost by the star during the interaction." @default.
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• W2036090830 date "1997-04-10" @default.
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• W2036090830 title "Relativistic Tidal Interaction of Stars with a Rotating Black Hole" @default.
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• W2036090830 doi "https://doi.org/10.1086/303875" @default.
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