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The evolution of a warped disc around a Kerr black hole
Monthly Notices of the Royal Astronomical Society, no. 2 (2002): 706-712
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摘要
We consider the evolution of a warped disc around a Kerr black hole, under conditions such that the warp propagates in a wave-like manner. This occurs when the dimensionless effective viscosity, α, that damps the warp is less than the characteristic angular semi-thickness, H/R, of the disc. We adopt linearized equations that are valid for...更多
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