Hydrodynamics and global structure of rotating Schwarzschild black holes

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dc.creatorHong, Soon-Tae
dc.creatorKim, Sung-Won
dc.date2005-03-18
dc.date.accessioned2026-07-07T07:48:41Z
dc.date.available2026-07-07T07:48:41Z
dc.descriptionExploiting a rotating Schwarzschild black hole metric, we study hydrodynamic properties of perfect fluid whirling inward toward the black holes along a conical surface. On the equatorial plane of the rotating Schwarzschild black hole, we derive radial equations of motion with effective potentials and the Euler equation for steady state axisymmetric fuid. Moreover, numerical analysis is performed to figure out effective potentials of particles on the rotating Schwarzschild manifolds in terms of angular velocity, total energy and angular momentum per unit rest mass. Higher dimensional global embeddings are also constructed inside and outside the event horizons of the rotating Schwarzschild black holes.
dc.description6 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0503079
dc.identifierhttp://arxiv.org/abs/gr-qc/0503079
dc.identifierJ.Korean Phys.Soc. 49 (2006) S748-S754
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/124584
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHydrodynamics and global structure of rotating Schwarzschild black holes
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