Ellipsoidal Black Hole - Black Tori Systems in 4D Gravity

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dc.creatorVacaru, Sergiu I.
dc.date2001-11-19
dc.date.accessioned2026-07-07T06:28:58Z
dc.date.available2026-07-07T06:28:58Z
dc.descriptionWe construct new classes of exact solutions of the 4D vacuum Einstein equations which describe ellipsoidal black holes, black tori and combined black hole -- black tori configurations. The solutions can be static or with anisotropic polarizations and running constants. They are defined by off--diagonal metric ansatz which may be diagonalized with respect to anholonomic moving frames. We examine physical properties of such anholonomic gravitational configurations and discuss why the anholonomy may remove the restriction that horizons must be with spherical topology.
dc.description12 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/hep-th/0111166
dc.identifierhttp://arxiv.org/abs/hep-th/0111166
dc.identifierChapter 12 in: "Clifford and Riemann Finsler Structures in Geometric Mechanics and Gravity, Selected Works by S. Vacaru, P. Stavrinos, E. Gaburov and D. Gonta (Geometry Balkan Press, 2006) http://www.mathem.pub.ro/dgds/mono/va-t.pdf
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97879
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectMathematical Physics
dc.subjectDifferential Geometry
dc.subjectExactly Solvable and Integrable Systems
dc.titleEllipsoidal Black Hole - Black Tori Systems in 4D Gravity
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