Locally Anisotropic Black Holes in Einstein Gravity

Details Locally Anisotropic Black Holes in Einstein Gravity Locally Anisotropic Black Holes in Einstein Gravity

2000-01-08

arxiv.org/abs/gr-qc/0001020v3

Chapter 4 in: "Clifford and Riemann Finsler Structures in Geometric Mechanics and Gravity, Selected Works by S. Vacaru, P. Sta

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

latex209, version 4, misprints corrected

Scientific paper

By applying the method of moving frames modelling one and two dimensional local anisotropies we construct new solutions of Einstein equations on pseudo-Riemannian spacetimes. The first class of solutions describes non-trivial deformations of static spherically symmetric black holes to locally anisotropic ones which have elliptic (in three dimensions) and ellipsoidal, toroidal and elliptic and another forms of cylinder symmetries (in four dimensions). The second class consists from black holes with oscillating elliptic horizons.

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