Black Tori Solutions in Einstein and 5D Gravity

The ’anholonomic frame’ method [1–3] is applied for constructing new classes of exact solutions of vacuum Einstein equations with off–diagonal metrics in 4D and 5D gravity. We examine several black tori solutions generated by anholonomic transforms with non–trivial topology of the Schwarzshild metric, which have a static toroidal horizon. We define ansatz and parametrizations which contain warping factors, running constants (in time and extra dimension coordinates) and effective nonlinear gravitational polarizations. Such anisotropic vacuum toroidal metrics, the first example was given in [1], differ substantially from the well known toroidal black holes [4] which were constructed as non–vacuum solutions of the Einstein–Maxwell gravity with cosmological constant. Finally, we analyze two anisotropic 5D and 4D black tori solutions with cosmological constant. Pacs 04.50.+h, 11.25.M, 11.10.Kk, 12.10.-g