Periodic analogues of the Kerr solutions: a numerical study

Abstract

AbstractIn recent years black hole configurations with non standard topology or with non-standard asymptotic behavior have gained considerable attention. In this article we carry out numerical investigations aimed to find periodic coaxial configurations of co-rotating3+1vacuum black holes, for which existence and uniqueness has not yet been theoretically proven. The aimed configurations would extend Myers/Korotkin-Nicolai’s family of non-rotating (static) coaxial arrays of black holes. We find that numerical solutions with a given value for the areaAand for the angular momentumJof the horizons appear to exist only when the separation between consecutive horizons is larger than a certain critical value that depends only onAand|J|. We also establish that the solutions have the same Lewis’s cylindrical asymptotic behavior as van Stockum’s infinite rotating cylinders. Below the mentioned critical value the rotational energy appears to be too big to sustain a global equilibrium and a singularity shows up at a finite distance from the bulk. This phenomenon is a relative of van Stockum’s asymptotic collapse, manifest when the angular momentum (per unit of axial length) reaches a critical value compared to the mass (per unit of axial length), and that results from a transition in the Lewis’s class of the cylindrical exterior solution. This remarkable phenomenon seems to be unexplored in the context of coaxial arrays of black holes. Ergospheres and other global properties are also presented in detail.