Charged Annular Disks and Reissner-Nordström Type Black Holes from Extremal Dust
arXiv:1009.1005 · doi:10.1103/PhysRevD.82.084005
Abstract
We present the first analytical superposition of a charged black hole with an annular disk of extremal dust. In order to obtain the solutions, we first solve the Einstein-Maxwell field equations for sources that represent disk-like configurations of matter in confomastatic spacetimes by assuming a functional dependence among the metric function, the electric potential and an auxiliary function,which is taken as a solution of the Laplace equation. We then employ the Lord Kelvin Inversion Method applied to models of finite extension in order to obtain annular disks. The structures obtained extend to infinity, but their total masses are finite and all the energy conditions are satisfied. Finally, we observe that the extremal Reissner-Nordström black hole can be embedded into the center of the disks by adding a boundary term in the inversion.
17 revtex pages, 8 eps figures
References in corpus (7)
- An Infinite Family of Generalized Kalnajs Disks
- Electrovacuum Static Counterrotating Relativistic Dust Disks
- Charged perfect fluid disks as sources of Taub-NUT-type spacetimes
- Finite axisymmetric charged dust disks in conformastatic spacetimes
- Counterrotating perfect fluid discs as sources of electrovacuum static spacetimes
- An Infinite Family of Self-consistent Models for Axisymmetric Flat Galaxies
- Relativistic static thin dust disks with an inner edge: An infinite family of new exact solutions