Counterrotating perfect fluid discs as sources of electrovacuum static spacetimes
arXiv:0810.2567 · doi:10.1088/0264-9381/21/21/007
Abstract
The interpretation of some electrovacuum spacetimes in terms of counterrotating perfect fluid discs is presented. The interpretation is mades by means of an "inverse problem" approach used to obtain disc sources of known static solutions of the Einstein-Maxwell equations. In order to do such interpretation, a detailed study is presented of the counterrotating model (CRM) for generic electrovacuum static axially symmetric relativistic thin discs with nonzero radial pressure. Four simple families of models of counterrotating charged discs based on Chazy-Curzon-type, Zipoy-Voorhees-type, Bonnor-Sackfield-type, and charged and magnetized Darmois electrovacuum metrics are considered where we obtain some discs with a CRM well behaved.
22 pages, 4 figures, LaTeX2e
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Cited by in corpus (11)
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- Finite axisymmetric charged dust disks in conformastatic spacetimes
- Counterrotating perfect fluid discs as sources of electrovacuum static spacetimes
- Charged Annular Disks and Reissner-Nordström Type Black Holes from Extremal Dust
- General magnetized Weyl solutions: Disks and motion of charged particles
- Perturbation of a Schwarzschild black hole due to a rotating thin disc
- An infinite family of magnetized Morgan-Morgan relativistic thin disks
- Exact relativistic models of perfect fluid disks in a magnetic field
- Rotating relativistic thin disks as sources of charged and magnetized Kerr-NUT spacetimes
- Relativistic Static Thin Disks of Polarized Matter
- Exact relativistic models of conformastatic charged dust thick disks