Magnetized Kerr-Newman-Taub-NUT spacetimes
arXiv:2103.04865 · doi:10.1140/epjc/s10052-021-09430-z
Abstract
We find a new class of exact solutions in the Einstein-Maxwell theory by employing the Ernst magnetization process to the Kerr-Newman-Taub-NUT spacetimes. We study the solutions and find that they are regular everywhere. We also find the quasilocal conserved quantities for the spacetimes, the corresponding Smarr formula and the first law of thermodynamics.
arXiv comment38 pages, 17 figures, typos corrected, one appendix added
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Cited by in corpus (10)
- Classifying topology of consistent thermodynamics of the four-dimensional neutral Lorentzian NUT-charged spacetimes
- Ehlers transformations as a tool for constructing accelerating NUT black holes
- Black Hole Chemistry: the first 15 years
- Magnetized Reissner-Nordstrom-Taub-NUT spacetime and microscopic entropy
- Kerr-Newman black hole in a Melvin-swirling universe
- Spontaneous pair production near magnetized Reissner-Nordstrom black holes
- Bianchi IX geometry and the Einstein-Maxwell theory
- Meissner effect and holographic dual for the Melvin-Kerr-Newman-Taub-NUT spacetimes
- Uniqueness of dark matter magnetized static black hole spacetime
- Phase diagrams of quasinormal frequencies for Schwarzschild, Kerr, and Taub-NUT black holes