Magnetized Kerr-Newman-Taub-NUT spacetimes

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.

38 pages, 17 figures, typos corrected, one appendix added

References in corpus (8)

• Particle Acceleration on the Background of the Kerr-Taub-NUT Spacetime
• Superradiant instability for black holes immersed in a magnetic field
• Superradiant instability of black holes immersed in a magnetic field
• Kerr-Taub-NUT Spacetime with Maxwell and Dilaton Fields
• The Disjointed Thermodynamics of Rotating Black Holes With a NUT Twist
• Deformed conformal symmetry of Kerr-Newman-NUT-AdS black holes
• Acceleration of electric current-carrying string loop near a Schwarzschild black hole immersed in an asymptotically uniform magnetic field
• Weakly charged generalized Kerr-NUT-(A)dS spacetimes

Cited by in corpus (9)

• 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
• Kerr-Newman black hole in a Melvin-swirling universe
• Bianchi IX geometry and the Einstein-Maxwell theory
• Spontaneous pair production near magnetized Reissner-Nordstrom black holes
• 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