On the physical parametrization and magnetic analogs of the Emparan-Teo dihole solution

Abstract

The Emparan-Teo non-extremal black dihole solution is reparametrized using Komar quantities and the separation distance as arbitrary parameters. We show how the potential $A_3$ can be calculated for the magnetic analogs of this solution in the Einstein-Maxwell and Einstein-Maxwell-dilaton theories. We also demonstrate that, similar to the extreme case, the external magnetic field can remove the supporting strut in the non-extremal black dihole too.

arXiv comment9 pages, 1 figure

References in corpus (5)

• Black diholes
• Macroscopic and Microscopic Description of Black Diholes
• The double-Reissner-Nordstrom solution and the interaction force between two spherically symmetric charged particles
• Black diholes with unbalanced magnetic charges
• Charged Rotating Black Holes in Equilibrium

Cited by in corpus (5)

• Analogs of the double-Reissner-Nordstrom solution in magnetostatics and dilaton gravity: mathematical description and some physical properties
• Stationary black diholes
• Discreteness of dyonic dilaton black holes
• Geodesic motion in a stationary dihole spacetime
• Binary Black Hole in a Double Magnetic Monopole Field