Alex Kehagias, Davide Perrone, Antonio Riotto
Published 2024-06-27Version 1
We provide a simple proof of why the Love number vanishes for extremal Reissner-Nordstrom and Kerr-Newman black holes. The argument is based on a conformal inversion isometry of the spacetime connecting the horizon with large distances.
Pair Production of Scalar Dyons in Kerr-Newman Black Holes
Nonextensive entropies impact onto thermodynamics and phase structure of Kerr-Newman black holes
Kerr-Newman Black Holes with String Corrections
![QR code for arXiv:2406.19262 [hep-th]](http://oss.arxitics.com/images/favicon.svg)