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Nonzero Love numbers of magnetic black holes

David Pereñiguez1,2,* and Edgars Karnickis2,†

  • 1William H. Miller III Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218, USA
  • 2Center of Gravity, Niels Bohr Institute, Blegdamsvej 17, 2100, Copenhagen, Denmark

  • *Contact author: dpereni1@jhu.edu
  • †Contact author: edgars.karnickis@gmail.com

Phys. Rev. D 113, L081502 – Published 6 April, 2026

DOI: https://doi.org/10.1103/m8wj-gxss

Abstract

Black holes are believed to possess vanishing Love numbers, which implies that they do not deform in the presence of external tides. This fact has been verified in a number of scenarios that involve tides of bosonic fields of various natures (e.g., scalar, electromagnetic, and gravitational) and has triggered active research in trying to identify the underlying reason. Surprisingly, two counterexamples have been found recently. The first concerns charged-field tides on electrically charged black holes. In that case, however, the response cannot be disentangled from dissipative effects, and might thus be argued to not consist of a truly conservative deformation. The second concerns fermionic tides on neutral holes. While these yield a purely conservative response, they lack a classical interpretation, which is the physical regime where black hole deformability is understood. Here, we consider magnetic Reissner-Nordström black holes and show that electrically charged, scalar-field tides induce nonvanishing tidal Love numbers. We prove that this is a purely nondissipative effect, in contrast to the cases of rotating or electrically charged black holes, and hence consists of a genuine deformation. In addition, the magnetic charge resolves common ambiguities in defining Love numbers, so our result does not rely on any regularization scheme. This constitutes a clear realization of how new physics can influence black hole tidal deformability and offers new perspectives on the study of black hole Love numbers.

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