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Coupling between gravitational and electromagnetic perturbations on Kerr spacetime

Fawzi Aly* and Dejan Stojkovic

  • *Contact author: mabbasal@buffalo.edu
  • Contact author: ds77@buffalo.edu

Phys. Rev. D 113, 104003 – Published 4 May, 2026

DOI: https://doi.org/10.1103/p4km-1fgf

Abstract

We extend our previous Schwarzschild metric-based studies of gravitational-electromagnetic (GEM) coupling to rotating black holes by working directly in a curvature-based Newman-Penrose/Teukolsky framework on Kerr spacetime. Within a minimally coupled Einstein-Maxwell system, we derive explicit quadratic electromagnetic source terms for the spin-2 Teukolsky equation, providing a foundation for future numerical studies of GEM interactions in the framework of black-hole spectroscopy. Moreover, we give order-of-magnitude arguments showing that GEM quadratic quasinormal modes (QQNMs) can become relevant in a range of charged and magnetized astrophysical scenarios. Finally, we show through a brief dilaton-theory example that the GEM QQNM spectrum is sensitive to how gravity couples to electromagnetism, thereby providing a model-based way to test minimal coupling and to constrain hidden U(1) sectors with gravitational-wave observations.

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