Astrophysical hints for magnetic black holes

TL;DR

This paper explores the potential astrophysical signatures and constraints of magnetically charged black holes, highlighting their unique electromagnetic and gravitational wave features that could be observable and provide insights into fundamental physics.

Contribution

It introduces new theoretical and observational considerations for detecting magnetic black holes, including their electromagnetic emissions, stable orbits, and gravitational wave signatures, expanding current understanding.

Findings

Stable orbits around magnetic black holes have distinctive features.

Electromagnetic emissions during binary inspirals can be extraordinarily bright.

Gravitational wave signals from magnetic black hole binaries show unique characteristics.

Abstract

We discuss a cornucopia of potential astrophysical signatures and constraints on magnetically charged black holes of various masses. As recently highlighted, being potentially viable astrophysical candidates with immense electromagnetic fields, they may be ideal windows to fundamental physics, electroweak symmetry restoration and non-perturbative quantum field theoretic phenomena. We investigate various potential astrophysical pointers and bounds -- including limits on charges, location of stable orbits and horizons in asymptotically flat and asymptotically de Sitter backgrounds, bounds from galactic magnetic fields and dark matter measurements, characteristic electromagnetic fluxes and tell-tale gravitational wave emissions during binary inspirals. Stable orbits around these objects hold an imprint of their nature and in the asymptotically de Sitter case, there is also a qualitatively new feature with the emergence of a stable outer orbit. We consider binary inspirals of both magnetic and neutral, and magnetic and magnetic, black hole pairs. The electromagnetic emissions and the gravitational waveform evolution, along with inter-black hole separation, display distinct features. Many of the astrophysical signatures may be observationally glaring -- for instance, even in regions of parameter space where no electroweak corona forms, owing to magnetic fields that are still many orders of magnitude larger than even Magnetars, their consequent electromagnetic emissions will be spectacular during binary inspirals. While adding new results, our discussions also complement works in similar contexts, that have appeared recently in the literature.