Migrating Carrollian particles on magnetized black hole horizons

Abstract

By considering a misaligned (asymptotically uniform) magnetic field in the background of a rotating black hole, we uncover a possibility for a highly non-trivial motion of Carrollian particles on the black hole horizon that is characterized by a time-dependent velocity field and reminds us (because of its latitudinal oscillations) of a 'monarch butterfly migration'.

6 pages, 3 figures

References in corpus (5)

• Conformal Carroll groups and BMS symmetry
• Alignment of Magnetized Accretion Disks and Relativistic Jets with Spinning Black Holes
• Dynamics of Carroll Particles
• The Black Hole Meissner Effect and Blandford-Znajek Jets
• Embedding of the Kerr-Newman Black Hole Surface in Euclidean Space