Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University
Phys. Rev. D 107(10), 104014 (2023)
By considering a misaligned (asymptotically uniform) magnetic field in the background of a rotating black hole, we uncover a possibility for a highly nontrivial 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.”
@article{UTF885,
author = {Bičák, J. and Kubizňák, D. and Perche, T. R.},
title = {{Migrating Carrollian particles on magnetized black hole horizons}},
journal = {Phys. Rev. D},
volume = {107},
number = {10},
pages = {104014},
year = {2023},
doi = {10.1103/PhysRevD.107.104014},
eprint = {2302.11639},
archivePrefix = {arXiv},
}