Migrating Carrollian particles on magnetized black hole horizons
arXiv:2302.11639 · doi:10.1103/PhysRevD.107.104014
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'.
arXiv comment6 pages, 3 figures
References in corpus (15)
- Spin Hall effect
- Conformal Carroll groups and BMS symmetry
- Alignment of Magnetized Accretion Disks and Relativistic Jets with Spinning Black Holes
- Carrollian Physics at the Black Hole Horizon
- Dynamics of Carroll Particles
- Bardeen-Petterson Alignment, Jets and Magnetic Truncation in GRMHD Simulations of Tilted Thin Accretion Discs
- Carrollian hydrodynamics from symmetries
- Superconducting p-branes and Extremal Black Holes
- Near-horizon description of extremal magnetised stationary black holes and Meissner effect
- The Black Hole Meissner Effect and Blandford-Znajek Jets
- Influence of frame-dragging on magnetic null points near rotating black hole
- Rotating black hole hair
- Embedding of the Kerr-Newman Black Hole Surface in Euclidean Space
- Carrollian Motion in Magnetized Black Hole Horizons
- Magnetic Alignment Process : A New Mechanism for Extracting Energy from Rotating Black Holes
Cited by in corpus (8)
- Spin Hall effects in the sky
- Weyl geometric effects on the propagation of light in gravitational fields
- Carrollian limit of quadratic gravity
- Uniqueness of Galilean and Carrollian limits of gravitational theories and application to higher derivative gravity
- Supersymmetric Carroll Galileons in Three Dimensions
- Fracton and Non-Lorentzian Particle Duality: Gauge Field Couplings and Geometric Implications
- Carroll black holes in (A)dS and their higher-derivative modifications
- Universal sectors of two-dimensional Carrollian CFTs