Moving away from the near-horizon attractor of the extreme Kerr force-free magnetosphere
DOI10.1088/1475-7516/2020/10/048zbMath1494.83019arXiv2007.15665OpenAlexW3102742776MaRDI QIDQ5071000
Marta Orselli, Troels Harmark, Roberto Oliveri, Filippo Camilloni, Gianluca Grignani
Publication date: 14 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2007.15665
Attractors and repellers of smooth dynamical systems and their topological structure (37C70) Black holes (83C57) Magnetohydrodynamics and electrohydrodynamics (76W05) Electromagnetic fields in general relativity and gravitational theory (83C50) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Perturbations in context of PDEs (35B20) Galactic and stellar structure (85A15)
Related Items (4)
Cites Work
- Unnamed Item
- Unnamed Item
- Force-free electrodynamics around extreme Kerr black holes
- A class of exact solutions to the force-free, axisy,metric, stationary magnetosphere of a Kerr black hole
- Exact solutions for extreme black hole magnetospheres
- Exact solutions to force-free electrodynamics in black hole backgrounds
- Robustness of the Blandford–Znajek mechanism
- Near-horizon symmetries of extremal black holes
- MHD Flows in Compact Astrophysical Objects
- Consistent Blandford-Znajek expansion
- Force-free electrodynamics near rotation axis of a Kerr black hole
- Force-free magnetosphere attractors for near-horizon extreme and near-extreme limits of Kerr black hole
- The Kerr/CFT correspondence and its extensions
This page was built for publication: Moving away from the near-horizon attractor of the extreme Kerr force-free magnetosphere
