Force-free magnetosphere attractors for near-horizon extreme and near-extreme limits of Kerr black hole

DOI10.1088/1361-6382/abdf70zbMath1481.83058arXiv2007.15662OpenAlexW3123244227MaRDI QIDQ5163337

Filippo Camilloni, Marta Orselli, Troels Harmark, Roberto Oliveri, Gianluca Grignani

Publication date: 3 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2007.15662

zbMATH Keywords

near-horizon geometryforce-free electrodynamicsforce-free magnetospheresnear-extreme Kerr black holes

Mathematics Subject Classification ID

Attractors (35B41) Black holes (83C57) Electromagnetic fields in general relativity and gravitational theory (83C50) Galactic and stellar structure (85A15) Einstein-Maxwell equations (83C22) Motion of the gyroscope (70E05)

Related Items (2)

Moving away from the near-horizon attractor of the extreme Kerr force-free magnetosphere ⋮ Blandford-Znajek monopole expansion revisited: novel non-analytic contributions to the power emission

Cites Work

• Black hole superradiance from Kerr/CFT
• 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
• Inspiral into Gargantua
• Exact solutions to force-free electrodynamics in black hole backgrounds
• Gravitational waves from plunges into Gargantua
• Consistent Blandford-Znajek expansion
• Moving away from the near-horizon attractor of the extreme Kerr force-free magnetosphere
• Polarization whorls from M87* at the event horizon telescope
• Corrigendum: Inspiral into Gargantua (2016 Class. Quantum Grav. 33 155002)
• Force-free electrodynamics near rotation axis of a Kerr black hole

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