Super-spinning Kerr attractors: observational signatures of accretion tori and proto-jets
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Publication:6159648
DOI10.1016/j.nuclphysb.2023.116229zbMath1523.83048MaRDI QIDQ6159648
Zdeněk Stuchlík, Daniela Pugliese
Publication date: 20 June 2023
Published in: Nuclear Physics. B (Search for Journal in Brave)
Attractors (35B41) Toric varieties, Newton polyhedra, Okounkov bodies (14M25) Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Motion of the gyroscope (70E05) Causal inference from observational studies (62D20)
Cites Work
- Repulsive gravity effects in horizon formation. Horizon remnants in naked singularities
- Observational phenomena related to primordial Kerr superspinars
- Appearance of Keplerian discs orbiting Kerr superspinars
- Evolution of Kerr superspinars due to accretion counterrotating thin discs
- Kerr naked singularities as particle accelerators
- Proto-jet configurations in RADs orbiting a Kerr SMBH: symmetries and limiting surfaces
- Stabilization of non-axisymmetric instabilities in a rotating flow by accretion on to a central black hole
- Ultra-high-energy collisions in the superspinning Kerr geometry
- Accretion disks around naked singularities
- Global Structure of the Kerr Family of Gravitational Fields
- Numerical hydrodynamics in general relativity
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