Repulsive gravity effects in horizon formation. Horizon remnants in naked singularities
From MaRDI portal
Publication:2059765
DOI10.1007/S10714-021-02858-4zbMath1483.83061OpenAlexW3202158741MaRDI QIDQ2059765
Hernando Quevedo, Daniela Pugliese
Publication date: 14 December 2021
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-021-02858-4
Black holes (83C57) Quantum optics (81V80) Space-time singularities, cosmic censorship, etc. (83C75)
Related Items (1)
Cites Work
- Unnamed Item
- Circular orbits and relative strains in Schwarzschild space-time
- The thermodynamics of black holes
- Collisional super-Penrose process and Wald inequalities
- Black hole-naked singularity dualism and the repulsion of two Kerr black holes due to spin-spin interaction
- On the spectrum of the radiation from a naked singularity
- Black holes as elementary particles
- Repulsive gravity near naked singularities and point massive particles
- Stationary black holes: uniqueness and beyond
- Sub-Planckian black holes and the generalized uncertainty principle
- Properties of the instantaneous ergo surface of a Kerr black hole
- The Black Hole Uncertainty Principle Correspondence
- Formation of naked singularities: The violation of cosmic censorship
- Black holes, star clusters, and naked singularities: numerical solution of Einstein’s equations
- Gravitation, thermodynamics and quantum theory
- Trapped surfaces and the nature of singularity in Lyraʼs geometry
- Causal nature and dynamics of trapping horizons in black hole collapse
- Gravitational Collapse and Spacetime Singularities
- Numerical approaches to spacetime singularities
This page was built for publication: Repulsive gravity effects in horizon formation. Horizon remnants in naked singularities