Black holes, white holes, and near-horizon physics
From MaRDI portal
Publication:6568176
DOI10.1007/jhep05(2024)172MaRDI QIDQ6568176
Publication date: 5 July 2024
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Cites Work
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- Evaporating firewalls
- Black holes: complementarity or firewalls?
- The flaw in the firewall argument
- Physical wavelets: Lorentz covariant, singularity-free, finite energy, zero action, localized solutions to the wave equation
- On white holes as particle accelerator
- Black holes turn white fast, otherwise stay black: no half measures
- Quantum black hole-white hole entangled states
- On the viability of regular black holes
- Can we observe fuzzballs or firewalls?
- Perturbations of the Kerr spacetime in horizon-penetrating coordinates
- Black to white hole tunneling: An exact classical solution
- Testing the black hole ‘no-hair’ hypothesis
- White holes and eternal black holes
- Stable gravastars with generalized exteriors
- SINGULARITY AVOIDANCE BY COLLAPSING SHELLS IN QUANTUM GRAVITY
- How to tell a gravastar from a black hole
- The information paradox: a pedagogical introduction
- Stable gravastars—an alternative to black holes?
- From black holes to white holes: a quantum gravitational, symmetric bounce
- TWILIGHT FOR THE ENERGY CONDITIONS?
- Towards consistent black-to-white hole bounces from matter collapse
- Evaporating black-to-white hole
- Energy conditions in general relativity and quantum field theory
- Mass and horizon Dirac observables in effective models of quantum black-to-white hole transition
- The lifetime problem of evaporating black holes: mutiny or resignation
- Effective black-to-white hole bounces: the cost of surgery
- Empty black holes, firewalls, and the origin of Bekenstein–Hawking entropy
- Exponential fading to white of black holes in quantum gravity
- Spacetime and Geometry
- The fuzzball proposal for black holes: an elementary review
- Gravastars must have anisotropic pressures
- General Relativity
- Unitary dynamics of spherical null gravitating shells
- A connection between regular black holes and horizonless ultracompact stars
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