Size and momentum of an infalling particle in the black hole interior
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Publication:2044872
DOI10.1007/JHEP06(2021)056zbMath1466.83031arXiv2102.05697MaRDI QIDQ2044872
Publication date: 10 August 2021
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2102.05697
Black holes (83C57) Quantization of the gravitational field (83C45) Analogues of general relativity in lower dimensions (83C80) Operator algebra methods applied to problems in quantum theory (81R15) Equations of motion in general relativity and gravitational theory (83C10) Correspondence, duality, holography (AdS/CFT, gauge/gravity, etc.) (81T35)
Related Items (9)
Operator growth and black hole formation ⋮ Scattering strings off quantum extremal surfaces ⋮ Collisions of localized shocks and quantum circuits ⋮ Bouncing inside the horizon and scrambling delays ⋮ The special role of toroidal black holes in holography ⋮ Six-point functions and collisions in the black hole interior ⋮ Random matrix theory for complexity growth and black hole interiors ⋮ Quantum error correction in SYK and bulk emergence ⋮ Seeing behind black hole horizons in SYK
Cites Work
- Black holes: complementarity or firewalls?
- Time evolution of entanglement entropy from black hole interiors
- Shockwave S-matrix from Schwarzian quantum mechanics
- Degenerate operators and the \(1/c\) expansion: Lorentzian resummations, high order computations, and super-Virasoro blocks
- Localized shocks
- Collision in the interior of wormhole
- Rescuing a black hole in the large-\(q\) coupled SYK model
- Quantum epidemiology: operator growth, thermal effects, and SYK
- Symmetries near the horizon
- Stringy effects in scrambling
- Entanglement is not enough
- The typical-state paradox: diagnosing horizons with complexity
- Conformal symmetry and its breaking in two-dimensional nearly anti-de Sitter space
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