Action complexity for semi-classical black holes

DOI10.1007/JHEP07(2020)173zbMath1451.83058arXiv2001.06453MaRDI QIDQ2215415

Lukas Schneiderbauer, Watse Sybesma, Larus Thorlacius

Publication date: 11 December 2020

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2001.06453

zbMATH Keywords

black holes2D gravity

Mathematics Subject Classification ID

Black holes (83C57) Geometrodynamics and the holographic principle (83E05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Analogues of general relativity in lower dimensions (83C80)

Related Items (5)

Gravitation from optimized computation: Einstein and beyond ⋮ Holographic complexity of rotating quantum black holes ⋮ Krylov complexity of open quantum systems: from hard spheres to black holes ⋮ Pure de Sitter space and the island moving back in time ⋮ Holographic complexity of quantum black holes

Cites Work

• Holographic complexity in Vaidya spacetimes. I.
• A boundary term for the gravitational action with null boundaries
• Comments on holographic complexity
• On the time dependence of holographic complexity
• Holographic complexity equals which action?
• Three lectures on complexity and black holes
• Holographic complexity: stretching the horizon of an evaporating black hole
• Models of \(\mathrm{AdS}_{2}\) backreaction and holography
• Computational complexity and black hole horizons
• Black hole evolution
• Symmetries and solvable models for evaporating \(2\)D black holes

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