Holographic duals of evaporating black holes

Abstract

We describe the dynamical evaporation of a black hole as the classical evolution in time of a black hole in an Anti-de Sitter braneworld. A bulk black hole whose horizon intersects the brane yields the classical bulk dual of a black hole coupled to quantum conformal fields. The evaporation of this black hole happens when the bulk horizon slides off the brane, making the horizon on the brane shrink. We use a large-D effective theory of the bulk Einstein equations to solve the time evolution of these systems. With this method, we study the dual evaporation of a variety of black holes interacting with colder radiation baths. We also obtain the dual of the collapse of holographic radiation to form a black hole on the brane. Finally, we discuss the evolution of the Page curve of the radiation in our evaporation setups, with entanglement islands appearing and then shrinking during the decreasing part of the curve.

27 pages, 13 figures. v2: 31 pages, 16 figures. Improved discussions, refs added. v3: matches published version

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Cited by in corpus (9)

• Massless Entanglement Islands in Cone Holography
• Quantum Kerr-de Sitter black holes in three dimensions
• Ghost Problem, Spectrum Identities and Various Constraints on Brane-localized Gravity
• Page Curve of AdS-Vaidya Model for Evaporating Black Holes
• Binary AdS black holes coupled to a bath in Type IIB
• Cone Holography with Neumann Boundary Conditions and Brane-localized Gauge Fields
• Unveiling horizons in quantum critical collapse
• Non-trivial saddles in microscopic description of black holes
• Primordial black holes in Randall-Sundrum: Cosmological signatures