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Black Hole Formation in AdS and Thermalization on the Boundary

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arxiv hep-th/9912209 v2 pith:6JFNKS26 submitted 1999-12-21 hep-th

classification hep-th
keywords shellblackboundaryholeholographiccollapsingequilibriumformation
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We investigate black hole formation by a spherically collapsing thin shell of matter in AdS space. This process has been suggested to have a holographic interpretation as thermalization of the CFT on the boundary of the AdS space. The AdS/CFT duality relates the shell in the bulk to an off-equilibrium state of the boundary theory which evolves towards a thermal equilibrium when the shell collapses to a black hole. We use 2-point functions to obtain information about the spectrum of excitations in the off-equilibrium state, and discuss how it characterizes the approach towards thermal equilibrium. The full holographic interpretation of the gravitational collapse would require a kinetic theory of the CFT at strong coupling. We speculate that the kinetic equations should be interpreted as a holographic dual of the equation of motion of the collapsing shell.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Black-hole formation and thermalization in open JT gravity

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    Numerical simulations show dynamical black hole formation in non-Markovian open JT gravity, corresponding to irreversible thermalization on the boundary.

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  4. Random matrix theory signatures in free field theory

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    In finite-volume massive free scalar field theory after local quench, spacing ratios of two-point function extrema follow GOE statistics and an extrema-based form factor shows RMT dip-ramp-plateau.

  5. Blackish Holes

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    Placing a Dirichlet wall just outside the BTZ horizon produces a dense spectrum of normal modes that, in the continuum limit, yields a thermal two-point function at the Hawking temperature.

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