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Late Time Correlation Functions, Baby Universes, and ETH in JT Gravity · Around

2019

Late Time Correlation Functions, Baby Universes, and ETH in JT Gravity

Saad, Phil

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Quantum black holes are described by a large number of macroscopically indistinguishable microstates.

Correlation functions of fields outside the horizon at long time separation probe this indistinguishability.
The simplest of these, the thermal two-point function, oscillates erratically around a nonperturbatively small average "ramp" and "plateau" after an initial period of decay; these non-decaying averaged features are signatures of the discreteness of the black hole spectrum.
For a theory described by an ensemble of Hamiltonians, the two-point function follows this averaged behavior.

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