Quantum Mechanics of the Interior of the Russo-Susskind-Thorlacius Black Hole
Ramin G. Daghigh, Michael D. Green, Gabor Kunstatter

TL;DR
This paper investigates the quantum behavior of black hole interiors in a 2D gravity model, showing singularity resolution, oscillatory dilaton dynamics, and phenomena like revivals, providing insights into black hole evaporation at the quantum level.
Contribution
It provides an exact quantum analysis of the homogeneous black hole interior in the RST model, including the construction of self-adjoint Hamiltonians and numerical solutions of the Schrödinger equation.
Findings
Singularity is resolved in the quantum model.
Dilaton expectation value oscillates between decreasing bounds.
Quantum revivals occur in the long-term dynamics.
Abstract
We study the quantum mechanics of homogeneous black hole interiors in the RST model of 2D gravity. The model, which contains a dilaton and metric, includes radiation back-reaction terms and is exactly solvable classically. The reduced phase space is four dimensional. The equations for one pair of variables can be trivially solved. The dynamics of the remaining degree of freedom, namely the dilaton, is more interesting and corresponds to that of a particle on the half line in a linear potential with time dependent coupling. We construct the self-adjoint extension of the corresponding quantized Hamiltonian and numerically solve the time dependent Schrdinger equation for Gaussian initial data. As expected the singularity is resolved and the expectation value of the dilaton oscillates between a minimum and maximum, which both gradually decrease with time due to the time…
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