A Unitary S-matrix for 2D Black Hole Formation and Evaporation
Erik Verlinde, Herman Verlinde

TL;DR
This paper constructs a unitary quantum S-matrix for a 2D dilaton gravity model with scalar fields, demonstrating black hole formation and evaporation, and draws parallels with the c=1 matrix model.
Contribution
It introduces a well-defined 2D toy model with a unitary S-matrix that captures black hole dynamics and connects it to matrix model results.
Findings
The S-matrix is explicitly constructed and shown to be unitary.
The model describes black hole formation and Hawking evaporation.
A correspondence with the c=1 matrix model is established.
Abstract
We study the black hole information paradox in the context of a two-dimensional toy model given by dilaton gravity coupled to massless scalar fields. After making the model well-defined by imposing reflecting boundary conditions at a critical value of the dilaton field, we quantize the theory and derive the quantum quantum -matrix for the case that =. This -matrix is unitary by construction, and we further argue that in the semiclassical regime it describes the formation and subsequent Hawking evaporation of two-dimensional black holes. Finally, we note an interesting correspondence between the dilaton gravity -matrix and that of the matrix model.
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