A Nonsingular Two Dimensional Black Hole
M. Trodden (Brown University), V. Mukhanov (ETH Zuerich), R., Brandenberger (Brown University)

TL;DR
This paper introduces a 2D gravity model that smoothly transitions from Schwarzschild-like behavior at large distances to de Sitter space inside the horizon, avoiding singularities.
Contribution
It presents a novel 2D gravity model based on the Limiting Curvature Construction that produces nonsingular black hole solutions.
Findings
Solutions approach Schwarzschild metric at large r
Inside the horizon, solutions resemble de Sitter space
Model avoids singularities in 2D black holes
Abstract
We construct a model of gravity in 1+1 spacetime dimensions in which the solutions approach the Schwarzschild metric at large and de Sitter space far inside the horizon. Our model may be viewed as a two dimensional application of the `Limiting Curvature Construction' recently proposed by two of the authors.
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