Interior metric and ray-tracing map in the firework black-to-white hole transition
Carlo Rovelli, Pierre Martin-Dussaud

TL;DR
This paper introduces an improved metric for the black-to-white hole transition via quantum tunnelling, providing a complete description of the process and an explicit ray-tracing map.
Contribution
It presents a refined metric that models the entire black-to-white hole transition and explicitly computes the associated ray-tracing map, advancing understanding of quantum gravitational effects.
Findings
The metric describes the full transition process.
The Einstein equations are solved except on a small transition surface.
An explicit ray-tracing map from past to future infinity is derived.
Abstract
The possibility that a black hole could tunnel into a white hole has recently received attention. Here we present a metric that improves the 'firework' metric: it describes the entire process and solves the Einstein equations everywhere except on a small transition surface that corresponds to the quantum tunnelling. We compute the corresponding ray-tracing map from past infinity to future infinity explicitly.
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