Reissner Nordstr\"{o}m Background Metric in Dynamical Co-ordinates: Exceptional Behaviour of Hadamard States
Sukratu Barve, A.R.Prasanna

TL;DR
This paper investigates the semiclassical behavior of the Reissner-Nordström black hole in a dynamical coordinate system, revealing differences from dust collapse models and analyzing the stability and quantum effects near horizons and singularities.
Contribution
It introduces a coordinate system for Reissner-Nordström solutions that captures dynamical evolution and examines the global validity of Wald axioms with Hadamard states, comparing semiclassical effects to dust collapse.
Findings
Divergence on the Cauchy horizon confirmed
Semiclassical domain extends up to the Cauchy horizon
Backreaction is significant near the central singularity
Abstract
We cast the Reissner Nordstrom solution in a particular co-ordinate system which shows dynamical evolution from initial data. The initial data for the case is regular. This procedure enables us to treat the metric as a collapse to a singularity. It also implies that one may assume Wald axioms to be valid globally in the Cauchy development, especially when Hadamard states are chosen. We can thus compare the semiclassical behaviour with spherical dust case, looking upon the metric as well as state specific information as evolution from initial data. We first recover the divergence on the Cauchy horizon obtained earlier. We point out that the semiclassical domain extends right upto the Cauchy horizon. This is different from the spherical dust case where the quantum gravity domain sets in before. We also find that the backreaction is not negligible near the central singularity, unlike…
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