Two-point function of a quantum scalar field in the interior region of a Reissner-Nordstrom black hole
Assaf Lanir, Adam Levi, Amos Ori, Orr Sela

TL;DR
This paper derives explicit formulas for the two-point function of a massless scalar field inside a Reissner-Nordstrom black hole in different quantum states, enabling calculations of key physical quantities like the stress-energy tensor.
Contribution
It provides the first explicit internal two-point function expressions in terms of $lm\omega$ modes for Reissner-Nordstrom black holes, extending known external results.
Findings
Explicit internal two-point functions in Unruh and Hartle-Hawking states.
Formulas for the trace of the renormalized stress-energy tensor.
Connection between the trace and the d'Alembertian of $<\Phi^{2}>_{ren}$.
Abstract
We derive explicit expressions for the two-point function of a massless scalar field in the interior region of a Reissner-Nordstrom black hole, in both the Unruh and Hartle-Hawking quantum states. The two-point function is expressed in terms of the standard modes of the scalar field (those associated with a spherical harmonic and a temporal mode ), which can be conveniently obtained by solving an ordinary differential equation, the radial equation. These explicit expressions are the internal analogs of the well known results in the external region (originally derived by Christensen and Fulling), in which the two-point function outside the black hole is written in terms of the external modes of the field. They allow the computation of and the renormalized stress-energy tensor inside the black hole, after the radial…
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