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Analysis of quantum effects inside spherical charged black holes
Phys. Rev. D 99, 061502(R) – Published 19 March, 2019
DOI: https://doi.org/10.1103/PhysRevD.99.061502
Abstract
We numerically compute the renormalized expectation value of a minimally coupled massless quantum scalar field in the interior of a four-dimensional Reissner-Nordstrom black hole, in both the Hartle-Hawking and Unruh states. To this end we use a recently developed mode-sum renormalization scheme based on covariant point splitting. In both quantum states, is found to approach a finite value at the inner horizon (IH). The final approach to the IH asymptotic value is marked by an inverse-power tail , where is the Regge-Wheeler “tortoise coordinate” and with for the Hartle-Hawking state and for the Unruh state. We also report here the results of an analytical computation of these inverse-power tails of near the IH. Our numerical results show very good agreement with this analytical derivation (for both the power index and the tail amplitude), in both quantum states. Finally, from this asymptotic behavior of we analytically compute the leading-order asymptotic behavior of the trace of the renormalized stress-energy tensor at the IH. In both quantum states this quantity is found to diverge like (with specified above and with a known parameter ). To the best of our knowledge, this is the first fully quantitative derivation of the asymptotic behavior of these renormalized quantities at the IH of a four-dimensional Reissner-Nordstrom black hole. In particular, this is the first conclusive result showing the divergence of the renormalized stress-energy tensor at the Cauchy horizon.
Physics Subject Headings (PhySH)
Corrections
27 May, 2021
Correction: The previously published Fig. 4 contained colored dots that were inconsistent with labeling in the caption and has been replaced.
Article Text
Supplemental Material
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