Long-range correlations of the stress tensor near the Cauchy horizon
arXiv:2311.06068 · doi:10.1103/PhysRevD.109.L061702
Abstract
We show that the stress tensor of a real scalar quantum field on Reissner-Nordstr{ö}m-de Sitter spacetime exhibits correlations over macroscopic distances near the Cauchy horizon. These diverge as the Cauchy horizon is approached and are universal, i.e., state-independent. This signals a breakdown of the semi-classical approximation near the Cauchy horizon. We also investigate the effect of turning on a charge of the scalar field and consider the correlation of the stress tensor between the two poles of the Cauchy horizon of Kerr-de Sitter spacetime.
5 pages, 4 figures, version as published in PRD
References in corpus (12)
- A Spin Entanglement Witness for Quantum Gravity
- Gravitationally-induced entanglement between two massive particles is sufficient evidence of quantum effects in gravity
- Quasinormal modes and Strong Cosmic Censorship
- Gravitationally Mediated Entanglement: Newtonian Field vs. Gravitons
- Mode-sum regularization of in the angular-splitting method
- Quantum stress tensor at the Cauchy horizon of Reissner-Nordström-deSitter spacetime
- Classical mass inflation vs semiclassical inner horizon inflation
- Hawking radiation inside a charged black hole
- Quantum correlations across the horizon in acoustic and gravitational Black Holes
- Quantum fluxes at the inner horizon of a near-extremal spherical charged black hole
- Quantum correlator outside a Schwarzschild black hole
- Quantum energy momentum tensor and equal time correlations in a Reissner-Nordström black hole