2021
DOI: 10.48550/arxiv.2104.06005
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The renormalized charged scalar current in the Reissner-Nordström-de Sitter spacetime

Christiane Klein,
Jochen Zahn

Abstract: We perform a Hadamard point-split renormalization of the current density jν of a charged scalar field in a Reissner-Nordström-de Sitter spacetime. We compute numerically the expectation values of the components jr and jt in the Unruh state in the exterior region and study their dependence on the field parameters and the position.

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Cited by 1 publication
(3 citation statements)
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“…That horizons with equal surface gravities emerge as the exceptionally regular special case may not be surprising: that this case is special was already known from consideration of the stress-energy tensor [15][16][17] , and similar observations arise with 'lukewarm' black holes, in which two Killing horizons bound a spacetime region in which the Killing vector in question is timelike 42,43 . It is however notable that in the HHI state, the overall sign of the leading divergence is determined by which of the two surface gravities is greater, in precisely the same way for both the detector's transition rate and for the energy density seen by an observer.…”
Section: Discussionmentioning
confidence: 79%
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“…That horizons with equal surface gravities emerge as the exceptionally regular special case may not be surprising: that this case is special was already known from consideration of the stress-energy tensor [15][16][17] , and similar observations arise with 'lukewarm' black holes, in which two Killing horizons bound a spacetime region in which the Killing vector in question is timelike 42,43 . It is however notable that in the HHI state, the overall sign of the leading divergence is determined by which of the two surface gravities is greater, in precisely the same way for both the detector's transition rate and for the energy density seen by an observer.…”
Section: Discussionmentioning
confidence: 79%
“…When the theory is extended to include quantised fields, new issues arise from the renormalised stressenergy tensor near the Cauchy horizon, and from the back-reaction of this stress-energy on the spacetime. There is evidence that the back-reaction of the quantum fields tends to make Cauchy horizons generically unstable even in situations where classical surface gravity considerations would suggest stability [13][14][15][16][17] .…”
Section: Introductionmentioning
confidence: 99%
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