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• W2275618008 abstract "We obtain point separated Noise Kernel for the Reissner Nordstr{o}m metric.The Noise Kernel defines the fluctuations of the quantum stress tensor and is of central importance to Semiclassical Stochastic Gravity.The metric is modeled as gravitationally collapsing spacetime, by using suitable coordinate transformations, defined earlier. The fluctuations of the quantum stress tensor, at the final stage of collapse are then analysed for both, the naked singularity and black hole end states. The behavior of this Noise Kernel, at the Cauchy Horizon for naked singularity shows markedly different behaviour from self similar Tolman Bondi metric, which was obtained earlier. In the latter a very unique divergence was seen, which does not appear for the Reissner Nordstr{o}m metric, here . It is known that the quantum stress tensor itself, diverges at the Cauchy Horizon (CH) for both of these metrics . In contrast, it can now be seen that the the fluctuations of the stress tensor behave differently for the two cases. We give a discussion and further directions for investigations of this interesting behaviour in the two cases (regarding the collapse scenario)." @default.
• W2275618008 created "2016-06-24" @default.
• W2275618008 creator A5022333779 @default.
• W2275618008 date "2016-04-06" @default.
• W2275618008 modified "2023-09-27" @default.
• W2275618008 title "Noise kernel for the Reissner-Nordström metric: Results at the Cauchy horizon" @default.
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• W2275618008 doi "https://doi.org/10.1103/physrevd.93.084007" @default.
• W2275618008 hasPublicationYear "2016" @default.
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