Noise Kernel for Self-similar Tolman Bondi Metric: Fluctuations on Cauchy Horizon

Abstract

We attempt to calculate the point separated Noise Kernel for self similar Tolman Bondi metric, using a method similar to that developed by Eftekharzadeh et. al for ultra-static spacetimes referring to the work by Page. In case of formation of a naked singularity, the Noise Kernel thus obtained is found to be regular except on the Cauchy horizon, where it diverges. The behavior of the noise in case of the formation of a covered singularity is found to be regular. This result seemingly renders back reaction non-negligible which questions the stability of the results obtained from the semiclassical treatment of the self similar Tolman Bondi metric.

References in corpus (2)

• Fate of gravitational collapse in semiclassical gravity
• Stochastic Gravity: Beyond Semiclassical Gravity

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