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Main Authors: Paul, Ribhu, Chakraborty, Sumanta
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2312.13954
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author Paul, Ribhu
Chakraborty, Sumanta
author_facet Paul, Ribhu
Chakraborty, Sumanta
contents We have demonstrated that the wave functional describing the quantum nature of the spacetime inside the black hole horizon, vanishes near the singularity, using the path integral formalism. This is akin to the DeWitt criterion, applied to the interior of a Schwarzschild black hole. To achieve the same we have expressed the interior of a Schwarzschild black hole as a Kantowski-Sachs spacetime and have applied the minisuperspace formalism to determine an exact form of the propagator, and hence the wave function near the singularity, using path integral over the reduced phase space. It is to be emphasized that our result is exact and not a saddle point approximation to the path integral.
format Preprint
id arxiv_https___arxiv_org_abs_2312_13954
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Singularity avoidance from path integral
Paul, Ribhu
Chakraborty, Sumanta
General Relativity and Quantum Cosmology
We have demonstrated that the wave functional describing the quantum nature of the spacetime inside the black hole horizon, vanishes near the singularity, using the path integral formalism. This is akin to the DeWitt criterion, applied to the interior of a Schwarzschild black hole. To achieve the same we have expressed the interior of a Schwarzschild black hole as a Kantowski-Sachs spacetime and have applied the minisuperspace formalism to determine an exact form of the propagator, and hence the wave function near the singularity, using path integral over the reduced phase space. It is to be emphasized that our result is exact and not a saddle point approximation to the path integral.
title Singularity avoidance from path integral
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2312.13954