Stochastic Quantum Mechanics Trajectories Near Schwarzschild Horizon Black Holes

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Rodríguez, Juan S. Jerez-, Escobar-Aguilar, Eric S., Matos, Tonatiuh
Format: Preprint
Published: 2025
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866918451269861376
author Rodríguez, Juan S. Jerez-
Escobar-Aguilar, Eric S.
Matos, Tonatiuh
author_facet Rodríguez, Juan S. Jerez-
Escobar-Aguilar, Eric S.
Matos, Tonatiuh
contents This work explores the possibility of applying stochastic quantum mechanics to curved spacetimes, with an emphasis on the Schwarzschild black hole. After reviewing the fundamental concepts of this approach, the quantum stochastic equations are extended to curved spacetime using a fully covariant treatment. Subsequently, the Klein-Gordon equation is solved for scalar perturbations, and the resulting stochastic trajectories are analyzed by varying parameters such as angular momentum, particle frequency, and computational integration time. In conclusion, we find that the trajectories are influenced by gravitational fluctuations in spacetime and that, depending on the variation of the fundamental parameters, different types of stochastic trajectories are obtained.
format Preprint
id arxiv_https___arxiv_org_abs_2512_05985
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Stochastic Quantum Mechanics Trajectories Near Schwarzschild Horizon Black Holes
Rodríguez, Juan S. Jerez-
Escobar-Aguilar, Eric S.
Matos, Tonatiuh
General Physics
This work explores the possibility of applying stochastic quantum mechanics to curved spacetimes, with an emphasis on the Schwarzschild black hole. After reviewing the fundamental concepts of this approach, the quantum stochastic equations are extended to curved spacetime using a fully covariant treatment. Subsequently, the Klein-Gordon equation is solved for scalar perturbations, and the resulting stochastic trajectories are analyzed by varying parameters such as angular momentum, particle frequency, and computational integration time. In conclusion, we find that the trajectories are influenced by gravitational fluctuations in spacetime and that, depending on the variation of the fundamental parameters, different types of stochastic trajectories are obtained.
title Stochastic Quantum Mechanics Trajectories Near Schwarzschild Horizon Black Holes
topic General Physics
url https://arxiv.org/abs/2512.05985