Stochastic Quantum Mechanics in Curved Spaces: Application to Schwarzschild Black Holes

ABSTRACT In this work, we start from the hypothesis that the universe lives in a Gravitational Wave Background (GWB). From this hypothesis, it follows that space–time is not locally flat because we have to take into account the fluctuations of the GWB in space–time. This implies that sufficiently small particles will feel these oscillations, preventing them from following geodesic trajectories. Thus, in a previous work, it was shown that if these particles follow the geodesic trajectories plus a stochastic term due to space–time fluctuations, the field equation for these quantum particles is simply the Klein–Gordon equation in this arbitrary curved space–time. In this work, we analyze these geodesics plus the stochastic trajectories in a Schwarzschild black hole.

Authors

Institutions

Publication Details

Journal
Astronomische Nachrichten
Published
2025-03-01
DOI
https://doi.org/10.1002/asna.70007
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Stochastic Quantum Mechanics in Curved Spaces: Application to Schwarzschild Black Holes

Tonatiuh Matos, Juan S. Jerez‐Rodriguez
Astronomische Nachrichten
Black Holes and Theoretical Physics
article

Stochastic Quantum Mechanics in Curved Spaces: Application to Schwarzschild Black Holes

Tonatiuh Matos, Juan S. Jerez‐Rodriguez
article en

Abstract

ABSTRACT In this work, we start from the hypothesis that the universe lives in a Gravitational Wave Background (GWB). From this hypothesis, it follows that space–time is not locally flat because we have to take into account the fluctuations of the GWB in space–time. This implies that sufficiently small particles will feel these oscillations, preventing them from following geodesic trajectories. Thus, in a previous work, it was shown that if these particles follow the geodesic trajectories plus a stochastic term due to space–time fluctuations, the field equation for these quantum particles is simply the Klein–Gordon equation in this arbitrary curved space–time. In this work, we analyze these geodesics plus the stochastic trajectories in a Schwarzschild black hole.

Astronomische NachrichtenVol. 346(3-4)
Instituto Politécnico Nacional (MX), Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional (MX)
Openalex Percentile: Top 95%
Black Holes and Theoretical Physics
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.