Intrinsic Heisenberg Lower Bounds on Schwarzschild and Weyl-Class Spacelike Slices

Fuente: arXiv
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Main Author: Schürmann, Thomas
Format: Preprint
Published: 2025
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author Schürmann, Thomas
author_facet Schürmann, Thomas
contents We establish a coordinate-invariant Heisenberg-type lower bound for quantum states strictly localized in geodesic balls of radius $r_g$ on horizon-regular spacelike slices of static, spherically symmetric, asymptotically flat (AF) black-holes. Via a variance-eigenvalue equivalence the momentum uncertainty reduces to the first Dirichlet eigenvalue of the Laplace-Beltrami operator, yielding a slice-uniform Hardy baseline $σ_p r_g \ge \hbar/2$ under mild convexity assumptions on the balls; the bound is never attained and admits a positive gap both on compact interior regions and uniformly far out. For the Schwarzschild Painlevé-Gullstrand (PG) slice, whose induced 3-geometry is Euclidean, one recovers the exact Euclidean scale $σ_p r_g \ge π\hbar$, which is optimal among all admissible slices. The entire construction extends across the black-hole horizon, and it transfers to the static axisymmetric Weyl class, where the Hardy floor, strict gap, and AF $π$-scale persist (a global PG-like optimum need not exist).
format Preprint
id arxiv_https___arxiv_org_abs_2509_19099
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Intrinsic Heisenberg Lower Bounds on Schwarzschild and Weyl-Class Spacelike Slices
Schürmann, Thomas
General Relativity and Quantum Cosmology
Quantum Physics
We establish a coordinate-invariant Heisenberg-type lower bound for quantum states strictly localized in geodesic balls of radius $r_g$ on horizon-regular spacelike slices of static, spherically symmetric, asymptotically flat (AF) black-holes. Via a variance-eigenvalue equivalence the momentum uncertainty reduces to the first Dirichlet eigenvalue of the Laplace-Beltrami operator, yielding a slice-uniform Hardy baseline $σ_p r_g \ge \hbar/2$ under mild convexity assumptions on the balls; the bound is never attained and admits a positive gap both on compact interior regions and uniformly far out. For the Schwarzschild Painlevé-Gullstrand (PG) slice, whose induced 3-geometry is Euclidean, one recovers the exact Euclidean scale $σ_p r_g \ge π\hbar$, which is optimal among all admissible slices. The entire construction extends across the black-hole horizon, and it transfers to the static axisymmetric Weyl class, where the Hardy floor, strict gap, and AF $π$-scale persist (a global PG-like optimum need not exist).
title Intrinsic Heisenberg Lower Bounds on Schwarzschild and Weyl-Class Spacelike Slices
topic General Relativity and Quantum Cosmology
Quantum Physics
url https://arxiv.org/abs/2509.19099