Gravitational eigenstates in weak gravity I: dipole decay rates of charged particles
A D Ernest

TL;DR
This paper develops analytical formulas for electromagnetic transition rates between gravitational eigenstates of charged particles, revealing that high angular momentum states can have unexpectedly long lifetimes, indicating potential stability in weak gravitational fields.
Contribution
It introduces non-relativistic, analytic expressions for dipole transition rates in gravitational eigenstates, a novel approach in gravitational quantum state analysis.
Findings
High angular momentum states have very long lifetimes.
Some gravitational eigenstates exhibit unexpected stability.
Transition rate formulas enable analysis of gravitational quantum states.
Abstract
The experimental demonstration that neutrons can reside in gravitational quantum stationary states formed in the gravitational field of the Earth indicates a need to examine in more detail the general theoretical properties of gravitational eigenstates. Despite the almost universal study of quantum theory applied to atomic and molecular states very little work has been done to investigate the properties of the hypothetical stationary states that should exist in similar types of gravitational central potential wells, particularly those with large quantum numbers. In this first of a series of papers, we attempt to address this shortfall by developing analytic, non-integral expressions for the electromagnetic dipole state-to-state transition rates of charged particles for any given initial and final gravitational quantum states. The expressions are non-relativistic and hence valid provided…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
