A Dirac Sea of Quantized Superluminal States in the Kerr-Newman Disk

TL;DR

This paper models the Kerr-Newman disk as a Dirac sea of quantized superluminal particles, deriving their energy and momentum states, and suggesting the disk's possible excited states within this framework.

Contribution

It introduces a novel quantized superluminal particle model for the Kerr-Newman disk, linking discrete superluminal states to the disk's continuous density profile.

Findings

Derived quantized energy and momentum states for superluminal orbits.

Proposed the Kerr-Newman disk as a Dirac sea of superluminal states.

Identified potential excited states of the disk.

Abstract

We model the continuous material component of the Kerr-Newman disk as a discrete distribution of superluminal particles undergoing quantized orbital rotation with velocity $v/c = a/r$. By matching the discrete distribution in the continuous limit with the Kerr disk densities, we derive the quantized energy and momentum states of the superluminal orbits. We conclude that the Kerr-Newman disk may be modeled as a Dirac sea of these superluminal states and we identify possible excited states of the disk.