The effect of radiative gravitational modes on the dynamics of a cylindrical shell of counter rotating particles

TL;DR

This paper investigates the relativistic dynamics of a cylindrical shell of counter rotating particles, revealing that gravitational radiative modes significantly influence shell motion, including oscillations, collapsing, and unbounded behaviors, with solutions decoupled from gravitational modes in certain cases.

Contribution

It demonstrates a family of solutions where the shell's motion is independent of gravitational modes and shows that radiative modes determine shell dynamics, including oscillations and collapse.

Findings

Existence of solutions with flat interior and decoupled shell motion.

Shell dynamics can be oscillatory, collapsing, or unbounded.

Radiative modes fully determine the shell's motion.

Abstract

In this paper we consider some aspects of the relativistic dynamics of a cylindrical shell of counter rotating particles. In some sense these are the simplest systems with a physically acceptable matter content that display in a well defined sense an interaction with the radiative modes of the gravitational field. These systems have been analyzed previously, but in most cases resorting to approximations, or considering a particular form for the initial value data. Here we show that there exists a family of solutions where the space time inside the shell is flat and the equation of motion of the shell decouples completely from the gravitational modes. The motion of the shell is governed by an equation of the same form as that of a particle in a time independent one dimensional potential. We find that under appropriate initial conditions one can have collapsing, bounded periodic, and unbounded motions. We analyze and solve also the linearized equations that describe the dynamics of the system near a stable static solutions, keeping a regular interior. The surprising result here is that the motion of the shell is completely determined by the configuration of the radiative modes of the gravitational field. In particular, there are oscillating solutions for any chosen period, in contrast with the "approximately Newtonian plus small radiative corrections" motion expectation. We comment on the physical meaning of these results and provide some explicit examples. We also discuss the relation of our results to the initial value problem for the linearized dynamics of the shell.