Gauge fixing and the Hamiltonian for cylindrical spacetimes

TL;DR

This paper develops a complete gauge fixing for cylindrical vacuum spacetimes, deriving a simplified Hamiltonian formalism that captures key physical parameters like angular and linear momentum, and explores solutions including spinning cosmic strings.

Contribution

It introduces a gauge fixing that results in a constraint-free model with explicit metric expressions and a well-defined Hamiltonian for cylindrical spacetimes, including solutions with non-zero angular momentum.

Findings

Derived explicit metric in terms of physical degrees of freedom.

Calculated the reduced Hamiltonian and its bounds.

Found solutions with constant fields and analyzed their properties.

Abstract

We introduce a complete gauge fixing for cylindrical spacetimes in vacuo that, in principle, do not contain the axis of symmetry. By cylindrically symmetric we understand spacetimes that possess two commuting spacelike Killing vectors, one of them rotational and the other one translational. The result of our gauge fixing is a constraint-free model whose phase space has four field-like degrees of freedom and that depends on three constant parameters. Two of these constants determine the global angular momentum and the linear momentum in the axis direction, while the third parameter is related with the behavior of the metric around the axis. We derive the explicit expression of the metric in terms of the physical degrees of freedom, calculate the reduced equations of motion and obtain the Hamiltonian that generates the reduced dynamics. We also find upper and lower bounds for this reduced Hamiltonian that provides the energy per unit length contained in the system. In addition, we show that the reduced formalism constructed is well defined and consistent at least when the linear momentum in the axis direction vanishes. Furthermore, in that case we prove that there exists an infinite number of solutions in which all physical fields are constant both in the surroundings of the axis and at sufficiently large distances from it. If the global angular momentum is different from zero, the isometry group of these solutions is generally not orthogonally transitive. Such solutions generalize the metric of a spinning cosmic string in the region where no closed timelike curves are present.