Critical Collapse of Cylindrically Symmetric Scalar Field in Four-Dimensional Einstein's Theory of Gravity

TL;DR

This paper investigates cylindrically symmetric gravitational collapse of a massless scalar field in four-dimensional Einstein gravity, identifying critical solutions with one unstable mode that delineate different end states.

Contribution

It presents new exact solutions for cylindrically symmetric scalar field collapse and analyzes their stability, highlighting a potential critical solution with a single unstable mode.

Findings

Existence of solutions leading to black holes with cylindrical symmetry.

Identification of a critical solution with one unstable mode.

Stability analysis of the solutions through linear perturbations.

Abstract

Four-dimensional cylindrically symmetric spacetimes with homothetic self-similarity are studied in the context of Einstein's Theory of Gravity, and a class of exact solutions to the Einstein-massless scalar field equations is found. Their local and global properties are investigated and found that they represent gravitational collapse of a massless scalar field. In some cases the collapse forms black holes with cylindrical symmetry, while in the other cases it does not. The linear perturbations of these solutions are also studied and given in closed form. From the spectra of the unstable eigen-modes, it is found that there exists one solution that has precisely one unstable mode, which may represent a critical solution, sitting on a boundary that separates two different basins of attraction in the phase space.