# Cosmic Strings in Conformal Gravity

## TL;DR

This paper derives exact solutions for spinning cosmic strings in conformal gravity, revealing how their spacetime structure can avoid closed timelike curves and connect to higher-dimensional models, highlighting conformal invariance's role in unifying gravity and quantum theory.

## Contribution

It provides exact exterior solutions for spinning cosmic strings in conformal gravity and demonstrates their relation to five-dimensional brane world models.

## Key findings

- J falls off as 1/r near the core
- Spacetime is Ricci flat
- Closed timelike curves can be avoided at infinity

## Abstract

We investigate the spacetime of a spinning cosmic string in conformal invariant gravity, where the interior consists of a gauged scalar field. We find exact solutions of the exterior of a stationary spinning cosmic string, where we write the metric as $ g_{\mu\nu}=\omega^2\tilde g_{\mu\nu}$, with $\omega$ a dilaton field which contains all the scale dependences. The "unphysical" metric $\tilde g_{\mu\nu}$ is related to the $(2+1)$-dimensional Kerr spacetime. The equation for the angular momentum $J$ decouples, for the vacuum situation as well as for global strings, from the other field equations and delivers a kind of spin-mass relation. For the most realistic solution, $J$ falls off as $\sim\frac{1}{r}$ and $\partial_r J \rightarrow 0$ close to the core. The spacetime is Ricci flat. The formation of closed timelike curves can be pushed to space infinity for suitable values of the parameters and the violation of the weak energy condition can be avoided. For the interior, a numerical solution is found. This solution can easily be matched at the boundary on the exterior exact solution by special choice of the parameters of the string. It turns out, as expected from the "holographic" principle, that the exact solution of the exterior is equivalent with the warped five-dimensional brane world model, with only a cosmological constant in the bulk. This example shows the power of conformal invariance to bridge the gap between general relativity and quantum field theory.