Instability of hyper-compact Kerr-like objects

TL;DR

This paper demonstrates that various horizonless, Kerr-like hyper-compact objects such as wormholes and superspinars are inherently unstable, reinforcing the likelihood that observed rapidly spinning compact objects are true black holes.

Contribution

The study extends instability analysis to a broad class of horizonless Kerr-like objects, including wormholes and superspinars, showing they are also unstable with short timescales.

Findings

Hyper-compact objects with Kerr-like geometry are unstable.

Instability timescales are very short.

Results support black holes as the likely nature of observed objects.

Abstract

Viable alternatives to astrophysical black holes include hyper-compact objects without horizon, such as gravastars, boson stars, wormholes and superspinars. The authors have recently shown that typical rapidly-spinning gravastars and boson stars develop a strong instability. That analysis is extended in this paper to a wide class of horizonless objects with approximate Kerr-like geometry. A detailed investigation of wormholes and superspinars is presented, using plausible models and mirror boundary conditions at the surface. Like gravastars and boson stars, these objects are unstable with very short instability timescales. This result strengthens previous conclusions that observed hyper-compact astrophysical objects with large rotation are likely to be black holes.