Multiple Rings in the Shadow of Extremely Compact Objects

TL;DR

This paper investigates how the images of horizon-less gravastars differ from black holes, revealing additional rings in their shadows that could help distinguish these objects observationally.

Contribution

It introduces a method to identify gravastars by analyzing extra rings in their shadow images, extending previous black hole imaging techniques.

Findings

Additional rings appear in gravastar images due to transmission and reflection effects.

A distinct ring caused by surface reflection can help constrain gravastar properties.

The approach links ring positions to light ray paths and disk emission models.

Abstract

The Event Horizon Telescope's image of the M87 black hole provides an exciting opportunity to study black hole physics. Since a black hole's event horizon absorbs all electromagnetic waves, it is difficult to actively probe the horizon's existence. However, with the help of a family of extremely compact, horizon-less objects, named gravastars", whose external space-times nearly identical to those of black holes, one can test the absence of event horizons: absences of additional features that arise due to the existence of the gravastar, or its surface, can be used as quantitative evidence for black holes. We apply Gralla et al.'s approach to studying black hole images to study the images of two types of gravastars: transparent ones and reflective ones. In both cases, the transmission of rays through gravastars, or their reflections on their surfaces, lead to more rings in their images. For simple emission models, where the redshifted emissivity of the disk is peaked at a particular radius r-peak, the position of a series of rings can be related in a simple manner to light ray propagation: a ring shows up around impact parameter b whenever rays incident from infinity at b intersects the disk at r-peak. We show that additional rings will appear in the images of transparent and reflective gravastars. In particular, one of the additional rings for the reflective gravastar is due to the prompt reflection of light on the gravastar surface and appears to be well separated from the others. This can be a robust feature, which may be reliably used to constrain the reflectivity of the black hole's horizon.