Linearization stability of reflection-asymmetric thin-shell wormholes with double shadows

TL;DR

This paper investigates the stability of reflection-asymmetric thin-shell wormholes with double shadows, which are theoretical models featuring two photon spheres, to understand their potential physical viability.

Contribution

It provides a linearization stability analysis of a new class of reflection-asymmetric thin-shell wormholes with double shadows, extending previous models.

Findings

Demonstrates conditions for stability of these wormholes

Shows how double shadows relate to stability criteria

Provides insights into observational signatures of such wormholes

Abstract

Wormholes are hypothetical objects which can be black hole mimickers with strong gravitational fields. Recently, Wielgus et al. have constructed reflection-asymmetric thin-shell wormholes which are composed of the parts of a Schwarzschild spacetime and a Reissner-Nordstrom spacetime with two photon spheres with different sizes each other in [M. Wielgus, J. Horak, F. Vincent, and M. Abramowicz, Phys. Rev. D 102, 084044 (2020)]. They have discussed observational property of the shadows with two photon rings in different sizes as seen from an observer and they have named their shadows double shadows. In this paper, we study the linearization stability of the reflection-asymmetric thin-shell wormholes with the double shadows.