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

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. Abramowitz, Phys. Rev. D 102, 084044 (2020)1 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.

Automated summary

The study introduces reflection-asymmetric thin-shell wormholes with double shadows, composed of parts of Schwarzschild and Reissner-Nordstrom spacetimes with two photon spheres of different sizes. The researchers discussed the observational properties of these double shadows seen from an observer's perspective, emphasizing the presence of two photon rings with varying diameters.