# Thin-shell wormholes from Kiselev black holes

## TL;DR

This paper explores the theoretical creation of thin-shell wormholes from Kiselev black holes, analyzing their stability and conditions for potential stability despite typical instability issues.

## Contribution

It introduces a method to construct thin-shell wormholes from Kiselev black holes and identifies conditions under which these wormholes can be stable.

## Key findings

- Most wormholes are unstable to radial perturbations
- A limit argument shows stable solutions are possible under certain conditions
- The study advances understanding of wormhole stability in black hole spacetimes

## Abstract

This paper discusses the theoretical construction of thin-shell wormholes from Kiselev black holes. We assume a barotropic equation of state for the exotic matter on the shell. While most of these wormholes are unstable to linearized radial perturbations, a limit argument is used to show that under certain conditions, stable solutions can be found.