# Thermodynamic Stability of a Schwarzschild Thin-Shell Wormhole

**Authors:** S. Danial Forghani, S. Habib Mazharimousavi, and M. Halilsoy

arXiv: 1812.04340 · 2019-09-13

## TL;DR

This paper investigates the thermodynamic stability of Schwarzschild thin-shell wormholes, deriving entropy and heat capacity functions that confirm their stability and suggesting broader applicability of the method.

## Contribution

It introduces a method to analyze thermodynamic stability of thin-shell wormholes, deriving entropy and heat capacity functions, and demonstrates the stability of Schwarzschild thin-shell wormholes.

## Key findings

- Entropy function satisfies local stability conditions
- Heat capacity is well-defined and regular
- Schwarzschild thin-shell wormholes are thermodynamically stable

## Abstract

The thermodynamic stability of a thin-shell wormhole in a Schwarzschild bulk is considered. From the first law, entropy function is found which satisfies the local intrinsic stability conditions. Heat capacity emerges as a well-defined regular function justifying the stability of a Schwarzschild thin-shell wormhole. The scope of applications of the method is not limited by the Schwarzschild wormhole.

## Full text

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## References

30 references — full list in the complete paper: https://tomesphere.com/paper/1812.04340/full.md

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Source: https://tomesphere.com/paper/1812.04340