# Asymptotically flat wormhole solutions with variable equation-of-state   parameter

**Authors:** Foad Parsaei, Sara Rastgoo

arXiv: 1903.08251 · 2019-05-22

## TL;DR

This paper explores exact asymptotically flat wormhole solutions in general relativity with a variable equation-of-state parameter, analyzing energy condition violations and the role of exotic matter.

## Contribution

It introduces new wormhole solutions with a variable equation of state that are asymptotically flat and examines the energy conditions and matter content involved.

## Key findings

- Wormhole solutions with asymptotically flat geometry are found.
- NEC violation is analyzed and shown to be minimal.
- Solutions connect phantom and dark energy regimes near the throat.

## Abstract

In this paper, we study exact wormhole solutions in the framework of general relativity with a general equation of state that reduced to a linear equation of state asymptotically. By considering a special shape function, we find classes of solutions which are asymptotically flat. We study the violation of NEC as the main ingredient in the wormhole physics. We investigate the possibility of finding wormhole solutions with asymptotically different state parameter. We show that in principle, wormhole with vanishing redshift function and the selected shape function, cannot satisfy NEC at large infinity. We present solutions which have the positive total amount of mater in the "volume integral quantifier" method. For this class of solutions, fluid near the wormhole throat is in the phantom regime and at some $r=r_{2}$, the phantom regime is connected to a dark energy regime. Thus, we need small amount of exotic matter to construct wormhole solutions.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1903.08251/full.md

## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1903.08251/full.md

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Source: https://tomesphere.com/paper/1903.08251