# Rotating wormhole solutions with a complex phantom scalar field

## TL;DR

This paper presents new rotating wormhole solutions supported by a complex phantom scalar field with self-interaction, demonstrating regular, asymptotically flat spacetimes and including static, non-spherically symmetric cases.

## Contribution

It introduces rotating wormhole solutions with a complex phantom scalar field and self-interaction, expanding the class of known wormhole geometries.

## Key findings

- Solutions are regular and asymptotically flat.
- A subset describes static, non-spherically symmetric wormholes.

## Abstract

We consider rotating wormhole solutions supported by a complex phantom scalar field with a quartic self-interaction, where the phantom field induces the rotation of the spacetime. The solutions are regular and asymptotically flat. A subset of solutions describing static but not spherically symmetric wormholes is also obtained.