Evolving Wormholes in a Cosmological Background

TL;DR

This paper reviews evolving wormhole solutions within cosmological backgrounds, highlighting how they can be constructed in general relativity and modified gravity theories without violating energy conditions.

Contribution

It systematically surveys time-dependent wormhole models in cosmological settings, emphasizing conditions for their viability in both Einstein and alternative gravity frameworks.

Findings

Wormholes can be embedded in FLRW and de Sitter universes.

Modified gravity theories support traversable wormholes without exotic matter.

Conditions for wormhole evolution consistent with energy constraints are identified.

Abstract

Wormholes are non-trivial topological structures that arise as exact solutions to Einstein's field equations, theoretically connecting distinct regions of spacetime via a throat-like geometry. While static traversable wormholes necessarily require exotic matter that violates the classical energy conditions, subsequent studies have sought to minimize such violations by introducing time-dependent geometries embedded within cosmological backgrounds. This review provides a comprehensive survey of evolving wormhole solutions, emphasizing their formulation within both general relativity and alternative theories of gravity. We explore key developments in the construction of non-static wormhole spacetimes, including those conformally related to static solutions, as well as dynamically evolving geometries influenced by scalar fields. Particular attention is given to the wormholes embedded into Friedmann-Lema\^itre-Robertson-Walker (FLRW) universes and de Sitter backgrounds, where the interplay between the cosmic expansion and wormhole dynamics is analyzed. We also examine the role of modified gravity theories, especially in hybrid metric-Palatini gravity, which enable the realization of traversable wormholes supported by effective stress-energy tensors that do not violate the null or weak energy conditions. By systematically analyzing a wide range of time-dependent wormhole solutions, this review identifies the specific geometric and physical conditions under which wormholes can evolve consistently with the null and weak energy conditions. These findings clarify how such configurations can be naturally integrated into cosmological models governed by general relativity or modified gravity, thereby contributing to a deeper theoretical understanding of localized spacetime structures in an expanding universe.