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Main Authors: Li, Guo-He, Fang, Yeqi, Wu, Yuchi, Tao, Jun
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2506.09310
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author Li, Guo-He
Fang, Yeqi
Wu, Yuchi
Tao, Jun
author_facet Li, Guo-He
Fang, Yeqi
Wu, Yuchi
Tao, Jun
contents In this study, we investigate wormhole solutions within the framework of $F(R,T)$ gravity coupled to an axion-dilaton system and explore the inflation. Based on the Giddings-Strominger (GS) and expanding wormhole solutions in asymptotically flat Euclidean spacetime, the matter-geometry coupling term induces complex dynamical oscillations and reduces the Euclidean action, which enhances the nucleation probability of wormholes. Furthermore, we apply this theoretical setup to a "wineglass" half-wormhole model in Euclidean Anti-de Sitter (EAdS) spacetime and derive a constraint on the coupling parameter. This constraint introduces an unstable maximum in scalar potential, altering the probability distribution of initial states and the evolution of universes from high-potential regions. This method increases the probability of long-lasting inflation, offering a potential pathway to reconciling the no-boundary proposal with astronomical observations.
format Preprint
id arxiv_https___arxiv_org_abs_2506_09310
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Wormhole Solutions and Pre-inflationary Epoch in $F(R, T)$ Gravity with Axion Fields
Li, Guo-He
Fang, Yeqi
Wu, Yuchi
Tao, Jun
General Relativity and Quantum Cosmology
In this study, we investigate wormhole solutions within the framework of $F(R,T)$ gravity coupled to an axion-dilaton system and explore the inflation. Based on the Giddings-Strominger (GS) and expanding wormhole solutions in asymptotically flat Euclidean spacetime, the matter-geometry coupling term induces complex dynamical oscillations and reduces the Euclidean action, which enhances the nucleation probability of wormholes. Furthermore, we apply this theoretical setup to a "wineglass" half-wormhole model in Euclidean Anti-de Sitter (EAdS) spacetime and derive a constraint on the coupling parameter. This constraint introduces an unstable maximum in scalar potential, altering the probability distribution of initial states and the evolution of universes from high-potential regions. This method increases the probability of long-lasting inflation, offering a potential pathway to reconciling the no-boundary proposal with astronomical observations.
title Wormhole Solutions and Pre-inflationary Epoch in $F(R, T)$ Gravity with Axion Fields
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2506.09310