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Instantons and Wormholes In Minkowski and (A)dS Spaces

Michael Gutperle, Wafic Sabra

TL;DR

This work analyzes instanton and wormhole solutions in $d$-dimensional gravity coupled to an axion–dilaton system across $\Lambda=0,\pm$. By exploiting an $O(d)$-invariant ansatz and a key first-integral constraint, it derives the conditions under which non-singular solutions exist and identifies a critical dilaton coupling $|b|<b_c$ governing regular wormholes. Instantons are shown to exist in flat and AdS spaces but are precluded in dS due to dilaton singularities, while wormholes require careful balancing of $c$, $b$, and $\Lambda$ and exhibit topology changes via necks of finite size; AdS wormholes persist with regulated actions via boundary terms. The results have implications for non-perturbative effects in string theory and quantum gravity, including potential links to baby universes and holographic renormalization in AdS.

Abstract

Instanton and wormhole solutions are constructed in a d-dimensional gravity theory with an axion-dilaton pair of scalar fields. We discuss the cases of vanishing, positive and negative cosmological constant.

Instantons and Wormholes In Minkowski and (A)dS Spaces

TL;DR

This work analyzes instanton and wormhole solutions in -dimensional gravity coupled to an axion–dilaton system across . By exploiting an -invariant ansatz and a key first-integral constraint, it derives the conditions under which non-singular solutions exist and identifies a critical dilaton coupling governing regular wormholes. Instantons are shown to exist in flat and AdS spaces but are precluded in dS due to dilaton singularities, while wormholes require careful balancing of , , and and exhibit topology changes via necks of finite size; AdS wormholes persist with regulated actions via boundary terms. The results have implications for non-perturbative effects in string theory and quantum gravity, including potential links to baby universes and holographic renormalization in AdS.

Abstract

Instanton and wormhole solutions are constructed in a d-dimensional gravity theory with an axion-dilaton pair of scalar fields. We discuss the cases of vanishing, positive and negative cosmological constant.

Paper Structure

This paper contains 12 sections, 50 equations.