Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology

The euclidean path integral remains, in spite of its familiar problems, an important approach to quantum gravity. One of its most striking and obscure features is the appearance of gravitational instantons or wormholes. These renormalize all terms in the Lagrangian and cause a number of puzzles or e...

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Main Authors: Arthur Hebecker, Thomas Mikhail, Pablo Soler
Format: Article
Language:English
Published: Frontiers Media S.A. 2018-10-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/article/10.3389/fspas.2018.00035/full
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spelling doaj-9ef8b7340b2a4e69b78570d03bd87c9b2020-11-24T22:22:36ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2018-10-01510.3389/fspas.2018.00035411231Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and CosmologyArthur HebeckerThomas MikhailPablo SolerThe euclidean path integral remains, in spite of its familiar problems, an important approach to quantum gravity. One of its most striking and obscure features is the appearance of gravitational instantons or wormholes. These renormalize all terms in the Lagrangian and cause a number of puzzles or even deep inconsistencies, related to the possibility of nucleation of “baby universes.” In this review, we revisit the early controversies surrounding these issues as well as some of the more recent discussions of the phenomenological relevance of gravitational instantons. In particular, wormholes are expected to break the shift symmetries of axions or Goldstone bosons non-perturbatively. This can be relevant to large-field inflation and connects to arguments made on the basis of the Weak Gravity or Swampland conjectures. It can also affect Goldstone bosons which are of physical interest in the context of the strong CP problem or as dark matter.https://www.frontiersin.org/article/10.3389/fspas.2018.00035/fullstring theoryquantum gravityeuclidean wormholeaxionsparticle physics -cosmology connectioninflation
collection DOAJ
language English
format Article
sources DOAJ
author Arthur Hebecker
Thomas Mikhail
Pablo Soler
spellingShingle Arthur Hebecker
Thomas Mikhail
Pablo Soler
Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology
Frontiers in Astronomy and Space Sciences
string theory
quantum gravity
euclidean wormhole
axions
particle physics -cosmology connection
inflation
author_facet Arthur Hebecker
Thomas Mikhail
Pablo Soler
author_sort Arthur Hebecker
title Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology
title_short Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology
title_full Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology
title_fullStr Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology
title_full_unstemmed Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology
title_sort euclidean wormholes, baby universes, and their impact on particle physics and cosmology
publisher Frontiers Media S.A.
series Frontiers in Astronomy and Space Sciences
issn 2296-987X
publishDate 2018-10-01
description The euclidean path integral remains, in spite of its familiar problems, an important approach to quantum gravity. One of its most striking and obscure features is the appearance of gravitational instantons or wormholes. These renormalize all terms in the Lagrangian and cause a number of puzzles or even deep inconsistencies, related to the possibility of nucleation of “baby universes.” In this review, we revisit the early controversies surrounding these issues as well as some of the more recent discussions of the phenomenological relevance of gravitational instantons. In particular, wormholes are expected to break the shift symmetries of axions or Goldstone bosons non-perturbatively. This can be relevant to large-field inflation and connects to arguments made on the basis of the Weak Gravity or Swampland conjectures. It can also affect Goldstone bosons which are of physical interest in the context of the strong CP problem or as dark matter.
topic string theory
quantum gravity
euclidean wormhole
axions
particle physics -cosmology connection
inflation
url https://www.frontiersin.org/article/10.3389/fspas.2018.00035/full
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