Sharpening the Distance Conjecture in diverse dimensions

Abstract The Distance Conjecture holds that any infinite-distance limit in the scalar field moduli space of a consistent theory of quantum gravity must be accompanied by a tower of light particles whose masses scale exponentially with proper field distance ‖ϕ‖ as m ~ exp(−λ‖ϕ‖), where λ is order-one...

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Main Authors: Muldrow Etheredge, Ben Heidenreich, Sami Kaya, Yue Qiu, Tom Rudelius
Format: Article
Language:English
Published: SpringerOpen 2022-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2022)114
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author Muldrow Etheredge
Ben Heidenreich
Sami Kaya
Yue Qiu
Tom Rudelius
author_facet Muldrow Etheredge
Ben Heidenreich
Sami Kaya
Yue Qiu
Tom Rudelius
author_sort Muldrow Etheredge
collection DOAJ
description Abstract The Distance Conjecture holds that any infinite-distance limit in the scalar field moduli space of a consistent theory of quantum gravity must be accompanied by a tower of light particles whose masses scale exponentially with proper field distance ‖ϕ‖ as m ~ exp(−λ‖ϕ‖), where λ is order-one in Planck units. While the evidence for this conjecture is formidable, there is at present no consensus on which values of λ are allowed. In this paper, we propose a sharp lower bound for the lightest tower in a given infinite-distance limit in d dimensions: λ ≥ 1 / d − 2 $$ 1/\sqrt{d-2} $$ . In support of this proposal, we show that (1) it is exactly preserved under dimensional reduction, (2) it is saturated in many examples of string/M-theory compactifications, including maximal supergravity in d = 4 – 10 dimensions, and (3) it is saturated in many examples of minimal supergravity in d = 4 – 10 dimensions, assuming appropriate versions of the Weak Gravity Conjecture. We argue that towers with λ < 1 / d − 2 $$ 1/\sqrt{d-2} $$ discussed previously in the literature are always accompanied by even lighter towers with λ ≥ 1 / d − 2 $$ 1/\sqrt{d-2} $$ , thereby satisfying our proposed bound. We discuss connections with and implications for the Emergent String Conjecture, the Scalar Weak Gravity Conjecture, the Repulsive Force Conjecture, large-field inflation, and scalar field potentials in quantum gravity. In particular, we argue that if our proposed bound applies beyond massless moduli spaces to scalar fields with potentials, then accelerated cosmological expansion cannot occur in asymptotic regimes of scalar field space in quantum gravity.
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spelling doaj.art-9cc5b72d958441e38ed92e822c7b3d482023-03-26T11:04:16ZengSpringerOpenJournal of High Energy Physics1029-84792022-12-0120221217110.1007/JHEP12(2022)114Sharpening the Distance Conjecture in diverse dimensionsMuldrow Etheredge0Ben Heidenreich1Sami Kaya2Yue Qiu3Tom Rudelius4Department of Physics, University of MassachusettsDepartment of Physics, University of MassachusettsDepartment of Physics, University of MassachusettsDepartment of Physics, University of MassachusettsDepartment of Physics, University of CaliforniaAbstract The Distance Conjecture holds that any infinite-distance limit in the scalar field moduli space of a consistent theory of quantum gravity must be accompanied by a tower of light particles whose masses scale exponentially with proper field distance ‖ϕ‖ as m ~ exp(−λ‖ϕ‖), where λ is order-one in Planck units. While the evidence for this conjecture is formidable, there is at present no consensus on which values of λ are allowed. In this paper, we propose a sharp lower bound for the lightest tower in a given infinite-distance limit in d dimensions: λ ≥ 1 / d − 2 $$ 1/\sqrt{d-2} $$ . In support of this proposal, we show that (1) it is exactly preserved under dimensional reduction, (2) it is saturated in many examples of string/M-theory compactifications, including maximal supergravity in d = 4 – 10 dimensions, and (3) it is saturated in many examples of minimal supergravity in d = 4 – 10 dimensions, assuming appropriate versions of the Weak Gravity Conjecture. We argue that towers with λ < 1 / d − 2 $$ 1/\sqrt{d-2} $$ discussed previously in the literature are always accompanied by even lighter towers with λ ≥ 1 / d − 2 $$ 1/\sqrt{d-2} $$ , thereby satisfying our proposed bound. We discuss connections with and implications for the Emergent String Conjecture, the Scalar Weak Gravity Conjecture, the Repulsive Force Conjecture, large-field inflation, and scalar field potentials in quantum gravity. In particular, we argue that if our proposed bound applies beyond massless moduli spaces to scalar fields with potentials, then accelerated cosmological expansion cannot occur in asymptotic regimes of scalar field space in quantum gravity.https://doi.org/10.1007/JHEP12(2022)114D-BranesP-BranesString and Brane PhenomenologySuperstring Vacua
spellingShingle Muldrow Etheredge
Ben Heidenreich
Sami Kaya
Yue Qiu
Tom Rudelius
Sharpening the Distance Conjecture in diverse dimensions
Journal of High Energy Physics
D-Branes
P-Branes
String and Brane Phenomenology
Superstring Vacua
title Sharpening the Distance Conjecture in diverse dimensions
title_full Sharpening the Distance Conjecture in diverse dimensions
title_fullStr Sharpening the Distance Conjecture in diverse dimensions
title_full_unstemmed Sharpening the Distance Conjecture in diverse dimensions
title_short Sharpening the Distance Conjecture in diverse dimensions
title_sort sharpening the distance conjecture in diverse dimensions
topic D-Branes
P-Branes
String and Brane Phenomenology
Superstring Vacua
url https://doi.org/10.1007/JHEP12(2022)114
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AT tomrudelius sharpeningthedistanceconjectureindiversedimensions