Hyperbolic compactification of M-theory and de Sitter quantum gravity

We present a mechanism for accelerated expansion of the universe in the generic case of negative-curvature compactifications of M-theory, with minimal ingredients. M-theory on a hyperbolic manifold with small closed geodesics supporting Casimir energy -- along with a single classical source (7-fo...

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Main Author: G. Bruno De Luca, Eva Silverstein, Gonzalo Torroba
Format: Article
Language:English
Published: SciPost 2022-03-01
Series:SciPost Physics
Online Access:https://scipost.org/SciPostPhys.12.3.083
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author G. Bruno De Luca, Eva Silverstein, Gonzalo Torroba
author_facet G. Bruno De Luca, Eva Silverstein, Gonzalo Torroba
author_sort G. Bruno De Luca, Eva Silverstein, Gonzalo Torroba
collection DOAJ
description We present a mechanism for accelerated expansion of the universe in the generic case of negative-curvature compactifications of M-theory, with minimal ingredients. M-theory on a hyperbolic manifold with small closed geodesics supporting Casimir energy -- along with a single classical source (7-form flux) -- contains an immediate 3-term structure for volume stabilization at positive potential energy. Hyperbolic manifolds are well-studied mathematically, with an important rigidity property at fixed volume. They and their Dehn fillings to more general Einstein spaces exhibit explicit discrete parameters that yield small closed geodesics supporting Casimir energy. The off-shell effective potential derived by M. Douglas incorporates the warped product structure via the constraints of general relativity, screening negative energy. Analyzing the fields sourced by the localized Casimir energy and the available discrete choices of manifolds and fluxes, we find a regime where the net curvature, Casimir energy, and flux compete at large radius and stabilize the volume. Further metric and form field deformations are highly constrained by hyperbolic rigidity and warping effects, leading to calculations giving strong indications of a positive Hessian, and residual tadpoles are small. We test this via explicit back reacted solutions and perturbations in patches including the Dehn filling regions, initiate a neural network study of further aspects of the internal fields, and derive a Maldacena-Nunez style no-go theorem for Anti-de Sitter extrema. A simple generalization incorporating 4-form flux produces axion monodromy inflation. As a relatively simple de Sitter uplift of the large-N M2-brane theory, the construction applies to de Sitter holography as well as to cosmological modeling, and introduces new connections between mathematics and the physics of string/M theory compactifications.
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spelling doaj.art-3d9ef25ab22c459cb07e5f8ffd7765b42022-12-21T20:03:20ZengSciPostSciPost Physics2542-46532022-03-0112308310.21468/SciPostPhys.12.3.083Hyperbolic compactification of M-theory and de Sitter quantum gravityG. Bruno De Luca, Eva Silverstein, Gonzalo TorrobaWe present a mechanism for accelerated expansion of the universe in the generic case of negative-curvature compactifications of M-theory, with minimal ingredients. M-theory on a hyperbolic manifold with small closed geodesics supporting Casimir energy -- along with a single classical source (7-form flux) -- contains an immediate 3-term structure for volume stabilization at positive potential energy. Hyperbolic manifolds are well-studied mathematically, with an important rigidity property at fixed volume. They and their Dehn fillings to more general Einstein spaces exhibit explicit discrete parameters that yield small closed geodesics supporting Casimir energy. The off-shell effective potential derived by M. Douglas incorporates the warped product structure via the constraints of general relativity, screening negative energy. Analyzing the fields sourced by the localized Casimir energy and the available discrete choices of manifolds and fluxes, we find a regime where the net curvature, Casimir energy, and flux compete at large radius and stabilize the volume. Further metric and form field deformations are highly constrained by hyperbolic rigidity and warping effects, leading to calculations giving strong indications of a positive Hessian, and residual tadpoles are small. We test this via explicit back reacted solutions and perturbations in patches including the Dehn filling regions, initiate a neural network study of further aspects of the internal fields, and derive a Maldacena-Nunez style no-go theorem for Anti-de Sitter extrema. A simple generalization incorporating 4-form flux produces axion monodromy inflation. As a relatively simple de Sitter uplift of the large-N M2-brane theory, the construction applies to de Sitter holography as well as to cosmological modeling, and introduces new connections between mathematics and the physics of string/M theory compactifications.https://scipost.org/SciPostPhys.12.3.083
spellingShingle G. Bruno De Luca, Eva Silverstein, Gonzalo Torroba
Hyperbolic compactification of M-theory and de Sitter quantum gravity
SciPost Physics
title Hyperbolic compactification of M-theory and de Sitter quantum gravity
title_full Hyperbolic compactification of M-theory and de Sitter quantum gravity
title_fullStr Hyperbolic compactification of M-theory and de Sitter quantum gravity
title_full_unstemmed Hyperbolic compactification of M-theory and de Sitter quantum gravity
title_short Hyperbolic compactification of M-theory and de Sitter quantum gravity
title_sort hyperbolic compactification of m theory and de sitter quantum gravity
url https://scipost.org/SciPostPhys.12.3.083
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