Hyperbolic compactification of M-theory and de Sitter quantum gravity
Open accessAbstract
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 for a range of parameters. 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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Almost all studies of Casimir energy in Kaluza-Klein and string-theoretic contexts assume the size of extra dimensions is time-independent, primarily to identify static stable vacua.
“Almost all of these studies assume that the size of the extra dimensions is time-independent, primarily because their objective is to identify static stable vacua.”
From Stress-energy tensor of a scalar field on a product spacetime with a time-dependent compact dimension (2026) · cites this paper as [10]
Sections 2 and 4 describe this paper’s use of Casimir energy to stabilize an internal volume, but they do not assess how often other Kaluza–Klein or string-theoretic studies assume time-independent extra dimensions or why they do so. Searches for static vacua and time-dependent extra dimensions found no passage addressing that broader claim. The indexed passages provide no page numbers. (LLM, conf=0.72)
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Entanglement wedge reconstruction and the information paradox
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“The structure of de Sitter in string theory is also relevant for other related approaches such as [121–123] and [124,125].”
BackgroundThe trouble with de Sitter space
Goheer, N., Kleban, M., & Susskind, L. (2003) · Journal of High Energy Physics · doi:10.1088/1126-6708/2003/07/056 · Cited by 281 · see citing works
ANNINOS, D. (2012) · International Journal of Modern Physics A · doi:10.1142/s0217751x1230013x · Cited by 174 · see citing works
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Asymptotic Safety: Swampland or Wonderland?
Basile, I., & Platania, A. (2021) · Universe · doi:10.3390/universe7100389 · Cited by 39 · see citing works
Paul, A., & Paban, S. (2026) · Journal of High Energy Physics · doi:10.1007/jhep09(2026)188
- Authors
- De Luca, G. B., Silverstein, E., & Torroba, G.
- Affiliations
- Stanford University
- Stanford University (US)
- Bariloche Atomic Centre (AR)
- Venue
- SciPost Physics
- Publisher
- Stichting SciPost
- Published
- 2022-03-04
- Volume
- 12
- Issue
- 3
- ISSN
- 2542-4653 (ISSN-L)
- OpenAlex
- W3158607831
- Cited by
- 39
- References
- 4
- Citations by year
- 2026: 8 · 2025: 5 · 2024: 9 · 2023: 13 · 2022: 3 · 2021: 1
- FWCI
- 0.94
- Type
- journal article
- Language
- en
- Open access
- diamond
- doi.org
- Locations
- SciPost Physics (publishedVersion, cc-by)
- arXiv (Cornell University) (submittedVersion)
- BOA (University of Milano-Bicocca) (submittedVersion, cc-by)
- DOAJ (DOAJ: Directory of Open Access Journals) (submittedVersion, cc-by-sa)
- arXiv (Cornell University)
- Greater South Information System
- Funders
- Agencia Nacional de Promoción Científica y Tecnológica (PICT 2018-2517)
- Comisión Nacional de Energía Atómica, Gobierno de Argentina
- Consejo Nacional de Investigaciones Científicas y Técnicas (11220150100299)
- National Science Foundation (PHY-1720397)
- Simons Foundation
- Universidad Nacional de Cuyo
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Keywords
- M-theory compactification, hyperbolic manifolds, de Sitter space, cosmic acceleration, Casimir energy, Dehn filling, warped product metrics, axion monodromy inflation, de Sitter holography, M2-branes, negative curvature, tadpoles
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