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Cosmic acceleration from M theory on twisted spaces

2005/04/30 by Ishwaree P. Neupane, David L. Wiltshire · 59 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Compactification (mathematics) #Conformal map #Cosmology and Gravitation Theories #Einstein #Geometry #Mathematical analysis #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Product (mathematics) #Pure mathematics #Scalar (mathematics) #Supergravity #Supersymmetry #Theoretical physics #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.72.083509

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 72(8) (American Physical Society) · 23 pages, 3 figures; added a summary Table, PRD version

openalex publication_date 2005/10/14 · arxiv created 2005/10/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

In a recent paper [I. P. Neupane and D. L. Wiltshire, Phys. Lett. B 619, 201 (2005).] we have found a new class of accelerating cosmologies arising from a time-dependent compactification of classical supergravity on product spaces that include one or more geometric twists along with nontrivial curved internal spaces. With such effects, a scalar potential can have a local minimum with positive vacuum energy. The existence of such a minimum generically predicts a period of accelerated expansion in the four-dimensional Einstein conformal frame. Here we extend our knowledge of these cosmological solutions by presenting new examples and discuss the properties of the solutions in a more general setting. We also relate the known (asymptotic) solutions for multiscalar fields with exponential potentials to the accelerating solutions arising from simple (or twisted) product spaces for internal manifolds.

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