Cosmology with twisted tori

We consider the cosmological role of the scalar fields generated by the compactification of 11-dimensional Einstein gravity on a 7D elliptic twisted torus, which has the attractive features of giving rise to a positive semi-definite potential, and partially fixing the moduli. This compactification i...

Full description

Bibliographic Details
Main Authors: Karthauser, Josef L.P., Saffin, P.M., Hindmarsh, Mark
Format: Article
Published: American Physical Society 2007
Online Access:https://eprints.nottingham.ac.uk/42118/
_version_ 1848796423267549184
author Karthauser, Josef L.P.
Saffin, P.M.
Hindmarsh, Mark
author_facet Karthauser, Josef L.P.
Saffin, P.M.
Hindmarsh, Mark
author_sort Karthauser, Josef L.P.
building Nottingham Research Data Repository
collection Online Access
description We consider the cosmological role of the scalar fields generated by the compactification of 11-dimensional Einstein gravity on a 7D elliptic twisted torus, which has the attractive features of giving rise to a positive semi-definite potential, and partially fixing the moduli. This compactification is therefore relevant for low energy M-theory, 11D supergravity. We find that slow-roll inflation with the moduli is not possible, but that there is a novel scaling solution in Friedmann cosmologies in which the massive moduli oscillate but maintain a constant energy density relative to the background barotropic fluid.
first_indexed 2025-11-14T19:47:45Z
format Article
id nottingham-42118
institution University of Nottingham Malaysia Campus
institution_category Local University
last_indexed 2025-11-14T19:47:45Z
publishDate 2007
publisher American Physical Society
recordtype eprints
repository_type Digital Repository
spelling nottingham-421182020-05-04T16:27:07Z https://eprints.nottingham.ac.uk/42118/ Cosmology with twisted tori Karthauser, Josef L.P. Saffin, P.M. Hindmarsh, Mark We consider the cosmological role of the scalar fields generated by the compactification of 11-dimensional Einstein gravity on a 7D elliptic twisted torus, which has the attractive features of giving rise to a positive semi-definite potential, and partially fixing the moduli. This compactification is therefore relevant for low energy M-theory, 11D supergravity. We find that slow-roll inflation with the moduli is not possible, but that there is a novel scaling solution in Friedmann cosmologies in which the massive moduli oscillate but maintain a constant energy density relative to the background barotropic fluid. American Physical Society 2007-11-27 Article PeerReviewed Karthauser, Josef L.P., Saffin, P.M. and Hindmarsh, Mark (2007) Cosmology with twisted tori. Physical Review Letters, 76 (10). p. 4039. ISSN 1079-7114 https://journals.aps.org/prd/abstract/10.1103/PhysRevD.76.104039 doi:10.1103/PhysRevD.76.104039 doi:10.1103/PhysRevD.76.104039
spellingShingle Karthauser, Josef L.P.
Saffin, P.M.
Hindmarsh, Mark
Cosmology with twisted tori
title Cosmology with twisted tori
title_full Cosmology with twisted tori
title_fullStr Cosmology with twisted tori
title_full_unstemmed Cosmology with twisted tori
title_short Cosmology with twisted tori
title_sort cosmology with twisted tori
url https://eprints.nottingham.ac.uk/42118/
https://eprints.nottingham.ac.uk/42118/
https://eprints.nottingham.ac.uk/42118/