Published October 25, 2010 | Version v1
Journal article

On climbing scalars in String Theory

  • 1. LPT, Bat. 210, Univ. Paris-Sud, F-91405 Orsay (France)
  • 2. Centre de Physique Theorique, Ecole Polytechnique, CNRS, F-91128 Palaiseau (France)
  • 3. Department of Physics, Tokyo Metropolitan University, Hachioji, Tokyo, 192-0397 (Japan)
  • 4. Scuola Normale Superiore and INFN, Piazza dei Cavalieri, 7, I-56126 Pisa (Italy)

Description

In string models with 'brane supersymmetry breaking' exponential potentials emerge at (closed-string) tree level but are not accompanied by tachyons. Potentials of this type have long been a source of embarrassment in flat space, but can have interesting implications for Cosmology. For instance, in ten dimensions the logarithmic slope |V'/V| lies precisely at a 'critical' value where the Lucchin-Matarrese attractor disappears while the scalar field is forced to climb up the potential when it emerges from the Big Bang. This type of behavior is in principle perturbative in the string coupling, persists after compactification, could have trapped scalar fields inside potential wells as a result of the cosmological evolution and could have also injected the inflationary phase of our Universe.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2010.09.040

Additional details

Identifiers

DOI
10.1016/j.physletb.2010.09.040;
arXiv
arXiv:1009.0874v1;
PII
S0370-2693(10)01128-7;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
694
Journal Issue
1
Journal Page Range
p. 80-88
ISSN
0370-2693
CODEN
PYLBAJ

Optional Information

Copyright
Copyright (c) 2010 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.