Loop corrections and graceful exit in string cosmology
Description
We examine the effect of perturbative string loops on the cosmological pre-big-bang evolution. We study loop corrections derived from heterotic string theory compactified on a ZN orbifold and we consider the effect of the all-order loop corrections to the Kaehler potential and of the corrections to gravitational couplings, including both threshold corrections and corrections due to the mixed Kaehler-gravitational anomaly. We find that string loops can drive the evolution into the region of the parameter space where a graceful exit is in principle possible, and we find solutions that, in the string frame, connect smoothly the superinflationary pre-big-bang evolution to a phase where the curvature and the derivative of the dilaton are decreasing. We also find that at a critical coupling the loop corrections to the Kaehler potential induce a ghost-like instability, i.e., the kinetic term of the dilaton vanishes. This is similar to what happens in Seiberg-Witten theory and signals the transition to a new regime where the light modes in the effective action are different and are related to the original ones by S-duality. In a string context, this means that we center a D-brane dominated phase
Additional details
Identifiers
- PII
- S0550321399002485;
Publishing Information
- Journal Title
- Nuclear Physics. B
- Journal Volume
- 552
- Journal Issue
- 1-2
- Journal Page Range
- p. 395-419
- ISSN
- 0550-3213
- CODEN
- NUPBBO
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 34082445
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COMPACTIFICATION; COSMOLOGICAL MODELS; GALACTIC EVOLUTION; PERTURBATION THEORY; RADIATIVE CORRECTIONS; STRING MODELS
- Descriptors DEC
- COMPOSITE MODELS; CORRECTIONS; EVOLUTION; EXTENDED PARTICLE MODEL; MATHEMATICAL MODELS; PARTICLE MODELS; QUARK MODEL
Optional Information
- Copyright
- Copyright (c) 1999 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.