Published July 12, 1999 | Version v1
Journal article

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.