Tree-level string cosmology
- 15 April 1996
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 53 (8) , 4247-4256
- https://doi.org/10.1103/physrevd.53.4247
Abstract
In this paper we examine the classical evolution of a cosmological model derived from the low-energy tree-level limit of a generic string theory. The action contains the metric, dilaton, central charge and an antisymmetric tensor field. We show that with a homogeneous and isotropic metric, allowing spatial curvature, there is a formal equivalence between this system and a scalar field minimally coupled to Einstein gravity in a spatially flat metric. We refer to this system as the shifted frame and using it we describe the full range of cosmological evolution that this model can exhibit. We show that generic solutions begin (or end) with a singularity. As the system approaches a singularity the dilaton becomes large and loop corrections will become important. © 1996 The American Physical Society.Keywords
All Related Versions
This publication has 32 references indexed in Scilit:
- Comments on cosmological string solutionsPhysics Letters B, 1991
- Rolling radii and a time-dependent dilationNuclear Physics B, 1990
- An expanding universe in string theoryNuclear Physics B, 1989
- Early cosmology and the dilaton and H field of superstring theoryNuclear Physics B, 1989
- Cosmological string theories and discrete inflationPhysics Letters B, 1988
- Attractor in a superstring model: The Einstein theory, the Friedmann universe, and inflationPhysical Review D, 1987
- Stability of string vacuaNuclear Physics B, 1986
- Strings in background fieldsNuclear Physics B, 1985
- Cosmological instability in ten-dimensional supergravityPhysics Letters B, 1985
- Effective field theory from quantized stringsPhysics Letters B, 1985