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Phys. Rev. D 53, 4247–4256 (1996)

Tree-level string cosmology

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Richard Easther and Kei-ichi Maeda
Department of Physics, Waseda University, 3-4-1 Okubo, Shinjuku-ku, Tokyo, Japan

David Wands
Astronomy Centre, School of Mathematical and Physical Sciences, University of Sussex, Brighton BN1 9QH, United Kingdom

Received 14 September 1995; published in the issue dated 15 April 1996

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.

© 1996 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.53.4247
DOI:
10.1103/PhysRevD.53.4247
PACS:
98.80.Cq, 04.50.+h, 11.25.-w