corner
corner

Phys. Rev. D 58, 043503 (1998) [11 pages]

Symmetries for generating string cosmologies

Download: PDF (223 kB) Buy this article Export: BibTeX or EndNote (RIS)

E. J. Copeland
Centre for Theoretical Physics, University of Sussex, Brighton, BN1 9QH, United Kingdom

James E. Lidsey
Centre for Theoretical Physics, University of Sussex, Brighton, BN1 9QH, United Kingdom;
Astronomy Centre, University of Sussex, Brighton, BN1 9QH, United Kingdom;
Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield, Mile End Road, London, E1 4NS, United Kingdom

David Wands
School of Computer Science and Mathematics, University of Portsmouth, Portsmouth, PO1 2EG, United Kingdom

Received 17 February 1998; published 1 July 1998

We discuss the symmetry properties of the low-energy effective action of the type IIB superstring that may be employed to derive four-dimensional solutions. A truncated effective action, compactified on a six-torus, but including both Neveu-Schwarz–Neveu-Schwarz and Ramond-Ramond field strengths, can be expressed as a non-linear sigma model which is invariant under global SL(3,R) transformations. This group contains as a sub-group the SL(2,R) symmetry of the ten-dimensional theory and a discrete Z2 reflection symmetry which leads to a further SL(2,R) sub-group. The symmetries are employed to analyze a general class of spatially homogeneous cosmological solutions with non-trivial Ramond-Ramond fields.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.58.043503
DOI:
10.1103/PhysRevD.58.043503
PACS:
98.80.Cq, 04.50.+h, 11.25.-w