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String windings in the early universe

Richard Easther1, Brian R Greene2,3, Mark G Jackson2,4 and Daniel Kabat2,5

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We study string dynamics in the early universe. Our motivation is the proposal of Brandenberger and Vafa that string winding modes may play a key role in decompactifying three spatial dimensions. We model the universe as a homogeneous but anisotropic nine-torus filled with a gas of excited strings. We adopt initial conditions which fix the dilaton and the volume of the torus, but otherwise assume all states are equally likely. We study the evolution of the system both analytically and numerically to determine the late-time behaviour. We find that, although dynamical evolution can indeed lead to three large spatial dimensions, such an outcome is not statistically favoured.


Keywords

extra dimensions

string theory and cosmology

 

E-print Number: hep-th/0409121

Cited: by |

Refers: to

PACS

11.27.+d Extended classical solutions; cosmic strings, domain walls, texture

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

98.80.Bp Origin and formation of the Universe

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 02 (February 2005)

Received 8 December 2004, accepted for publication 1 February 2005

Published 22 February 2005



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