Richard Easther et al JCAP02(2005)009 doi:10.1088/1475-7516/2005/02/009
Richard Easther1, Brian R Greene2,3, Mark G Jackson2,4 and Daniel Kabat2,5
Show affiliationsWe 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.
E-print Number: hep-th/0409121
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Refers: to
11.27.+d Extended classical solutions; cosmic strings, domain walls, texture
Issue 02 (February 2005)
Received 8 December 2004, accepted for publication 1 February 2005
Published 22 February 2005
Richard Easther et al JCAP02(2005)009
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