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A note on the evolution of cosmic string/superstring networks

M Sakellariadou

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In the context of the brane world scenario, cosmic superstrings can be formed in D-brane annihilation at the end of the brane inflationary era. The cosmic superstring network has a scaling solution and the characteristic scale of the network is proportional to the square root of the reconnection probability.


Keywords

cosmology with extra dimensions

string theory and cosmology

physics of the early universe

 

E-print Number: hep-th/0410234

Cited: by |

Refers: to

PACS

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

11.25.Uv D branes

11.25.Wx String and brane phenomenology

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

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 04 (April 2005)

Received 2 November 2004, accepted for publication 31 March 2005

Published 6 April 2005



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