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Phys. Rev. Lett. 78, 2066–2069 (1997)

Nonintercommuting Cosmic Strings

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Luís M. A. Bettencourt1,2, Pablo Laguna3, and Richard A. Matzner4,5
1The Blackett Laboratory, Imperial College, London SW7 2BZ, United Kingdom
2Institut für Theoretische Physik, Universität Heidelberg, Philosophenweg 16, Heidelberg 69120, Germany
3Department of Astronomy & Astrophysics and Center for Gravitational Physics & Geometry, Penn State University, University Park, Pennsylvania 16802
4Center for Relativity, The University of Texas, Austin, Texas 78712
5Orson Anderson Scholar, Los Alamos National Laboratory, Los Alamos, New Mexico 87545

Received 12 December 1996; published in the issue dated 17 March 1997

We perform the numerical field evolution for the collision of two Abelian type I cosmic strings. We present evidence that, for collisions at small but characteristic relative velocities and angles, these cosmic strings do not exchange ends and separate. Rather, local higher winding number bound states are formed close to the collision point, which promote multiple local scatterings at right angles and prevent intercommutation from happening. This constitutes the simplest example of the breakdown of the intercommutation rule, usually assumed in the construction of effective models for cosmic string network evolution.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.78.2066
DOI:
10.1103/PhysRevLett.78.2066
PACS:
98.80.Cq, 11.27.+d