Fractal properties and small-scale structure of cosmic string networks

C. J. A. P. Martins and E. P. S. Shellard
Phys. Rev. D 73, 043515 – Published 22 February 2006

Abstract

We present results from a detailed numerical study of the small-scale and loop production properties of cosmic string networks, based on the largest and highest resolution string simulations to date. We investigate the nontrivial fractal properties of cosmic strings, in particular, the fractal dimension and renormalized string mass per unit length, and we also study velocity correlations. We demonstrate important differences between string networks in flat (Minkowski) spacetime and the two very similar expanding cases. For high resolution matter era network simulations, we provide strong evidence that small-scale structure has converged to “scaling” on all dynamical length scales, without the need for other radiative damping mechanisms. We also discuss preliminary evidence that the dominant loop production size is also approaching scaling.

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  • Received 7 December 2005

DOI:https://doi.org/10.1103/PhysRevD.73.043515

©2006 American Physical Society

Authors & Affiliations

C. J. A. P. Martins1,2,* and E. P. S. Shellard2,†

  • 1Centro de Física do Porto, Rua do Campo Alegre 687, 4169-007, Porto, Portugal
  • 2Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, United Kingdom

  • *Electronic address: C.J.A.P.Martins@damtp.cam.ac.uk
  • Electronic address: E.P.S.Shellard@damtp.cam.ac.uk

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Issue

Vol. 73, Iss. 4 — 15 February 2006

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