Wiggly Cosmic Strings

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

1 DAMTP, U. Cambridge, Silver St., Cambridge CB3 9EW, U.K.
2 CAUP, R. do Campo Alegre 823, 4150 Porto, Portugal


Almost all analytic studies of cosmic strings so far were concerned with the simplest, Goto-Nambu strings. However, it is abundantly clear that in order to describe more realistic cosmic string networks, and in particular phenomena such as small-scale structure and charge and current build-up on strings, one must include additional degrees of freedom along the strings. These are generically called `elastic' string models.

In this talk, a generalised analytic string evolution model, based on Carter's transonic elastic model, will be presented. This explicitly includes the effects of small-scale structure, through an evolution equation for the `renormalised' string mass per unit length. The evolution of string networks in the context of this model will be discussed, and some of its consequences will explored.


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