Cosmic Strings - Dead Again?
Abstract
I report on recent numerical simulations of the simplest field theory with cosmic string solutions, the Abelian Higgs model. We find that random networks of string quickly converge to a scaling solution in which the network scale length increases linearly with time. There are very few loops with sizes less than , and the strings are smooth, showing no signs of ``small scale structure''. We claim that particle production is the dominant energy-loss mechanism, not gravitational radiation as previously thought. For strings in Grand Unified Models, stringent constraints can be placed from cosmic ray observations on the string tension : we estimate , three orders of magnitude lower than the constraint from Cosmic Microwave Background fluctuations.
Cite
@article{arxiv.hep-ph/9806469,
title = {Cosmic Strings - Dead Again?},
author = {Mark Hindmarsh},
journal= {arXiv preprint arXiv:hep-ph/9806469},
year = {2016}
}
Comments
Late appearance of talk given at Cosmo 97, Ambleside, England, Sept 97, based on hep-ph/9708427 (error concerning UHE cosmic ray bounds addressed). 4pp, 1eps fig, LaTeX2e