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High Energy Physics - Phenomenology

Title: Cosmic Strings - Dead Again?

Authors: Mark Hindmarsh (Sussex)
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 $\xi$ increases linearly with time. There are very few loops with sizes less than $\xi$, 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 $\mu$: we estimate $G\mu < 10^{-9}$, three orders of magnitude lower than the constraint from Cosmic Microwave Background fluctuations.
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
Subjects: High Energy Physics - Phenomenology (hep-ph); Astrophysics (astro-ph)
Report number: SUSX-TH-98-016
Cite as: arXiv:hep-ph/9806469
  (or arXiv:hep-ph/9806469v1 for this version)

Submission history

From: Mark Hindmarsh [view email]
[v1] Wed, 24 Jun 1998 16:39:24 GMT (8kb)