pith. sign in

arxiv: astro-ph/9910354 · v1 · submitted 1999-10-19 · 🌌 astro-ph · gr-qc· hep-ph

Radiation from cosmic string standing waves

classification 🌌 astro-ph gr-qchep-ph
keywords stringcosmicradiationfallsfieldratestandingthose
0
0 comments X
read the original abstract

We have simulated large-amplitude standing waves on an Abelian-Higgs cosmic string in classical lattice field theory. The radiation rate falls exponentially with wavelength, as one would expect from the field profile around a gauge string. Our results agree with those of Shellard and Moore, but not those of Vincent, Antunes, and Hindmarsh. The radiation rate falls too rapidly to sustain a scaling solution via direct radiation of particles from string length. There is thus reason to doubt claims of strong constraints on cosmic string theories from cosmic ray observations.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.