Evolution and radiation from superconducting cosmic strings

Details Evolution and radiation from superconducting cosmic strings Evolution and radiation from superconducting cosmic strings

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nuphb.323...95b&link_type=abstract

Nuclear Physics B, Volume 323, Issue 1, p. 95-112.

Physics

Nuclear Physics

18

Scientific paper

We study the evolution of cosmic superconducting strings and their decay. We show that they pass by three stages. The last one produces high-energy particles. The size of the loop at this stage is less than 30 pc. If particles can leave the string, and μ22 is the linear density necessary to explain galaxy formation, the strings are shown to produce isotropic γ radiation in excess of present bounds. However, we show that the produced particles degrade drastically in energy in the magnetic field of the string so that high-energy particles are not produced.

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