Superheavy superconducting cosmic strings from superstring models

Details Superheavy superconducting cosmic strings from superstring models Superheavy superconducting cosmic strings from superstring models

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phlb..183..289l&link_type=abstract

Physics Letters B, Volume 183, Issue 3-4, p. 289-295.

Physics

24

Scientific paper

We discuss how cosmic strings relevant for galaxy formation can appear in certain gauge models inspired by the ten dimensional E8 × E8 superstring theory. Despite their superheavy (~ 1015-1016 GeV) mass scale these strings, which also happen to be superconducting, are produced only when the temperature of the universe approaches the TeV scale. An inflationary scanario can therefore precede the phase transition which gives rise to the cosmic strins. The generation of the baryon asymmetry in the presence of such high scales is also discussed.
Supported in part by the Department of Energy under Contract Number DE-AC02-78ER05007.

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