Texture: A cosmological topological defect

Details Texture: A cosmological topological defect Texture: A cosmological topological defect

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvd..35.3705d&link_type=abstract

Physical Review D (Particles and Fields), Volume 35, Issue 12, 15 June 1987, pp.3705-3708

Mathematics

Logic

85

Origin And Formation Of The Universe, Fundamental Problems And General Formalism

Scientific paper

The notions of phase transition and causality, combined with the standard cosmological model, lead to the appearance of topological defects in the early Universe. The most familiar types of defects are solitons, strings, and domain walls. Another type-textures-can exist when the spatial universe is compact. When these appear the whole Universe takes on a winding number, and the consequences are quite amusing.

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