1994/12/16 by R. J. Rivers, Rivers, R. J., T. S. Evans +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Force Microscopy Techniques and Applications #Magnetic properties of thin films #Theoretical and Computational Physics #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9412059
44 pages, LaTeX (figures included as LaTeX), available through anonymous ftp from ftp://euclid.tp.ph.ic.ac.uk/papers/94-5_06.tex or at http://euclid.tp.ph.ic.ac.uk/Papers/index.html
arxiv created 1994/12/16 · openalex publication_date 1994/12/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We shall show that the density of defects produced at a second-order phase transition is determined by the correlation length of the fields. This is true both for defects appearing in the Ginzburg regime and for defects produced at a quench, when the Ginzburg regime is irrelevant. (Invited lectures given by R.J.R. to the Nato Advanced Study Institute and Euroconference on Formation and Interaction of Topological Defects, Isaac Newton Institute, Cambridge (UK), September, 1994.)