Physics
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..54.2163m&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 54, May 13, 1985, p. 2163-2165.
Physics
37
Cosmology, Einstein Equations, Expansion, Universe, Equations Of Motion, Fourier Transformation, Nonlinear Equations, Thermodynamic Equilibrium
Scientific paper
The time evolution of the N-vector model coupled to the Einstein field equation in a Robertson-Walker metric is studied numerically under the assumption of initial equilibrium at high temperatures and in the limit as N tends to infinity. The system shows inflationary expansion of the Robertson-Walker scale factor, alpha(t), over many e-foldings as well as local ordering. The associated structure factor develops a Bragg peak near zero wave number which has the proper weight for a spontaneously broken symmetry and has a width (inversely proportional to a characteristic domain size) which is inversely proportional to alpha(t).
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