C. J. A. P. Martins, with E. P. S. Shellard, extended the velocity-dependent one-scale model of cosmic string networks. Their 2002 paper refined the curvature-related momentum parameter and incorporated radiation backreaction to study scaling solutions under different expansion histories.[ref]
A scaling state maintains fixed dimensionless ratios between the network's characteristic length and cosmological scales. It is a dynamical outcome of expansion, string motion and losses, rather than a consequence of dimensional analysis alone.
Articles by others on the same topic
There are currently no matching articles.