Answers are grounded in this paper and cite their sources.
We study the effects of friction on the scaling evolution of string networks in condensed matter and cosmological contexts. We derive a generalized ``one-scale'' model with the string correlation length L and velocity v as dynamical variables. In nonrelativistic systems, we obtain a well-known L{∝}t1/2 law, showing that loop production is important. For electroweak cosmic strings, we show transient damped epoch scaling with L{∝}t5/4 (or, in the matter era, L{∝}t3/2). A low initial density implies an earlier period with L{∝}t1/2. For GUT strings, the approach to linear scaling L{∝}t is faster than previously estimated. {} 1996 The American Physical Society.
No takes yet. Share an insight, caveat, or question.
Martins et al. (1996) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: