Evolution of cosmic string networks

Details Evolution of cosmic string networks Evolution of cosmic string networks

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ecsn.reptr....a&link_type=abstract

Unknown

Physics

Condensed Matter

Statistical Mechanics

Astronomical Models, Cosmology, Statistical Mechanics, String Theory, Computerized Simulation, Galactic Evolution, Random Walk, Stellar Gravitation

Scientific paper

Results on cosmic strings are summarized including: (1) the application of non-equilibrium statistical mechanics to cosmic string evolution; (2) a simple one scale model for the long strings which has a great deal of predictive power; (3) results from large scale numerical simulations; and (4) a discussion of the observational consequences of our results. An upper bound on G mu of approximately 10(-7) emerges from the millisecond pulsar gravity wave bound. How numerical uncertainties affect this are discussed. Any changes which weaken the bound would probably also give the long strings the dominant role in producing observational consequences.

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