Superfluid-like turbulence in cosmology

Details Superfluid-like turbulence in cosmology Superfluid-like turbulence in cosmology

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991stin...9211942g&link_type=abstract

Presented at the Sixth Marcel Grossmann Meeting on General Relativity, Kyoto, Japan, 24-29 Jun. 1991

Mathematics

Logic

Baryons, Cosmology, Dark Matter, Particle Motion, String Theory, Superfluidity, Turbulence, Vortices, Angular Momentum, Flow Velocity, Quadrupoles, Universe

Scientific paper

A network of vortices in a superfluid system exhibits turbulent behavior. It is argued that the universe may have experienced such a phase of superfluid-like turbulence due to the existence of a coherent state with non-topological charge and a network of global strings. The unique feature of a distribution of turbulent domains is that it can yield non-gravitationally induced large-scale coherent velocities. It may be difficult, however, to relate these velocities to the observed large-scale bulk motion.

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