Renormalized analytic solution for the enstrophy cascade in two-dimensional quantum turbulence<sup>-3</sup>
ORAL
Abstract
The forward enstrophy cascade in two-dimensional quantum turbulence in a superfluid film connected to a thermal bath is investigated using a Fokker-Planck equation based on Kosterlitz-Thouless renormalization. The steady-state cascade is formed by injecting vortex pairs of large initial separation at a constant rate. They diffuse with a constant flux to smaller scales, finally annihilating when reaching the core size. The energy spectrum varies as k-3, similar to the spectrum known for 2D classical-fluid enstrophy cascades. The dynamics of the cascade can also be studied, and for the case of a sharply peaked initial vortex-pair distribution, it takes about four eddy turnover times for the system to evolve to the decaying k-3 cascade, in agreement with recent computer simulations. These insights into the nature of the cascade also allow a better understanding of the phase-ordering process of temperature-quenched 2D superfluids, where the decay of the vorticity is found to proceed via the turbulent cascade. This connection with turbulence may be a fundamental characteristic of phase-ordering in general.
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Presenters
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Gary Williams
Physics & Astronomy, UCLA
Authors
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Andrew Forrester
Physics & Astronomy, UCLA
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Han-Ching Chu
Physics & Astronomy, UCLA
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Gary Williams
Physics & Astronomy, UCLA