Spectrum of turbulent Kelvin-waves cascade in superfluid helium
Andrew W. Baggaley, Carlo F. Barenghi

TL;DR
This paper investigates the Kelvin-waves cascade in superfluid helium through numerical simulations, analyzing vortex filament interactions, curvature, amplitude spectrum, and fractal dimension to understand turbulence decay.
Contribution
It provides the first detailed numerical analysis of Kelvin-waves cascade, comparing amplitude spectrum results with existing theories.
Findings
Kelvin-waves cascade develops in vortex filament interactions
Amplitude spectrum aligns with certain theoretical models
Fractal dimension analysis offers insights into vortex complexity
Abstract
To explain the observed decay of superfluid turbulence at very low temperature, it has been proposed that a cascade of Kelvin waves (analogous to the classical Kolmogorov cascade) transfers kinetic energy to length scales which are small enough that sound can be radiated away. We report results of numerical simulations of the interaction of quantized vortex filaments. We observe the development of the Kelvin-waves cascade, and compute the statistics of the curvature, the amplitude spectrum (which we compare with competing theories) and the fractal dimension.
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