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arxiv: 1804.01655 · v1 · pith:OTME3XZYnew · submitted 2018-04-05 · ❄️ cond-mat.other · physics.flu-dyn

Dissipation in quantum turbulence in superfluid ⁴He above 1K

classification ❄️ cond-mat.other physics.flu-dyn
keywords kappaoftenquantumsuperfluidtherevortexabovecase
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There are two commonly discussed forms of quantum turbulence in superfluid $^4$He above 1K: in one there is a random tangle of quantizes vortex lines, existing in the presence of a non-turbulent normal fluid; in the second there is a coupled turbulent motion of the two fluids, often exhibiting quasi-classical characteristics on scales larger than the separation between the quantized vortex lines in the superfluid component. The decay of vortex line density, $L$, in the former case is often described by the equation $dL/dt=-\chi_2 (\kappa/2\pi)L^2$, where $\kappa$ is the quantum of circulation, and $\chi_2$ is a dimensionless parameter of order unity. The decay of total turbulent energy, $E$, in the second case is often characterized by an effective kinematic viscosity, $\nu'$, such that $dE/dt=-\nu' \kappa^2 L^2$. We present new values of $\chi_2$ derived from numerical simulations and from experiment, which we compare with those derived from a theory developed by Vinen and Niemela. We summarise what is presently known about the values of $\nu'$ from experiment, and we present a brief introductory discussion of the relationship between $\chi_2$ and $\nu'$, leaving a more detailed discussion to a later paper.

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