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Dissipation of quasiclassical turbulence in superfluid 4He

Research output: Contribution to Journal/Magazine › Journal article › peer-review

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Dissipation of quasiclassical turbulence in superfluid 4He. / Zmeev, Dmitriy E.; Walmsley, P. M.; Golov, A. I. et al.
In: Physical review letters, Vol. 115, No. 15, 155303, 09.10.2015.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Zmeev, DE, Walmsley, PM, Golov, AI, McClintock, PVE, Fisher, SN & Vinen, WF 2015, 'Dissipation of quasiclassical turbulence in superfluid 4He', Physical review letters, vol. 115, no. 15, 155303. https://doi.org/10.1103/PhysRevLett.115.155303

APA

Zmeev, D. E., Walmsley, P. M., Golov, A. I., McClintock, P. V. E., Fisher, S. N., & Vinen, W. F. (2015). Dissipation of quasiclassical turbulence in superfluid 4He. Physical review letters, 115(15), Article 155303. https://doi.org/10.1103/PhysRevLett.115.155303

Vancouver

Zmeev DE, Walmsley PM, Golov AI, McClintock PVE, Fisher SN, Vinen WF. Dissipation of quasiclassical turbulence in superfluid 4He. Physical review letters. 2015 Oct 9;115(15):155303. Epub 2015 Oct 8. doi: 10.1103/PhysRevLett.115.155303

Author

Zmeev, Dmitriy E. ; Walmsley, P. M. ; Golov, A. I. et al. / Dissipation of quasiclassical turbulence in superfluid 4He. In: Physical review letters. 2015 ; Vol. 115, No. 15.

Bibtex

@article{8b5a51693afa4522bd73a4691641b9f5,
title = "Dissipation of quasiclassical turbulence in superfluid 4He",
abstract = "We compare the decay of turbulence in superfluid 4He produced by a moving grid to the decay of urbulence created by either impulsive spin-down to rest or by intense ion injection. In all cases the vortex line density L decays at late time t approximately as L / -3/2. At temperatures above 0.8 K, all methods result in the same rate of decay. Below 0.8 K, the spin-down turbulence maintains initial rotation and decays slower than grid turbulence and ion-jet turbulence. This may be due to a decoupling of the large-scale superfluid flow from the normal component at low temperatures, which changes its effective boundary condition from no-slip to slip.",
author = "Zmeev, {Dmitriy E.} and Walmsley, {P. M.} and Golov, {A. I.} and McClintock, {Peter V. E.} and Fisher, {Shaun N.} and Vinen, {W. F.}",
year = "2015",
month = oct,
day = "9",
doi = "10.1103/PhysRevLett.115.155303",
language = "English",
volume = "115",
journal = "Physical review letters",
issn = "1079-7114",
publisher = "American Physical Society",
number = "15",

}

RIS

TY - JOUR

T1 - Dissipation of quasiclassical turbulence in superfluid 4He

AU - Zmeev, Dmitriy E.

AU - Walmsley, P. M.

AU - Golov, A. I.

AU - McClintock, Peter V. E.

AU - Fisher, Shaun N.

AU - Vinen, W. F.

PY - 2015/10/9

Y1 - 2015/10/9

N2 - We compare the decay of turbulence in superfluid 4He produced by a moving grid to the decay of urbulence created by either impulsive spin-down to rest or by intense ion injection. In all cases the vortex line density L decays at late time t approximately as L / -3/2. At temperatures above 0.8 K, all methods result in the same rate of decay. Below 0.8 K, the spin-down turbulence maintains initial rotation and decays slower than grid turbulence and ion-jet turbulence. This may be due to a decoupling of the large-scale superfluid flow from the normal component at low temperatures, which changes its effective boundary condition from no-slip to slip.

AB - We compare the decay of turbulence in superfluid 4He produced by a moving grid to the decay of urbulence created by either impulsive spin-down to rest or by intense ion injection. In all cases the vortex line density L decays at late time t approximately as L / -3/2. At temperatures above 0.8 K, all methods result in the same rate of decay. Below 0.8 K, the spin-down turbulence maintains initial rotation and decays slower than grid turbulence and ion-jet turbulence. This may be due to a decoupling of the large-scale superfluid flow from the normal component at low temperatures, which changes its effective boundary condition from no-slip to slip.

U2 - 10.1103/PhysRevLett.115.155303

DO - 10.1103/PhysRevLett.115.155303

M3 - Journal article

VL - 115

JO - Physical review letters

JF - Physical review letters

SN - 1079-7114

IS - 15

M1 - 155303

ER -