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AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability.

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AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability. / Blaauwgeers, R.; Eltsov, V. B.; Eska, G. et al.
In: Physica B: Condensed Matter, Vol. 329-33, No. 1, 05.2003, p. 57-61.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Blaauwgeers, R, Eltsov, VB, Eska, G, Finne, AP, Haley, RP, Krusius, M, Skrbek, L & Volovik, GE 2003, 'AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability.', Physica B: Condensed Matter, vol. 329-33, no. 1, pp. 57-61. https://doi.org/10.1016/S0921-4526(02)01920-8

APA

Blaauwgeers, R., Eltsov, V. B., Eska, G., Finne, A. P., Haley, R. P., Krusius, M., Skrbek, L., & Volovik, G. E. (2003). AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability. Physica B: Condensed Matter, 329-33(1), 57-61. https://doi.org/10.1016/S0921-4526(02)01920-8

Vancouver

Blaauwgeers R, Eltsov VB, Eska G, Finne AP, Haley RP, Krusius M et al. AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability. Physica B: Condensed Matter. 2003 May;329-33(1):57-61. doi: 10.1016/S0921-4526(02)01920-8

Author

Blaauwgeers, R. ; Eltsov, V. B. ; Eska, G. et al. / AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability. In: Physica B: Condensed Matter. 2003 ; Vol. 329-33, No. 1. pp. 57-61.

Bibtex

@article{72022a98c758429da6f3cb21ee0cd73b,
title = "AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability.",
abstract = "The Kelvin-Helmholtz instability takes place on the interface between two horizontally stratified fluid layers which are in a state of relative shear flow with respect to each other. The problem was solved for the ideal case of inviscid and incompressible fluids in 1871 by Lord Kelvin. The first case of superfluid shear flow has been discovered in uniformly rotating superfluid He-3, when the phase boundary between the A and B phases is maintained at a stable location with a magnetic barrier field. At sufficiently high rotation the AB interface undergoes an instability, in which the interface becomes corrugated in a standing-wave pattern. The critical velocity of this process displays the temperature and magnetic field dependences which fit the characteristics of the Kelvin-Helmholtz instability. (C) 2003 Elsevier Science B.V. All rights reserved.",
keywords = "superfluid helium-3, shear flow, Kelvin-Helmholtz instability, AB phase boundary, quantized vortex lines",
author = "R. Blaauwgeers and Eltsov, {V. B.} and G. Eska and Finne, {A. P.} and Haley, {R. P.} and M. Krusius and L. Skrbek and Volovik, {G. E.}",
year = "2003",
month = may,
doi = "10.1016/S0921-4526(02)01920-8",
language = "English",
volume = "329-33",
pages = "57--61",
journal = "Physica B: Condensed Matter",
issn = "0921-4526",
publisher = "ELSEVIER SCIENCE BV",
number = "1",

}

RIS

TY - JOUR

T1 - AB interface in rotating superfluid He-3: the first example of a superfluid shear-flow instability.

AU - Blaauwgeers, R.

AU - Eltsov, V. B.

AU - Eska, G.

AU - Finne, A. P.

AU - Haley, R. P.

AU - Krusius, M.

AU - Skrbek, L.

AU - Volovik, G. E.

PY - 2003/5

Y1 - 2003/5

N2 - The Kelvin-Helmholtz instability takes place on the interface between two horizontally stratified fluid layers which are in a state of relative shear flow with respect to each other. The problem was solved for the ideal case of inviscid and incompressible fluids in 1871 by Lord Kelvin. The first case of superfluid shear flow has been discovered in uniformly rotating superfluid He-3, when the phase boundary between the A and B phases is maintained at a stable location with a magnetic barrier field. At sufficiently high rotation the AB interface undergoes an instability, in which the interface becomes corrugated in a standing-wave pattern. The critical velocity of this process displays the temperature and magnetic field dependences which fit the characteristics of the Kelvin-Helmholtz instability. (C) 2003 Elsevier Science B.V. All rights reserved.

AB - The Kelvin-Helmholtz instability takes place on the interface between two horizontally stratified fluid layers which are in a state of relative shear flow with respect to each other. The problem was solved for the ideal case of inviscid and incompressible fluids in 1871 by Lord Kelvin. The first case of superfluid shear flow has been discovered in uniformly rotating superfluid He-3, when the phase boundary between the A and B phases is maintained at a stable location with a magnetic barrier field. At sufficiently high rotation the AB interface undergoes an instability, in which the interface becomes corrugated in a standing-wave pattern. The critical velocity of this process displays the temperature and magnetic field dependences which fit the characteristics of the Kelvin-Helmholtz instability. (C) 2003 Elsevier Science B.V. All rights reserved.

KW - superfluid helium-3

KW - shear flow

KW - Kelvin-Helmholtz instability

KW - AB phase boundary

KW - quantized vortex lines

U2 - 10.1016/S0921-4526(02)01920-8

DO - 10.1016/S0921-4526(02)01920-8

M3 - Journal article

VL - 329-33

SP - 57

EP - 61

JO - Physica B: Condensed Matter

JF - Physica B: Condensed Matter

SN - 0921-4526

IS - 1

ER -