Shear flow and Kelvin-Helmholtz instability in superfluids.

نویسندگان

  • R Blaauwgeers
  • V B Eltsov
  • G Eska
  • A P Finne
  • R P Haley
  • M Krusius
  • J J Ruohio
  • L Skrbek
  • G E Volovik
چکیده

The first realization of instabilities in the shear flow between two superfluids is examined. The interface separating the A and B phases of superfluid 3He is magnetically stabilized. With uniform rotation we create a state with discontinuous tangential velocities at the interface, supported by the difference in quantized vorticity in the two phases. This state remains stable and nondissipative to high relative velocities, but finally undergoes an instability when an interfacial mode is excited and some vortices cross the phase boundary. The measured properties of the instability are consistent with the classic Kelvin-Helmholtz theory when modified for two-fluid hydrodynamics.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

On Kelvin-Helmholtz instability in superfluids

The Kelvin-Helmholtz instability in superfluids is discussed, based on the first experimental observation of such instability at the interface between superfluid He-A and superfluid He-B [1]. We discuss why the Kelvin-Helmholtz criterion, the Landau critical velocity for nucleation of ripplons, and the free energy consideration all give different values for the instability treshold. 1 Classical...

متن کامل

Black - hole horizon and metric singularity at the brane separating two sliding superfluids

An analog of black hole can be realized in the low-temperature laboratory. The horizon can be constructed for the 'relativistic' rip-plons (surface waves) living on the brane. The brane is represented by the interface between two superfluid liquids, 3 He-A and 3 He-B, sliding along each other without friction. Similar experimental arrangement has been recently used for the observation and inves...

متن کامل

نا پایداری کلوین - هلمهولتز در اسپیکول‌های خورشیدی

Magneto hydrodynamic waves, propagating along spicules, may become unstable and the expected instability is of Kelvin-Helmholtz type. Such instability can trigger the onset of wave turbulence leading to an effective plasma heating and particle acceleration. In present study, two-dimensional magneto hydrodynamic simulations performed on a Cartesian grid is presented in spicules with different de...

متن کامل

ar X iv : c on d - m at / 0 11 13 43 v 2 4 M ar 2 00 2 Shear flow and Kelvin - Helmholtz instability in superfluids

R. Blaauwgeers, V. B. Eltsov, G. Eska, A. P. Finne, R. P. Haley, M. Krusius, J. J. Ruohio, L. Skrbek, and G. E. Volovik Low Temperature Laboratory, Helsinki University of Technology, P.O.Box 2200, FIN-02015 HUT, Finland Kamerlingh Onnes Laboratory, Leiden University, P.O.Box 9504, 2300 RA Leiden, The Netherlands Kapitza Institute for Physical Problems, Kosygina 2, 117334 Moscow, Russia Physikal...

متن کامل

Parallel Flow Velocity Shear Kelvin Helmholtz Instability with Ac Electric Field

Electrostatic velocity shear Kelvin-Helmholtz instability has been studied for bi-Maxwellian plasma in the presence of perpendicular a.c. electric field by using the method of characteristic solution. The effects of a.c. electric field temperature variation, velocity shear scale length, electron ion temperature ratio and other parameters on growth rate have been discussed.

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:
  • Physical review letters

دوره 89 15  شماره 

صفحات  -

تاریخ انتشار 2002