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Quantized Vortices and Quantized Vortices and Quantum Turbulence - - PowerPoint PPT Presentation

Quantized Vortices and Quantized Vortices and Quantum Turbulence Quantum Turbulence Makoto TSUBOTA Department of Physics, Osaka City University, Japan Review article M. Tsubota, J. Phys. Soc. Jpn.77 (2008) 111006 Progress in Low


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SLIDE 1

Quantized Vortices and Quantized Vortices and Quantum Turbulence Quantum Turbulence

Makoto TSUBOTA

Department of Physics, Osaka City University, Japan

Review article ・ M. Tsubota, J. Phys. Soc. Jpn.77 (2008) 111006 ・ Progress in Low Temperature Physics Vol.16, eds.

  • W. P. Halperin and M. Tsubota, Elsevier, 2009
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SLIDE 2

What is “quantum”?

Element of something

What is “quantum mechanics”?

Mechanics with element Energy, momentum and angular momentum etc. are quantized. The element is determined by the Planck’s constant h.

What is “quantum turbulence”?

Turbulence with some “element”

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SLIDE 3

Leonardo Da Vinci (1452-1519)

Da Vinci observed turbulent flow and found that turbulence consists of many vortices with different scales. Turbulence is not a simple disordered state but having some structures with vortices.

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SLIDE 4

Certainly turbulence looks to have many vortices.

Turbulence behind a dragonfly However, these vortices are unstable; they repeatedly appear, diffuse and disappear.

It is not so straightforward to confirm the Da Vinci message in classical turbulence.

http://www.nagare.or.jp/mm/2004/gallery/iida/dragonfly.html

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SLIDE 5

The Da Vinci message “turbulence consists of vortices” is actually realized in quantum turbulence (QT) comprised of quantized vortices.

Key concept

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SLIDE 6

Contents

  • 0. Introduction

Basics of Quantum Hydrodynamics of the GP(Gross- Pitaevskii) model, Brief research history of QT

  • 1. Vortex lattice formation in a rotating BEC(Bose-

Einstein condensate)

  • 2. QT by the GP model -Energy spectrum-
  • 3. QT in atomic BECs
  • 4. Quantized vortices in two-component BECs

Quantum Kelvin-Helmholtz instability, QT

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SLIDE 7

Each atom behaves as a particle at high temperatures.

Each atom occupies the same single particle ground

  • state. The matter waves become coherent, making a

macroscopic wave function Ψ . Thermal de Broglie wave length ~ Distance between particles

Each atom behaves like a wave at low temperatures.

Bose-Einstein condensation (BEC)

  • 0. Introduction

Ψ

Quantum mechanics ~ Duality of matter and wave ~

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SLIDE 8

Basics of quantum hydrodynamics of the GP model (1)

The wave function Ψ obeys the Gross-Pitaevskii (GP) equation

ih t = h2 2m 2 + µ

  • + g

2

(1) When we use the expression , the real and imaginary parts of Eq. (1) are reduced to

r,t

( ) =

n0 r,t

( ) exp i r,t ( )

[ ]

n0 t = h 2m 2 n0 + n02

( )

h t = h2 2m

  • (

)

2 2 n0

n0

  • + µ gn0

(2) (3)

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SLIDE 9

Basics of quantum hydrodynamics of the GP model (2)

n0 t = h 2m 2 n0 + n02

( )

(2) Equation (2) is a continuity equation of the condensate. The flux density with gives

j = ih 2m * *

( )

= n0 exp i

[ ]

j = n0vs, vs h m n0 t = j

Superflow is driven by the potential θ which is the phase of the wave function.

vs

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SLIDE 10

Basics of quantum hydrodynamics of the GP model (3)

h t = h2 2m

  • (

)

2 2 n0

n0

  • + µ gn0

(3) Equation (3) with leads to the equation of superflow

vs = h m vs t + vs

( )vs = 1

m µ gn0 + h 2m 2 n0 n0

  • Equation (4) is quite similar to the Euler equation of a perfect

fluid, but has a different term of “quantum pressure”. (4) The quantum pressure plays an important role in nucleation and reconnection of quantized vortices.

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SLIDE 11

Summary of this part

GP Eq. with

ih t = h2 2m 2 + µ

  • + g

2

= n0 exp i

[ ]

Continuity Eq. of the density n0 Euler-like Eq. of Superflow Superflow

n0 t = j, j = n0vs

vs h m

vs t + vs

( )vs = 1

m µ gn0 + h 2m 2 n0 n0

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SLIDE 12

Quantization of circulation Quantization of circulation Superfow

vs = h m Single-connected region

A vortex with quantized circulation and vacant core

Quantized vortex Quantized vortex

= vs dl = h m dl = h m

C

  • C
  • n

(n: integer) Multi-connected region = vs dl

C

  • = 0, rot vs = 0

Basics of quantum hydrodynamics of the GP model (4)

Quantized circulation = h m

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SLIDE 13

A quantized vortex is a vortex of superflow in a BEC. Any rotational motion in superfluid is sustained by quantized vortices.

(i) The circulation is quantized. (iii) The core size is very small.

vs ds =n

  • n = 0,1, 2,L

( )

A vortex with n≧2 is unstable. (ii) Free from the decay mechanism of the viscous diffusion of the vorticity.

Every vortex has the same circulation. The vortex is stable. ρ r

s

~Å (r) rot vs The order of the coherence length.

= h / m

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SLIDE 14

Classical Turbulence (CT) vs. Quantum Turbulence (QT) Classical turbulence Quantum turbulence

・The vortices are unstable. Not easy to identify each vortex. ・The circulation differs from one to another, not conserved. ・The quantized vortices are stable topological defects. ・Every vortex has the same circulation. ・Circulation is conserved.

Motion of vortex cores

QT can be much simpler than CT, because each element of turbulence is well-defined.

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SLIDE 15

Models available for simulation of QT

Vortex filament model Biot-Savart law A vortex makes the superflow of the Biot-Savart law, and moves with this local flow.

vs r

( ) =

4 s r

( ) d s

s r

3

  • s

r Gross-Pitaevskii (GP) model for the macroscopic wave function

ih(r,t) t = h22 2m + Vext(r) + g (r,t)

2

  • (r,t)

(r) = n0(r)e

i( r )

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SLIDE 16
  • Brief Research History of QT -

Liquid 4He enters the superfluid state below 2.17 K (λ point) with Bose-Einstein condensation. Its hydrodynamics are well described by the two-fluid model:

Temperature (K)

point

The two-fluid model (Tisza, Landau)

The system is a mixture of inviscid superfluid and viscous normal fluid.

= s + n

j = svs + nvn

Normal fluid Superfluid

Entropy Viscosity Velocity Density

s T

( )

n T

( )

vs r

( )

vn r

( )

n T

( )

sn T

( )

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SLIDE 17

The two-fluid model can explain various experimentally

  • bserved phenomena of superfluidity (e.g., the

thermomechanical effect, film flow, etc.)

However, …

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SLIDE 18

(ii) v > v

s c

vs

A tangle of quantized vortices develops. The two fluids interact through mutual friction generated by tangling, and the superflow decays.

v = 0

s

Superfluidity breaks down in fast flow

(i) v < v

s c

vs

The two fluids do not interact so that the superfluid can flow forever without decaying.

vs

t

(some critical velocity)

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SLIDE 19

1955: R. P. Feynman proposed that “superfluid turbulence” consists of a tangle of quantized vortices. 1955 – 1957: W. F. Vinen observed “superfluid turbulence”. Mutual friction between the vortex tangle and the normal fluid causes dissipation of the flow.

Progress in Low Temperature Physics Vol. I (1955), p.17 Such a large vortex should break up into smaller vortices like the cascade process in classical turbulence.

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SLIDE 20

Many experimental studies were conducted chiefly on thermal counterflow of superfluid 4He. 1980s K. W. Schwarz Phys. Rev. B38, 2398 (1988)

Performed a direct numerical simulation of the three-dimensional dynamics of quantized vortices and succeeded in quantitatively explaining the observed temperature difference ΔT .

Vortex tangle

Heater Normal flow Superflow

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SLIDE 21

Development of a vortex tangle in a thermal counterflow

  • K. W. Schwarz, Phys. Rev. B38, 2398

(1988). Schwarz obtained numerically the statistically steady state of a vortex tangle, which is sustained by the competition between the applied flow and the mutual friction.

vs vn Counterflow turbulence has been successfully explained. Vortex filament model

  • H. Adachi, S. Fujiyama, MT, Phys. Rev.

B81, 104511(2010)(Editors suggestion) We made more correct simulation by taking the full account of the vortex interaction.

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SLIDE 22

What is the relation between superfluid turbulence and classical turbulence?

Most studies of superfluid turbulence have focused on thermal counterflow.

⇨ No analogy with classical turbulence

When Feynman drew the above figure, he was thinking of a cascade process in classical turbulence.

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SLIDE 23

New era of quantum turbulence has come!

  • 1. Superfluid helium

Classical analogue has been considered since 1998. ~ Energy spectrum of QT ~

  • 2. Atomic Bose-Einstein condensates (BECs)

BEC was realized in 1995.

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SLIDE 24

Contents

  • 0. Introduction

Basics of Quantum Hydrodynamics of the GP model, Brief research history of QT

1. Vortex lattice formation in a rotating BEC 2. QT by the GP model -Energy spectrum- 3. QT in atomic BECs 4. Quantized vortices in two-component BECs

Quantum Kelvin-Helmholtz instability, QT

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SLIDE 25
  • 1. Vortex lattice formation in a rotating BEC

M.Tsubota, K.Kasamatsu, M.Ueda, Phys.Rev.A65, 023603(2002) K.Kasamatsu, T.Tsubota, M.Ueda, Phys.Rev.A67, 033610(2003)

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SLIDE 26

Realization of atomic gas BEC 1995 87Rb, 7Li, 23Na Laser cooling

An atom is subjected to a laser beam whose frequency is tuned to lie just below that of an atomic transition between an excited state and the ground state. → An atom moving toward to the laser beam absorbs it by the Doppler shift, reducing its velocity. Cold atoms are collected at the focus of six laser beams. T~ 100μK

Magnetic trap

Trapping cooled gases

Evaporation cooling

Atoms with high kinetic energy are released from the trapping potential.

BEC T~ 100 nK

Motion of atoms is reduced by laser. The atoms are trapped by potential. The fast atoms are released out

  • f the trap.
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SLIDE 27

Observation of BEC

Turning off the trapping potential, → the gas expands with falling feely. → The observation of the position of atoms determines the initial distribution of velocity.

By MIT

The Nobel Prize in Physics 2001!

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The fluid rotates with the same angular velocity with the vessel. This means that there appears one vortex in the vessel. The single vortex can make the solid-body rotation with any angular velocity.

What happens if we rotate a vessel having a usual viscous classical fluid inside?

This does not occur in quantum fluids! Such experiments were done in atomic BECs.

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SLIDE 29

Observation of quantized vortices in atomic BECs

K.W.Madison, et al. PRL 84, 806 (2000) J.R. Abo-Shaeer, et al. Science 292, 476 (2001)

  • P. Engels, et al.

PRL 87, 210403 (2001)

ENS MIT JILA

  • E. Hodby, et al.

PRL 88, 010405 (2002)

Oxford

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SLIDE 30

How can we rotate the trapped BEC?

K.W.Madison et al. Phys.Rev Lett 84, 806 (2000)

Non-axisymmetric potential Optical spoon Total potential

Rotation frequency

Ω

z x y

100µm 5µm 20µm 16µm Ustir(R) = m 2

2 (xX 2 + yY 2)

Vext(R) = Vtrap(R) + Ustir(R)

x y

Axisymmetric potential

“cigar-shape”

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SLIDE 31

Direct observation of the vortex lattice formation

Snapshots of the BEC after turning on the rotation

  • 1. The BEC becomes

elliptic, then oscillating.

  • 2. The surface becomes unstable.
  • 3. Vortices enter the BEC

from the surface.

  • 4. The BEC recovers the

axisymmetry, the vortices forming a lattice.

K.W. Madison et al. PRL 86 , 4443 (2001)

Rx Ry

= Rx

2 Ry 2

Rx

2 + Ry 2

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SLIDE 32

The Gross-Pitaevskii(GP) equation in a rotating frame

Wave function Interaction

s-wave scattering length

ih t = h2 2m 2 + Vtrap + g

2

(r,t)

g = 4h2as m as

in a rotating frame

ih t = h2 2m 2 + (Vtrap + Ustir) + g

2 Lz

Ustir(R) = m 2

2 (xX 2 + yY 2)

Two-dimensional

simplified

Ω Ω

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SLIDE 33

The GP equation with a dissipative term

ih t = h2 2m 2 + (Vtrap + Ustir) + g

2 µ Lz

  • (i )h

t = 0.03: dimensionless parameter

S.Choi, et al. PRA 57, 4057 (1998) I.Aranson, et al. PRB 54, 13072 (1996)

This dissipation comes microscopically from the interaction between the condensate and the noncondensate.

E.Zaremba, T. Nikuni, and A. Griffin, J. Low Temp. Phys. 116, 277 (1999) C.W. Gardiner, J.R. Anglin, and T.I.A. Fudge, J. Phys. B 35, 1555 (2002)

  • M. Kobayashi and M. Tsubota, Phys. Rev. Lett. 97, 145301 (2006)
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SLIDE 34

Profile of a single quantized vortex

h2

2m

2 + Vtrap + g 2 = µ

(r) = n0(r)e

i( r )

A quantized vortex

n0

  • Velocity field

0.005 0.01 0.015 0.02 2 4 6 8 10

r

||

2

Vortex core= healing length

h 2mgn0

A vortex

vs h m

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SLIDE 35

Dynamics of the vortex lattice formation (1)

Time development of the condensate density n0

= 0.7

Experiment

MT, K. Kasamatsu,

  • M. Ueda, Phys. Rev.

A 65, 023603 (2002)

V

trap(r) = 1

2 m

2r 2

(r) = n0(r)e

i( r )

K.W.Madison et al. PRL 86 , 4443 (2001)

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SLIDE 36

Dynamics of the vortex lattice formation (2)

t=0 67ms 340ms 390ms 410ms 700ms

Time-development of the condensate density n0

Are these holes actually quantized vortices?

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SLIDE 37

Dynamics of the vortex lattice formation (3)

Time-development of the phase

(r) = n0(r)e

i( r )

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SLIDE 38

Dynamics of the vortex lattice formation (4)

t=0 67ms 340ms 390ms 410ms 700ms

Ghost vortices Becoming real vortices Time-development of the phase

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SLIDE 39

Simultaneous display of the density and the phase

M.Tsubota, K.Kasamatsu, M.Ueda, Phys.Rev.A65, 023603(2002) K.Kasamatsu, T.Tsubota, M.Ueda, Phys.Rev.A67, 033610(2003)

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SLIDE 40

Contents

  • 0. Introduction

Basics of Quantum Hydrodynamics of the GP model, Brief research history of QT

1. Vortex lattice formation in a rotating BEC 2. QT by the GP model -Energy spectrum- 3. QT in atomic BECs 4. Quantized vortices in two-component BECs

Quantum Kelvin-Helmholtz instability, QT

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SLIDE 41
  • 2. QT by the GP model
  • M. Kobayashi, MT, Phys. Rev. Lett. 94, 065302 (2005):
  • J. Phys. Soc. Jpn.74, 3248 (2005)

The main interests What is the relation between QT and CT? How similar? How different? We will focus on the statistical quantities.

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SLIDE 42

Energy spectra of fully developed turbulence

Energy- containing range Inertial range Energy-dissipative range

Energy spectrum of turbulence

Kolmogorov law

Energy spectrum of the velocity field Energy-containing range

The energy is injected into the system at .

k k0 = 1/ l0

Inertial range

Dissipation does not work. The nonlinear interaction transfers the energy from low k region to high k region. Kolmogorov law (K41) : E(k)=Cε2/3 k -5/3

Energy-dissipative range

The energy is dissipated with the rate ε at the Kolmogorov wave number kc = (ε/ν3 )1/4. Richardson cascade process

E = 1 2 v

  • 2 dr =

E(k)dk

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SLIDE 43

Most textbooks describe this kind of Richardson cascade. However, this is only a cartoon; nobody has ever confirmed it clearly. One of the reasons is that it is not so easy to identify each eddy in a fluid.

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SLIDE 44

Does quantum turbulence (QT) satisfy the Does quantum turbulence (QT) satisfy the Kolmogorov law? Kolmogorov law? If so, QT If so, QT shows some analogy with CT. shows some analogy with CT. Having this sort of motivation, the studies Having this sort of motivation, the studies

  • f QT have entered a new stage since the
  • f QT have entered a new stage since the

middle of 90 middle of 90’ ’s ! s !

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SLIDE 45

Energy spectra of quantum turbulence (QT)

Decaying Kolmogorov turbulence in a model of superflow

  • C. Nore, M. Abid and M.E.Brachet, Phys.Fluids 9, 2644 (1997)

The Gross-Pitaevskii (GP) model Energy Spectrum of Superfluid Turbulence with No Normal-Fluid Component

  • T. Araki, M.Tsubota and S.K.Nemirovskii, Phys.Rev.Lett.89, 145301(2002)

The vortex-filament model Kolmogorov Spectrum of Superfluid Turbulence: Numerical Analysis of the Gross-Pitaevskii Equation with a Small-Scale Dissipation

  • M. Kobayashi and M. Tsubota,
  • Phys. Rev. Lett. 94, 065302 (2005), J. Phys. Soc. Jpn.74, 3248 (2005).

There are three works which directly study the energy spectrum of QT at zero temperature.

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SLIDE 46
  • C. Nore, M. Abid and M.E.Brachet, Phys.Fluids 9, 2644(1997)

By using the GP model, they

  • btained a vortex tangle with

starting from the Taylor- Green vortices.

t=2

4 6 8 10 12

We should note that the GP model describes a compressible fluid.

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SLIDE 47

In order to study the Kolmogorov spectrum, it is necessary to decompose the total energy into some components. (Nore et al., 1997)

Total energy The kinetic energy is divided into the compressible part with and the incompressible part with .

E = 1 dx

  • dx

* 2 + g

2

2

  • E = Eint + Eq + Ekin

= exp i

( )

Ekin = 1 dx

  • dx

( )

  • 2

Ekin

c =

1 dx

  • dx

( )

c

[ ]

  • 2

Ekin

i =

1 dx

  • dx

( )

i

[ ]

  • 2

div

( )

i = 0

rot

( )

c = 0

This incompressible kinetic energy Ekini should

  • bey the Kolmogorov spectrum.
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SLIDE 48
  • C. Nore, M. Abid and M.E.Brachet, Phys.Fluids 9, 2644(1997)

△: 2 < k < 12 ○: 2 < k < 14 □: 2 < k < 16

The right figure shows the energy spectrum at a moment. The left figure shows the development of the exponent n(t). The exponent n(t) goes through 5/3 on the way of the dynamics.

n(t) t k E(k)

5/3

E(k)~ k -n(t) In the late stage, however, the exponent deviates from 5/3, because the sound waves resulting from vortex reconnections disturb the cascade process of the inertial range.

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SLIDE 49

Reconnection of quantized vortices (Numerical analysis of the Gross-Pitaevskii equation)

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SLIDE 50
  • C. Nore, M. Abid and M.E.Brachet, Phys.Fluids 9, 2644(1997)

△: 2 < k < 12 ○: 2 < k < 14 □: 2 < k < 16

The right figure shows the energy spectrum at a moment. The left figure shows the development of the exponent n(t). The exponent n(t) goes through 5/3 on the way of the dynamics.

n(t) t k E(k)

5/3

E(k)~ k -n(t) In the late stage, however, the exponent deviates from 5/3, because the sound waves resulting from vortex reconnections disturb the cascade process of the inertial range.

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SLIDE 51

Kolmogorov spectrum of quantum turbulence

  • M. Kobayashi and M. Tsubota, Phys. Rev. Lett. 94, 065302 (2005),
  • J. Phys. Soc. Jpn. 74, 3248 (2005)
  • 1. We solved the GP equation in the wave number

space in order to use the fast Fourier transformation.

  • 2. We made a steady state of turbulence. In order

to do that, 2-1 We introduced a dissipative term which dissipates the Fourier component of the high wave number, namely, phonons of short wave length. 2-2 We excited the system at a large scale by moving a random potential.

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SLIDE 52

To solve the GP equation numerically with high accuracy, we use the Fourier spectral method in space with the periodic boundary condition in a cube.

The GP equation in the Fourier space

healing length giving the vortex core size

i t k,t

( ) = k

2 µ

( ) k,t

( )

+ g V 2 k1,t

( ) * k2,t ( ) k k1 + k2,t ( )

k1 ,k 2

  • 2 = 1 g

2

The GP equation in the real space

i t r,t

( ) =

2 µ + g r,t

( )

2

[ ] r,t

( )

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SLIDE 53

The GP equation with the small scale dissipation

:healing length giving the vortex core size

We introduce the dissipation that works only in the scale smaller than ξ.

  • 2 = 1 g

2

{i (k)} t k,t

( ) = k

2 µ

( ) k,t

( )

+ g V 2 k1,t

( ) * k2,t ( ) k k1 + k2,t ( )

k1 ,k 2

  • (k ) = 0 k 2 /

( )

How to dissipate the energy at small scales?

Since there is no vortex motion at the scales smaller than ξ, this dissipation must work for only short-wavelength sound waves.

  • cf. M. Kobayashi and M. Tsubota, PRL 97, 145301 (2006)
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SLIDE 54

This is done by moving the random potential satisfying the space-time correlation:

V(x,t)V( x , t ) = V

2 exp x

x

( )

2

2X0

2

t t

( )

2

2T

2

  • The variable X0 determines the

scale of the energy-containing range.

V0=50, X0=4 and T0=6.4×10-2

How to inject the energy at large scales?

X0 ξ

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SLIDE 55

Thus steady turbulence is obtained.(1)

Time development of each energy component

Vortices Phase in a central plane Moving random potential

slide-56
SLIDE 56

Thus steady turbulence is obtained.(2)

Time development of each energy component

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SLIDE 57

Energy spectrum of the steady turbulence

The energy spectrum obeys the Kolmogorov form. Quantum turbulence is found to show the essence

  • f classical turbulence!

2π / X0 2π / ξ

The inertial range is sustained by the Richardson cascade of quantized vortices.

  • M. Kobayashi and M. Tsubota,
  • J. Phys. Soc. Jpn. 74, 3248 (2005)
slide-58
SLIDE 58

Picture of the cascade process

Quantized vortices Phonons (wave turbulence?)

slide-59
SLIDE 59

Contents

  • 0. Introduction

Basics of Quantum Hydrodynamics of the GP model, Brief research history of QT

1. Vortex lattice formation in a rotating BEC 2. QT by the GP model -Energy spectrum- 3. QT in atomic BECs 4. Quantized vortices in two-component BECs

Quantum Kelvin-Helmholtz instability, QT

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SLIDE 60

Atomic BEC Superfluid He Vortex tangle Vortex lattice

There are two main cooperative phenomena of quantized vortices; Vortex lattice under rotation and Vortex tangle (Quantum turbulence).

None

3.

  • 3. QT in Atomic Bose-Einstien condensates (BECs)
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SLIDE 61

Is it possible to make turbulence in a trapped BEC?

(1) We cannot apply some dc flow to the system. (2) This is a finite-size trapped system. Is this serious?

We use the idea of rotating turbulence.

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SLIDE 62

QT in a trapped BEC

  • 1. Trap the BEC in a

weakly elliptic potential.

U x

( ) = m 2

2 11

( ) 12 ( )x 2 + 1+ 1 ( ) 12 ( )y 2 + 1+ 2 ( )z2

[ ]

  • 2. Rotate the system first

around the x-axis, next around the z-axis. x y z

t

( ) = x, zsinxt, z cosxt

( )

  • M. Kobayashi and M. Tsubota, Phys. Rev. A76, 045603 (2007)

Making QT by combining two rotations

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SLIDE 63

Actually this idea has been already used in CT.

  • S. Goto, N. Ishii, S. Kida, and M. Nishioka, Phys. Fluids 19, 061705 (2007)

Rotation around

  • ne axis

Rotation around two axes

slide-64
SLIDE 64

Precession

Precessing motion of a gyroscope

Spin axis itself rotates around another axis.

We consider the case where the spinning and precessing rotational axes are perpendicular to each other. Hence, the two rotations do not commute, and thus cannot be represented by their sum. Ωz Ωx Are these two rotations represented by their sum? No! Are these two rotations represented by their sum? No!

slide-65
SLIDE 65

Condensate density Quantized vortices

Two precessions (ωx×ωz) We confirmed a scaling law

  • f the energy spectrum

similar to K41.

  • M. Kobayashi and M. Tsubota, Phys. Rev. A76, 045603 (2007)

n 1.78 ± 0.194

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SLIDE 66

Recently quantum turbulence was realized also in atomic BECs!

Henn et al., PRL103, 045301(2009)

Coupled large amplitude oscillation

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SLIDE 67
  • 4. Quantized vortices in two-component BECs

Review article: K.Kasamatsu, MT, M.Ueda, Int. J. Mod.

  • Phys. 11, 1835(2005)
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SLIDE 68

Vortices and hydrodynamics in multi-component BECs

Depending on the symmetry, multi-component order parameters can yield various kinds of topological defects.

Triangular (Abrikosv)lattice

Ω

?

Ω

Ψ1 Ψ3 Ψ2 Ψ4 Topological defects in two-component BECs superfluid 3He, superconductivity with non-s-wave symmetry (Sr2RuO4, UPt3 ), bilayer quantum Hall systen, nonlinear optics, nuclear physics, cosmology(Neutron star), …

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SLIDE 69

0.005 0.01 0.015

  • 10
  • 5

5 10

|1|2 |2|2

  • 0.4

0.5 0.6 0.7 0.8 0.9 1 0.5 1 1.5

  • g12/g

=

Vortex lattices in rotating two-component BECs

Triangular lattices Square lattices

|ψ1|2 |ψ2|2 Triangle Square x cross section |ψ1|2 |ψ2|2

  • K. Kasamatsu, MT, M. Ueda, PRL91,

150406 (2003)

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SLIDE 70

Hydrodynamic instability in two-component BECs

Quantum Kelvin-Helmholtz instability (KHI)

  • H. Takeuchi, N. Suzuki, K. Kasamatsu, H. Saito, MT, PRB81, 094517 (2010)

Crossover between KHI and counterflow instability

  • N. Suzuki, H. Takeuchi, K. Kasamatsu, MT, H. Saito, PRA81, 063604 (2010)

Counterflow instability and QT

  • H. Takeuchi, S. Ishino, MT, PRL105, 205301(2010);
  • S. Ishino, H. Takeuchi, MT, PRA83, 063602(2011)

Rayleigh-Taylor instability

  • K. Sasaki, N, Suzuki, D. Akamatsu, H. Saito, PRA80, 042704 (2009)
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SLIDE 71

Hydrodynamic instability of shear flows

KHI: KHI:

One of the most fundamental instability in classical fluid dynamics We study the KHI in two-component atomic Bose-Einstein condensates(BECs). 4-1. Quantum Kelvin-Helmholtz instability in two-component BECs

  • H. Takeuchi, N. Suzuki, K. Kasamatsu, H. Saito, M. Tsubota,
  • Phys. Rev. B81, 094517(2010).
slide-72
SLIDE 72

Classical KHI

When the relative velocity Vd=|V1-V2| is sufficiently large, the vortex sheet becomes dynamically unstable and the interface modes with complex frequencies are amplified.

interface

V1 V2

slide-73
SLIDE 73

Two-component BEC

Two order parameters (macroscopic wave functions)

Coupled Gross-Pitaevskii(GP) equations m=m1=m2 g=g11=g22

particle density phase

superfluid velocity of component j

iht

1 = h2

2m1 2 + U1 + g11

1 2 + g12 2 2

  • 1

iht2 = h2 2m2 2 + U2 + g12

1 2 + g22 2 2

  • 2
slide-74
SLIDE 74

1 2 3 4 5

  • 30
  • 20
  • 10

10 20 30 x

interface layer g12=10g

y/ξ interface component 1 component 2

y x

V1=0 V2<0 strong repulsive interaction

Phase-separated two-component BEC

Uj(y)=fj y f1 =-f2 > 0 condition for phase separation: g12>g µ=µ1-mV1

2/2= µ2-mV2 2/2 > 0

slide-75
SLIDE 75

Phase diagram of quantum KHI

stable stable

V V2

2=V

=VD

D

wave number

Vd

V V2

2=V

=VL

L

dynamic thermodynamic ω:frequency of ripplon dynamic KHI(analogue of the classical KHI) thermodynamic KHI(unique to quantum KHI)

thermodynamic KHI

( (V VL

L<|V

<|V2

2|)

|) both KHI ( (V VD

D<|V

<|V2

2|

|) )

dynamic KHI in energy conserving systems

dynamic instability superflow instability

  • Analysis by the Bogoliubov-de Gennes equations-
slide-76
SLIDE 76

V1=0 V2≠0

vortex sheet vortex sheet

Dynamic KHI when the energy is conserved

x y ωeff

ji=nivi

effective super-current velocity

stable stable

| |V V2

2|

|=V =VD

D

wave number

|V |V2

2|>

|>V VD

D

relative velocity

Vd

slide-77
SLIDE 77

V1=0 V2≠0

vortex sheet vortex sheet

x y ωeff

ji=nivi

effective super-current velocity

stable stable

| |V V2

2|

|=V =VD

D

wave number

|V |V2

2|>

|>V VD

D

relative velocity

Vd

Dynamic KHI when the energy is conserved

slide-78
SLIDE 78

y x

(3)sawtooth wave

singular

(1)straight vortex sheet (2)amplification (4)singular vorticity (5)release vortex (6)final state

V1=0

|V |V2

2|>

|>V VD

D

Dynamic KHI when the energy is conserved

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SLIDE 79

x y z x z V1=0 V2≠0 Kelvin waves cause more complicated dynamics towards quantum turbulence.

|V |V2

2|>

|>V VD

D

Dynamic KHI in 3D system

slide-80
SLIDE 80

Multi-component BECs are rich stages for exotic instability and vortex structures!

4-2. Counterflow of two-component BECs: two-component quantum turbulence

  • H. Takeuchi, S. Ishino, MT, Phys. Rev. Lett.105, 205301(2010);
  • S. Ishino, H. Takeuchi, MT, Phys. Rev. A83, 063602(2011)
slide-81
SLIDE 81

Superfluid Normal fluid

Heat

BEC 1 BEC 2

Thermal counter flow Counterflow of two-component BECs

When the relative velocity exceeds some critical value, the superfluid becomes turbulent.

When the relative velocity exceeds some critical value, two BECs are expected to become unstable and turbulent.

Motivation

slide-82
SLIDE 82

Two-component GP model

:intracomponent interaction :intercomponent interaction

The mixture is stable. BEC1 BEC2

slide-83
SLIDE 83

:intracomponent interaction :intercomponent interaction

The mixture is stable. BEC1 BEC2

The large relative velocity should make it unstable.

However,

Two-component GP model

  • Ref. V. I. Yukalov and E. P. Yukalova, Laser Phys. Lett. 1, 50 (2004)
slide-84
SLIDE 84

Direction of flow

Density Phase

Results (One-dimension)

, ,

slide-85
SLIDE 85

Phase

Flow direction

x x

Gray solitons

, ,

Results

Density

(One-dimension)

slide-86
SLIDE 86

Density Phase

Results (two-dimension)

Flow direction

, ,

slide-87
SLIDE 87

Density Phase

Flow direction

The solitons decay to vortex pairs through snake instability.

Results (two-dimension)

, ,

slide-88
SLIDE 88

3D 2-component QT

Flow direction

Solitons → Vortex loops → QT

, ,

slide-89
SLIDE 89

Flow direction

The unstable mode is amplified to lead to the disk-shaped low density regions.

Scenario to turbulence (1)

, ,

Isosurface of

slide-90
SLIDE 90

Vortex rings are nucleated inside the low density regions.

, ,

Vortex core of component 1

Scenario to turbulence (2)

Flow direction

Isosurface of

slide-91
SLIDE 91

The vortices expand and grow.

, ,

Scenario to turbulence (3)

Flow direction

Vortex core of component 1 Isosurface of

slide-92
SLIDE 92

The vortices expand to reconnect with other vortices.

, ,

Scenario to turbulence (4)

Flow direction

Vortex core of component 1 Isosurface of

slide-93
SLIDE 93

Eventually the vortices become tangled.

, ,

Scenario to turbulence (5)

Flow direction

Vortex core of component 1 Isosurface of

slide-94
SLIDE 94

Scenario to binary quantum turbulence

slide-95
SLIDE 95

momentum exchange t

J’ L

Scenario to turbulence

Expansion of a ring means “phase slippage”.

0 12.2 12.8 13.3 13.8 26.0

slide-96
SLIDE 96

Why is binary QT interesting?

We know one-component QT obeys the Kolmogorov law(K41).

  • M. Kobayashi, MT, J. Phys. Soc. Jpn. 74, 3248 (2005)

What happens to two-component QT?

  • By changing g12, we can control their coupling.
  • By considering the unsymmetric case g11≠g22, we can

consider the coupling of different QTs. etc.

slide-97
SLIDE 97

Summary

  • 0. Introduction

Basics of Quantum Hydrodynamics of the GP model, Brief research history of QT 1. Vortex lattice formation in a rotating BEC 2. QT by the GP model -Energy spectrum- 3. QT in atomic BECs 4. Quantized vortices in two-component BECs Quantum Kelvin-Helmholtz instability, QT