quantum condensation: disorder and instability · 2012. 8. 28. · insulator in the lattice after...
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The 6th Windsor Summer School
Low-Dimensional Materials, Strong Correlations and Quantum Technologies
Great Park, Windsor, UK, August 14 - 26, 2012
Quantum Condensation: Disorder and Instability
Boris Altshuler Physics Department, Columbia University
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1.Bose Condensation in the
presence of disorder
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Bose-Einstein Condensation
Macroscopic occupation of a single quantum state
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Bose–Einstein condensation: 2D velocity distribution of Rb atoms at different temperatures, JILA Science, 1995
200nK100nK
0K
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Bose-Einstein Condensation
Macroscopic occupation of a single quantum state
Q: ? 1. External Potential 2. Interaction between the particles
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Superfluid
Mott Insulator
In the lattice
After release of the potential
Markus Greiner, Olaf Mandel, Tilman Esslinger,
Theodor W. Hänsch & Immanuel Bloch “Quantum
phase transition from a superfluid to a Mott insulator in a gas
of ultracold atoms” Nature 415, 39-44 (3 January 2002)
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Bose-Einstein Condensation
Macroscopic occupation of a single quantum state
Q: ? 1. External Potential 2. Interaction between
the particles
In general the problem of bosons subject to an external potential is pathological: at zero temperature all of them will find themselves in the one-particle ground state even if it is a localized one. Even weak interaction is relevant!
?
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Bose-Einstein Condensation
Macroscopic occupation of a single quantum state
Global Phase Coherence – single wave function
Disorder – Localized one-particle states Weak Interaction
Need tunneling
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222
,, ,
2
r ti V r g r t r t
t m
Gross-Pitaevskii equation
Bose-Einstein Condensation
,r t Wave function of the condensate
V r External potential - smooth
Coupling constant Short Range interaction
g
Localized one-particle states? Condensation centers
Discrete version of the GP equation
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222
,, ,
2
r ti V r g r t r t
t m
Gross-Pitaevskii equation
, ir t t “Wave functions” at different condensation centers
Discrete version:
2i
i i i ij i
j i
ti r g t t J t
t
ijJ“Josephson coupling” between the condensation centers i and j
i One-particle energy at the condensation center i
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Gross-Pitaevskii equation
i t “Wave functions” at different condensation centers (CC)
Discrete version:
2i
i i i ij i
j i
ti r g t t J t
t
ijJ“Josephson coupling” between CC i and j
i One-particle energies
Large 2
i t Small quantum fluctuations of
2
i t Only phase matters
ii
i it t e
XY spin model
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Superfluid – Insulator transition
Large 2
i t Small quantum fluctuations of
2
i t Only phase matters
ii
i it t e
XY spin model
Ordered phase – Superfluid
Disordered phase – Insulator Reason for the transition quantum fluctuations of the phase due to the onsite interaction Energy scales in the problem: • Coupling • Dispersion in the one-particle energies • Interaction energy
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12
I
2
1ˆ
I
IH
Hamiltonian
diagonalize
2
1
0
0ˆ
E
EH
22
1212 IEE
Two well problem
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2
1ˆ
I
IH diagonalize
2
1
0
0ˆ
E
EH
II
IIEE
12
121222
1212
von Neumann & Wigner “noncrossing rule”
Level repulsion
v. Neumann J. & Wigner E. 1929 Phys. Zeit. v.30, p.467
What about the eigenfunctions ?
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2
1ˆ
I
IH
II
IIEE
12
121222
1212
What about the eigenfunctions ?
1 1 2 2 1 1 2 2, ; , , ; ,E E
1,2
12
2,12,1
12
IO
I
1,22,12,1
12
I
Off-resonance Eigenfunctions are
close to the original on-site wave functions
Resonance In both eigenstates the probability is equally
shared between the sites
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Anderson
Model
• Lattice - tight binding model
• Onsite energies i - random
• Hopping matrix elements Iij j i
Iij
Iij = { -W < i <W uniformly distributed
I < Ic I > Ic Insulator
All eigenstates are localized
Localization length x
Metal There appear states extended
all over the whole system
Anderson Transition
I i and j are nearest neighbors
0 otherwise
WdfIc
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Anderson insulator Few isolated resonances
Anderson metal There are many resonances
and they overlap
Transition: Typically each site is in the resonance with some other one
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1. Mean level spacing
2. Thouless energy D diffusion constant
. ET has a meaning of the inverse diffusion time of the traveling
through the system or the escape rate (for open systems)
dimensionless Thouless
conductance
L system size
d # of dimensions
L
Energy scales (Thouless, 1972)
1
1
dL
22TE DL
1Tg E 22 Qg e G R G
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Superfluid – Insulator transition
Ordered phase – Superfluid
Disordered phase – Insulator
Tunneling amplitude Energy needed for the tunneling “charging energy”
J
cE
cJ E
cJ E
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Superfluid
Mott Insulator
In the lattice
After release of the potential
Markus Greiner, Olaf Mandel, Tilman Esslinger,
Theodor W. Hänsch & Immanuel Bloch “Quantum
phase transition from a superfluid to a Mott insulator in a gas
of ultracold atoms” Nature 415, 39-44 (3 January 2002)
cJ E
cJ E
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2. Superconductor-Insulator
Transition in two dimensions
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24
Q
c Q
c
R hR R
g e
Superconductor-Insulator Transition
D. B. Haviland, Y. Liu and A. M. Goldman, Phys. Rev. Lett., 62, 2180-2183, (1989).
R
T
cR
? ?
Bi
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0
0
normal z x
Anderson spin chain P.W. Anderson:
Phys. Rev. 112,1800, 1958
SU2 algebra spin 1/2
Anderson spin chain
,,,
ˆ aaaaaaH BCSBCS
aaKaaKaaK z ˆˆ12
1ˆ
,
,,,
ˆˆˆˆ KKKH BCS
z
BCS
BCS
(paired)
xz
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3
2
0
1ln
1
c BCS c
c BCS
D
T T
T g
exp 1c D BCST
}
Ovchinnikov 1973, Maekawa & Fukuyama 1982 Finkelshtein 1987
Disorder-caused corrections to Tc, D
Suppression of Superconductivity
by Coulomb interaction
1.Quantum corrections in normal metals in 2D
Weak localization, e-e interactions
24
2g
e
1ln
g
g g
Dimensionless Thouless conductance
mean free time
frequency, infrared cutoff
2. Correction to due to the Coulomb repulsion
1lnBCS
BCS g
cT
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Anderson Theorem
Neither superconductor
order parameter D nor transition temperature
Tc depend on disorder
Provided that D is homogenous in space
Corrections to the Anderson theorem
– due to inhomogeneity in D
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Interpretation : Tc D exp 1
BCS
SC temperature Debye temperature
Dimensionless
BCS coupling
constant
BCS lnTc
D
1
TcTc
1
glogTc
3
Tc
eff BCS 1 #
gln
1
Tc
Pure BCS interaction (no Coulomb repulsion):
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O
Interpretation continued: “weak localization” logarithm
eff BCS 1 #
gln
1
Tc
Q: Why logarithm?
A: Return and interference
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BCS lnTc
D
1
eff BCS 1 #
gln
1
Tc
•In the universal ( ) limit the effective coupling constant equals to the bare one - Anderson theorem
•If there is only BCS attraction, then disorder increases Tc and D by optimizing spatial
dependence of D. !
Problem in conventional superconductors: Coulomb Interaction
Tc and D reach maxima at the point of Anderson localization
g
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Interpretation continued: Coulomb Interaction
eff BCS #
glnTc
Anderson theorem - the gap is homogenous in space.
Without Coulomb interaction adjustment of the gap to the random potential strengthens superconductivity.
Homogenous gap in the presence of disorder violates electroneutrality; Coulomb interaction tries to restore it and thus suppresses superconductivity
Perturbation theory: 2
2
1 1ln lnc D
c BCS c c
T
T g T T
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3
2
0
1ln
1
c BCS c
c BCS
D
T T
T g
exp 1c D BCST
}
Ovchinnikov 1973, Maekawa & Fukuyama 1982 Finkelshtein 1987
Disorder-caused corrections to Tc, D
Suppression of Superconductivity
by Coulomb interaction
2. Correction to due to the Coulomb repulsion
1lnBCS
BCS g
cT
3. One can sum up triple log corrections neglecting single log terms, i.e. neglecting effects of Anderson localization.
!
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3
2
0
1lnc BCS c
c BCS
T T
T g
Ovchinnikov 1973, Maekawa & Fukuyama 1982 Finkelshtein 1987
Disorder-caused corrections to Tc, D
Suppression of Superconductivity
by Coulomb interaction
4.
One can sum up triple log corrections neglecting localization effects.
Finkelshtein (1987) renormalization group Aleiner (unpublished) BCS-like mean field
2
0
0
ln
ln
g
c
c
c
Tg
Tg
T
2
20
1ln 0c
cBCS
g TT
5.
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Ovchinnikov 1973, Maekawa & Fukuyama 1982 Finkelshtein 1987
Disorder-caused corrections to Tc, D
Suppression of Superconductivity
by Coulomb interaction
4. 2
0
0
ln
ln
g
c
c
c
Tg
Tg
T
2
#0c
BCS
g T
5.
2
11
Q
c c Q
BCS c
Rg R R
g
Conclusion:
critical resistance is much smaller than the quantum resistance c QR R !
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QUANTUM PHASE TRANSITION Theory of Dirty Bosons
Fisher, Grinstein and Girvin 1990
Wen and Zee 1990
Fisher 1990
Only phase fluctuations of the order parameter are
important near the superconductor - insulator transition
CONCLUSIONS
1. Exactly at the transition point and at T 0 conductance
tends to a universal value gqc
2. Close to the transition point magnetic field and
temperature dependencies demonstrate universal scaling
246 ??qc
eg K
h
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0
cESingle grain: charging energy one-particle mean level spacing SC transition temperature SC gap
Granular films.
1
2D array: tunneling conductance
dwell time
normal state sheet resistance
tg
1
1esc tg
QN
t
RR
g
0cT
Below Tc0: Josephson coupling
D
Ambegoakar & Baratoff (1963) J tE g D
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1cg
Fisher, Grinstein & Girvin 1990
Wen and Zee 1990
Fisher 1990
Quantum Phase Transition
Dirty Boson Theory D ∞
Only phase fluctuations
1. Exactly at the transition point and at conductance tends to a universal value
2. Close to the transition point magnetic field and temperature dependencies demonstrate universal scaling
26 ??
4c c Q Q
hR g R R K
e
0T
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Josephson energy
charging energy
superconductor insulator ?
Problem: is renormalized
Superconductor-insulator transition in granular films.
only two energy scales
D JE
cE
J cE E
c JE E
Efetov 1980
cE
0
c cE E
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RPA renormalization
Conventional dynamical screening
0
1
1 1 t
c tc
c c
g
E i i gE
E E
D
2
2
0
1 1
,eff
Dq
U q U q i Dq
Charging energy of a grain
Ambegoakar, Eckern & Schon (1982, 1984)
Example: Coulomb interaction
2 2
2 2
0 222 2
2
4 4, 4eff
e eU q U q e
Dqqq
i Dq
2 2
2
0 2
2
2 2, 2eff
e eU q U q e
Dqqq
i Dq
3d
2d
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+
e
e e
e
e
e
dynamical
screening
Ueff q, U0 q
1 U0 q Dq
2
i Dq2
DISSIPATION
or
DYNAMICAL SCREENING ? ?
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Granular material Homogenous media Correspondence Bare charging energy
Bare potential in the momentum representation
Effective charging energy
Effective potential
Mean spacing of fermionic levels
Fermionic density of states
Dimensionless tunneling conductance
Diffusion constant
RPA renormalization
Conventional dynamical screening
0
1
1 1 t
c tc
c c
g
E i i gE
E E
D
2
2
0
1 1
,eff
Dq
U q U q i Dq
0U q
,effU q
D
0
0cE U q
,c effE U q
1
1 2
tg Dq
cE
0
cE
1
tg
Charging energy of a grain
Ambegoakar, Eckern & Schon (1982, 1984)
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0
1 1
0
1
0 0
1
,
,
,
c
tc c
c c
E I
gE E II
E E III
D
DD
D
0
1
1 1 t
c tc
g
E gE
D {
superconductor insulator
Superconductor-insulator transition in granular films.
J cE E
c JE EJ tE g D
case II 1 cE D J t
c
t
E g
Eg
D
D
1c
c Q
g
R R D
not
! !
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2
1
1
logc
D
g
D
Three Regimes
met
al
superconductor
insulator
II
I
mean level spacing
1
cg
D
1 0
cE
III
0
c cg E D
bare charging energy
SC gap
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superconductor - metal transition I.
T
T
II.
III.
superconductor - insulator transition
superconductor - insulator transition
R
c QR R
R
R
c QR R
QR
homogenous films
0
1 cE D
0
1 cE D
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Regime I homogenous films
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R
T
Bi
Haviland, Liu & Goldman, PRL, (1989)
McGreer, Nease, Haviland, Martinez, Halley & Goldman, PRL, (1991).
Regime II Inhomogeneous films
Regime I. Homogenous films
0
cED
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Regime III. ?
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2
50 100
Baturina, Mironov, Vinokur, Baklanov, & Strunk JETP Lett. 88, 752 (2008)
TiN films
Regime III. ?
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3.Driven Bose Condensation
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? What is the difference between a pendulum clock and a Bose condensate Q:
Absolutely Classical system
Macroscopic Quantum system
? ? ? ? What is in common between a pendulum and a Bose condensate Q: ?
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Oscillator
Single bosonic state
Harmonic, N-th state
N bosons without interaction
Nonlinear, N-th state
N interacting bosons
Classical: .
Macroscopic quantum state N
Bose condensate has a lot in common with a pendulum !?
E 6N
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Of course not But why A:
Can we tell that the pendulum is in a “macroscopic quantum state” ? Q:
!
? What is the difference between a pendulum clock and a Bose condensate Q:
?
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Bose condensate can be in the thermodynamic equilibrium
The pendulum clock needs energy pumping from e.g. gravity in order to compensate the dissipation. Driven system
Answer #1 (correct but incomplete):
Why the pendulum is not a system in “macroscopic quantum state”
?
Q:
What if the bosons have finite life-time and their number is not conserved ?
Q:
?
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E
0N 1N
6N
Bose Condensate: N
Why we can not call the pendulum is in a “macroscopic quantum state” ? Q:
Long range phase coherence.
Can it be used as a signature of the macroscopic quantum state
Another possible answer:
?
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Driven Bose Condensate ?
• stationary state • pumping + dissipation • number of bosons is not conserved
Can we call the laser beam a Bose-condensate of phonons ?
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Hui Deng, Gregor Weihs, Charles Santori, Jacqueline Bloch, and Yoshihisa Yamamoto, “Condensation of semiconductor microcavity exciton polaritons” Science 298, 199–202 (2002).
J. Kasprzak, M. Richard, S. Kundermann, A. Baas, P. Jeambrun, J. M. J.Keeling, F. M. Marchetti, M. H. Szymanska, R. Andre, J. L. Staehli, V. Savona, P. B. Littlewood, B. Deveaud and Le Si Dang,”Bose–Einstein condensation of exciton polaritons ”Nature 443, 409 (2006).
S. O. Demokritov, V. E. Demidov, O. Dzyapko, G. A. Melkov, A. A.
Serga, B. Hillebrands & A. N. Slavin “Bose–Einstein condensation of
quasi-equilibrium magnons at room temperature under pumping”,
Nature 443, pp.430-433 (2006)
J.Klaers, J.Schmitt, F.Vewinger & M.Weitz “Bose–Einstein
condensation of photons in an optical microcavity”, Nature 468,
pp.545–548 (2010)
Bose-condensation out of equilibrium
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2 2
|| 0 min 0 0; ;c k k ck
2D light +
excitons
Photons with weak interaction Polaritons
2
0
02
ck
constant 2D light
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Small effective mass Critical temp. – up to the room temp.
Photons with weak interaction Polaritons
0
410~ mm 1 mTc
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#of incoming particles in unit time # of outgoing particles in unit time Total number of particles
Stationary state:
inn
outn
in outn n
Classical particles with finite lifetime :
inn const
1outn N
N
Bosons: inn WN
outn N
Threshold
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Photons with weak interaction Polaritons
Dissipation.
Pumping
Measurements:
1. Far field. Angular distribution (small deviations from the normal to the plane) of the emitted light momentum distribution of the polaritons.
2. Near field. 2D density of the polaritons.
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Dissipation.
Pumping
Stationary state: Pumping = Dissipation
For bosons both the pumping and the dissipation are proportional to the number of the particles
Instability: lasing threshold
Photons with weak interaction Polaritons
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First observation of the condensation
J. Kasprzak, M. Richard, S. Kundermann, A. Baas, P. Jeambrun, J. M. J. Keeling, F. M. Marchetti, M. H. Szymanska, R. Andre, J. L. Staehli, V. Savona, P. B. Littlewood, B. Deveaud and Le Si Dang, Nature 443, 409 (2006).
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× 673 pixels | 1,280 × 841 pixels.
Compare:
polaritons atoms
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First observation of the condensation
J. Kasprzak, M. Richard, S. Kundermann, A. Baas, P. Jeambrun, J. M. J. Keeling, F. M. Marchetti, M. H. Szymanska, R. Andre, J. L. Staehli, V. Savona, P. B. Littlewood, B. Deveaud and Le Si Dang, Nature 443, 409 (2006).
Polaritons condense at zero in-plane momentum
Why ?
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To the Editor — Several experimental groups have demonstrated that exciton–polaritons quasiparticles made from a mix of light and matter can form a coherent state (that is, a condensate in momentum space) in a semiconductor microcavity. However, there is little agreement in the community regarding the nature and associated terminology of this condensate: is it a Bose–Einstein condensate (BEC), a laser, or something else? Polaritons are also sometimes described as exhibiting superfluidity. Here we wish to point out that describing polaritons and their condensate in terms of a BEC and superfluidity may be misleading.
…
L. V. Butov and A. V. Kavokin
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Polariton array: 1.4-mm-wide Au/Ti strips are equally spaced a =2.8 m. A /2 AlAs cavity (red lines) is sandwiched by two distributed Bragg reflectors with alternating GaAlAs/AlAs /4 layers (two short dotted vertical lines.). The cavity resonance wavelength varies around the quantum well exciton resonance - 776 nm with tapering.
Three stacks of four GaAs quantum wells are positioned at the central three antinodes of the photon field (black oscillatory curve).
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Spatial distribution (near field)
Angular (momentum)distribution (far field) -state
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Phases of the neighboring strips differ by . Condensation to the state with the maximal momentum!
Angular (momentum) distribution (far field)
-state
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Dynamical d-wave condensation of exciton-polaritons in a two-dimensional square-lattice potential Na Young Kim, Kenichiro Kusudo, CongjunWu, Naoyuki Masumoto,
Andreas Löffler,
Sven Höfling, Norio Kumada, LukasWorschech, Alfred Forchel &
Yoshihisa Yamamoto a=4m
Three condensates
simultaneously ?
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atoms
Condensation in periodic potential. Compare:
polaritons
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Exciton-polaritons localized by disorder
Phys. Rev. B 80, 045317 (2009).
5 bright spots
Natural assumption: each spot is the location of a droplet of the Bose-condensate.
This is not the case!
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Exciton-polaritons localized by disorder D. N. Krizhanovskii, K. G. Lagoudakis, M. Wouters, B. Pietka, R. A. Bradley, K. Guda, D. M. Whittaker, M. S. Skolnick, B. Deveaud-Piedran, M. Richard, R. Andre, and Le Si Dang, Phys. Rev. B 80, 045317 (2009)
6 frequency modes real space: 5 spots
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Frequency spectra of each spot
Spatial distribution of each frequency mode
Exciton-polaritons localized by disorder
Each frequency is radiated by several spots; Each spot radiates several frequencies !
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Exciton-polaritons localized by disorder D. N. Krizhanovskii et. Al., Phys. Rev. B 80, 045317 (2009)
Momentum space
Imaging at the energy of each mode:
Real space
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D. N. Krizhanovskii et. Al.,
Phys. Rev. B 80, 045317 (2009) Separated images of the modes
Real space
• Different spots – localized states of exciton-polaritons.
• More modes than localized states? Several condensates on one site?
• Some modes have minimum at (at the ground state!)
• No symmetry?
0k
Momentum space
k k
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One center: Coherent states
• One one-particle state,
• Coherent many-particle states
• Complex number -
• Occupation number is , while is the phase
2z
Need to take into account: • Pumping and dissipation • Nonlinearity=interaction between the bosons
QM description – density matrix
Fokker-Planck equation Langevin equation
a z z z
,z z
aiz z e
eigenvalue of the annihilation operator
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Fokker-Planck eq-n for the density matrix
1. No pumping, no dissipation. Hamiltonian 2,H z z H z
2. Pumping .Dissipation Hamiltonian function W
,z z
2 ImH H H
it z z z z z z
, ,,h z z H z z i z z
,h z z
2
2 Imz zt z
h
zW
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Fokker-Planck eq-n for the density matrix
2. Pumping .Dissipation Hamiltonian function W
,z z
, ,,h z z H z z i z z
,h z z
2
2 Imz zt z
h
zW
3. Hamiltonian of weakly interacting bosons with coupling constant at a state with one-particle energy
2 41
4,H z z z z
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Fokker-Planck eq-n for the density matrix
2. Pumping .Dissipation Hamiltonian function W
,z z
, ,,h z z H z z i z z
,h z z
2
2 Imz zt z
h
zW
3. Hamiltonian of weakly interacting bosons with coupling constant at a state with one-particle energy
2 41
4,H z z z z
4. Dissipative function
21
2,z z g z g W
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Fokker-Planck eq-n for the density matrix
- pumping. - dissipation
W
,z z
2
2 ImH
t zW
z
i
z z
- one-particle energy - coupling constant
2 41
4,H z z z z
monotonically increasing function e.g. due to the depletion of the reservoir
21
2,z z g z
g W
Weakly interacting bosons
2g g z
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Fokker-Planck eq-n for the density matrix
- pumping. - dissipation
W
,z z
2
2 ImH
t zW
z
i
z z
- one-particle energy - coupling constant
2 41
4,H z z z z
monotonically increasing function e.g. due to the depletion of the reservoir
21
2,z z g z
g W
Weakly interacting bosons
2g g z
- threshold 0 0g
2 20
s sg z z
stable number of bosons above the threshold
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,h z zzi f t
t z
Langevin equation One center:
Gaussian random white noise
f z
0;f t
f t f t W t t
2 2
4
2
1
2 I
,2
mh
t z z
h z z z
Wz z
igz
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2z
g i z f tt
One center - conclusions
g W – dissipation; W - pumping
– interaction constant;
Gaussian random white noise
f z
0;f t
f t f t W t t
Threshold: 0W g
Below the threshold: no noise – no light Above the threshold: need nonlinearity in dissipation or pumping
Frequency of the emitted light Blue shift
2 212
H z z
– one-particle energy
2 2g g z g A z
1.
2.
3.
4.
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2z
g i z f tt
One center - conclusions
g W – dissipation; W - pumping
– interaction constant;
Gaussian random white noise
f z
0;f t
f t f t W t t
Frequency of the emitted light Blue shift
2 212
H z z
– one-particle energy
Note: This is the classical equation for a nonlinear oscillator with dissipation in the presence of the noise
Re z - coordinate - momentum Im z
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N>1 centers:
Both matrices and are Hermitian
; 1, 2,...,z z Z N
, ,J
2
,,
,2
2
zh Z Z
z zJ
ig
i
, ,22 2
z z zg i iJ f t
t
212
z
set of independent
centers
Generic bilinear coupling
System of the Langevin equations
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212
1, ,2
, 2h Z Z i z
iJ z z
g
System of coupled nonlinear oscillators
, ,22 2
z z zg i iJ f t
t
, ,J
212
z
N>1 centers: ; 1, 2,...,z z Z N
Two types of coupling: Hermitian ”Josephson” coupling
Anti-Hermitian Dissipative coupling
Both matrices and are Hermitian , ,J
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Josephson coupling-tunneling
Dissipative coupling
, ,22 2
z z zg i iJ f t
t
,J
212
z
,
System of coupled nonlinear oscillators
Physics of the off-diagonal decay:
Interference of the radiated photons
1. N>1 centers: ; 1, 2,...,z z Z N
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Josephson coupling-tunneling
Dissipative coupling
, ,22 2
z z zg i iJ f t
t
,J 212
z ,
Physics of the off-diagonal decay:
Interference of the radiated photons
1. N>1 centers: ; 1, 2,...,z z Z N
0 g Weak lasing regime
The increment is positive when the centers are out of phase
The system is stabilized without nonlinearities in dissipation
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, ,22 2
z z zi iJ f t
tg
0;f f t f t W t t
System of N coupled classical nonlinear oscillators in the presence of the pumping and noise.
212
z
N>1 centers: ; 1, 2,...,z z Z N
It is also a discrete version of the Gross-Pitaevskii equation (nonlinear Schrodinger equation)
222
,, ,
2
r ti V r g r t r t
t m
+ non-Hermitian terms + “thermal” noise
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, ,22 2
z z zi iJ f t
tg
0;f f t f t W t t
System of N coupled classical nonlinear oscillators in the presence of the pumping and noise.
212
z
N>1 centers: ; 1, 2,...,z z Z N
Wouters and Carusotto equation (M. Wouters and I. Carusotto, Phys. Rev. Lett. 99, 140402 (2007). • Include – dependence of the pumping • No noise term • No dissipative coupling
It is also a discrete version of the Gross-Pitaevskii eq-n (1961) + non-Hermitian terms + “thermal” noise
0
z W
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, ,22 2
z z zg i iJ f t
t
0;f f t f t W t t 2
12
z
N>1 centers: ; 1, 2,...,z z Z N
Neglect noise
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Condensation: Stationary (up to the total phase) nontrivial solution
2
, ,2 02 2
z z zg i z iJ
t
N>1 centers: ; 1, 2,...,z z Z N
is always a solution - trivial solution. Are there other nontrivial solutions?
0Z
0i t
Z t e Z
Without dissipative coupling: • g>0 – only trivial solution • g<0 – need to take into account g(z) – dependence • g=0 – threshold
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Condensation: Stationary (up to the total phase) nontrivial solution
2
, ,2 02 2
z z zg i z iJ
t
N>1 centers: ; 1, 2,...,z z Z N
is always a solution - trivial solution. Are there other nontrivial solutions?
0Z
0i t
Z t e Z
the phases of are locked z
BEC Mode locking
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Christiaan Huygens
(1629-1695)
Mode locking: Pendulum Clock
1656 - patented first pendulum clock
1665 – discovered the phenomenon of synchronization
Invisible oscillations of the wooden beam
The second pendulum always had the same frequency and opposite phase as compared with the first one
Q: What about two centers of Bose condensation ?
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, ,2 02 2
z z zg i iJ
t
Without the noise:
2
2z
In linear limit the system resembles “random laser”: • many localized one-particle states, which could
serve as the condensation centers for photons • the photons choose the smallest decay rate
rather than the lowest energy
Difference: Interaction=nonlinearity allows synchronization of the different centers of condensation
0
1. N>1 centers: ; 1, 2,...,z z Z N
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N=2 condensation centers:
2x2 matrices and :
In general We assume time reflection symmetry, i.e.
ˆ ˆ
ˆ ˆ
x y
x y
x y
x yJ J J
1 2( ), ( )z t z t
J
0y yJ
;x xJ J
Remaining 3 variables:
Pauli matrices
1 2( ), ( )z t z t 4 real variables. However the total phase is irrelevant for our discussion
2 2 1 21 2
1 2
, , lnz z
z z iz z
ˆ i
Occupations of the two centers and the phase difference
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N=2 centers: Nontrivial stationary solutions
is always a solution – trivial stationary point 1,2 0z
At two nontrivial solutions appear. One of them is stable (s), another – unstable (u)
g
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N=2 centers:
2x2 matrices and :
In general We assume time reflection symmetry, i.e.
ˆ ˆ
ˆ ˆ
x y
x y
x y
x yJ J J
1 2( ), ( )z t z t
J
0y yJ
;x xJ J
Remaining 3 variables – pseudo spin:
Pauli matrices
1 2( ), ( )z t z t 4 real variables. However the total phase is irrelevant for our discussion
,
ˆ i
iS t z t z t
ˆ i
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N=2 centers: Pseudo spin
,
ˆ i
iS t z t z t
2
1
2
221
122121
122121
zzS
zzzzS
zzzzS
z
y
x
22
1
2
2412 zzS
In components:
x x z y
y y z z x
z z y
S gS S S S S
S gS JS S S S
S gS JS
xS gS S
Equations:
1 2
11 22
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2 2
arctan ; cosJr
r
g J g rS
g Jr
2 2
2 2
gr
J g
0
0
0
x z y
y z z x
z y
gS S S S S
gS JS S S S
gS JS
N=2 centers: Nontrivial stationary points
Stationary points:
is always a solution – trivial stationary point 0S
At two more solutions appear - nontrivial stationary points provided that In polar coordinates they are
g 0S
n ! !
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2 2
arctan ; cosJr
r
g J g rS
g Jr
2 2
2 2
gr
J g
N=2 centers: Nontrivial stationary points
is always a solution – trivial stationary point 0S
At two more solutions appear - nontrivial stationary points provided that In polar coordinates they are
g 0S
Note: time reversal symmetry breaking, which translates into the breaking of the symmetry
0,
k k
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xS
yS
0; 5 ; 0.25J g
xSxS
Nontrivial attractor
Trivial attractor
Saddle point
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STR – stable trivial stationary point UTR – unstable trivial stationary point
SNT – stable nontrivial stationary point UNT – unstable nontrivial stationary point
0S
0S
} }
g
gDistance from the “threshold”
dissipative coupling
original energy mismatch
Stability diagram
0.25
0.5
J
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g
SLC – stable limiting cycle ULC – unstable limiting cycle
g
Nonlinear Zoo: • Hopf bifurcations – subcritical and supercritical
• Fold bifurcations • Period doubling instabilities • . . .
Thanks to Sergej Flach and Kristian Rayanov, MPIPKS, Dresden
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0.3 0.233g 0.3 0.235g
Nonlinear Zoo: • Hopf bifurcations –
subcritical and supercritical
• Fold bifurcations • Period doubling
instabilities • . . .
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2 2
2 2
2 2
arctan ;g
J g
J gS
g J
N=2 centers: Nontrivial stationary points
is always a solution – trivial stationary point 0S
At more solutions - nontrivial stationary points. g
Stable provided that
2
Identical Condensation Centers 0 0
g J
J g Limiting Cycle
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Radiation in the stable states
1. Nontrivial stationary point – single line
2. Limiting cycle – sequence of the lines
3. Trivial stationary state – two lines 4. Line-shapes and photon statistics are determined by the noise 5. Switching between different stable states due
to the noise – Kramers problem. Coexistence of the signals.
6. Phase locking time-reversal symmetry
violation asymmetry k k
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2 2
2 2
2 2
arctan ;g
J g
J gS
g J
N=2n identical condensation centers
For nearest neighbor couplings
g J
n such pairs!
Symmetry breaking Period doubling Close to - state
Ferromagnetic coupling + dissipative coupling
Almost “antiferromagnetic” state
Stable non-stationary states J g ?
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g
J
g JTrivial stationary state
2 nontrivial stationary points
Limiting cycles
1z 2z
2 nontrivial PT-symmetric stationary states
1 2:
:
P z z
T t t
2 identical condensation centers:
2 2
2 2arctan
g
J g
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1z 2z
2 nontrivial PT-symmetric stationary states
1 2: ; :P z z T t t
2N identical condensation centers;
2 2
2 2arctan
g
J g
1 2
3 5 6
7
4
1 2
3 5 6
7
4
g J
g J “Phase transition” point
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Conclusions
• Driven system selects the most stable state rather than the state with the lowest energy
• Nontrivial stable states. System stabilizes itself without adjusting the reservoir. Weak lasing.
• Existing experiments can be naturally interpreted.
• In particular – natural explanation of the violation of the T-invariance
• Equations of motion: Condensation centers = coupled nonlinear oscillators
• Periodic structures: phase locking – driven states of matter . Dissipative coupling is crucial