Non-equilibrium dynamics of cold atoms in optical lattices Vladimir Gritsev Harvard Anatoli...
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Transcript of Non-equilibrium dynamics of cold atoms in optical lattices Vladimir Gritsev Harvard Anatoli...
Non-equilibrium dynamics of cold atoms in optical lattices
Vladimir Gritsev HarvardAnatoli Polkovnikov Harvard/Boston UniversityEhud Altman Harvard/WeizmannBertrand Halperin HarvardMikhail Lukin HarvardEugene Demler Harvard
Harvard-MIT CUA
Motivation: understanding transport phenomena in correlated electron systems
e.g. transport near quantum phase transition
Superconductor to Insulator transition in thin films
Marcovic et al., PRL 81:5217 (1998)
Tuned by film thickness Tuned by magnetic field
V.F. Gantmakher et al., Physica B 284-288, 649 (2000)
Yazdani and KapitulnikPhys.Rev.Lett. 74:3037 (1995)
Scaling near the superconductor to insulator transition
Mason and KapitulnikPhys. Rev. Lett. 82:5341 (1999)
Breakdown of scaling near the superconductor to insulator transition
Outline
Current decay for interacting atoms in optical lattices. Connecting classical dynamical instability with quantum superfluid to Mott transition
Conclusions
Phase dynamics of coupled 1d condensates.Competition of quantum fluctuations and tunneling.Application of the exact solution of quantumsine Gordon model
v
J
Current decay for interacting atoms in optical lattices
Connecting classical dynamical instability with quantum superfluid to Mott transition
References:
J. Superconductivity 17:577 (2004)Phys. Rev. Lett. 95:20402 (2005)Phys. Rev. A 71:63613 (2005)
Atoms in optical lattices. Bose Hubbard model
Theory: Jaksch et al. PRL 81:3108(1998)
Experiment: Kasevich et al., Science (2001) Greiner et al., Nature (2001) Cataliotti et al., Science (2001) Phillips et al., J. Physics B (2002) Esslinger et al., PRL (2004), …
Equilibrium superfluid to insulator transition
1n
t/U
SuperfluidMott insulator
Theory: Fisher et al. PRB (89), Jaksch et al. PRL (98)Experiment: Greiner et al. Nature (01)
U
Moving condensate in an optical lattice. Dynamical instability
v
Theory: Niu et al. PRA (01), Smerzi et al. PRL (02)Experiment: Fallani et al. PRL (04)
Related experiments byEiermann et al, PRL (03)
This talk: This talk: How to connectHow to connect the the dynamical instabilitydynamical instability (irreversible, classical) (irreversible, classical)to the to the superfluid to Mott transitionsuperfluid to Mott transition (equilibrium, quantum) (equilibrium, quantum)
U/t
p
SF MI
???Possible experimental
sequence:
Unstable
???
p
U/J
Stable
SF MI
This talk
Linear stability analysis: States with p> are unstable
Classical limit of the Hubbard model. Discreet Gross-Pitaevskii equation
Current carrying states
r
Dynamical instability
Amplification ofdensity fluctuations
unstableunstable
GP regime . Maximum of the current for .
When we include quantum fluctuations, the amplitude of the order parameter is suppressed
Dynamical instability for integer filling
decreases with increasing phase gradient
Order parameter for a current carrying state
Current
SF MI
p
U/J
Dynamical instability for integer filling
0.0 0.1 0.2 0.3 0.4 0.5
p*
I(p)
s(p)
sin(p)
Condensate momentum p/
Dynamical instability occurs for
Vicinity of the SF-I quantum phase transition. Classical description applies for
Dynamical instability. Gutzwiller approximation
0.0
0.1
0.2
0.3
0.4
0.5
0.0 0.2 0.4 0.6 0.8 1.0
d=3
d=2
d=1
unstable
stable
U/Uc
p/
Wavefunction
Time evolution
Phase diagram. Integer filling
We look for stability against small fluctuations
Order parameter suppression by the current. Number state (Fock) representation
Integer filling
N N+1N-1 N+2N-2
N N+1N-1 N+2N-2
Order parameter suppression by the current. Number state (Fock) representation
Integer filling
N-1/2 N+1/2N-3/2 N+3/2
N-1/2 N+1/2N-3/2 N+3/2
N N+1N-1 N+2N-2
N N+1N-1 N+2N-2
Fractional filling
SF MI
p
U/J
Dynamical instability
Integer filling
p
Fractional filling
U/J
The first instability develops near the edges, where N=1
0 100 200 300 400 500
-0.2
-0.1
0.0
0.1
0.2
0.00 0.17 0.34 0.52 0.69 0.86
Cen
ter
of M
ass
Mom
entu
m
Time
N=1.5 N=3
U=0.01 tJ=1/4
Gutzwiller ansatz simulations (2D)
Optical lattice and parabolic trap. Gutzwiller approximation
Beyond semiclassical equations. Current decay by tunneling
pha
se
jpha
se
jpha
se
j
Current carrying states are metastable. They can decay by thermal or quantum tunneling
Thermal activation Quantum tunneling
S – classical action corresponding to the motion in an inverted potential.
Decay of current by quantum tunnelingp
hase
j
Escape from metastable state by quantum tunneling.
WKB approximation
pha
se
j
Quantumphase slip
Decay rate from a metastable state. Example
0
22 3
0
1 ( ) 0
2 c
dxS d x bx p p
m d
2
1
1 2 cos
2j
j jj
dS d JN
U d
At p/2 we get
2
2 3
1 1
1 cos
2 3j
j j j jj
d JNS d JN p
U d
j jpj
Weakly interacting systems. Quantum rotor model.Decay of current by quantum tunneling
For the link on which the QPS takes place
d=1. Phase slip on one link + response of the chain.Phases on other links can be treated in a harmonic approximation
For d>1 we have to include transverse directions. Need to excite many chains to create a phase slip
The transverse size of the phase slip diverges near a phase slip. We can use continuum approximation to treat transverse directions
|| cos ,J J p
J J
Longitudinal stiffness is much smaller than the transverse.
SF MI
p
U/J
Weakly interacting systems. Gross-Pitaevskii regime.Decay of current by quantum tunneling
Quantum phase slips are strongly suppressed in the GP regime
Fallani et al., PRL (04)
This state becomes unstable at corresponding to the
maximum of the current:
13cp
2 2 21 .I p p p
Close to a SF-Mott transition we can use an effective relativistivc GL theory (Altman, Auerbach, 2004)
Strongly interacting regime. Vicinity of the SF-Mott transition
SF MI
p
U/J
Metastable current carrying state:2 21 ip xp e
Strong broadening of the phase transition in d=1 and d=2
is discontinuous at the transition. Phase slips are not important.Sharp phase transition
- correlation length
SF MI
p
U/J
Strongly interacting regime. Vicinity of the SF-Mott transitionDecay of current by quantum tunneling
Action of a quantum phase slip in d=1,2,3
Decay of current by quantum tunneling
0.0
0.1
0.2
0.3
0.4
0.5
0.0 0.2 0.4 0.6 0.8 1.0
d=3
d=2
d=1
unstable
stable
U/Uc
p/
Decay of current by thermal activationp
hase
j
Escape from metastable state by thermal activation
pha
se
j
Thermalphase slip
E
Thermally activated current decay. Weakly interacting regime
E
Activation energy in d=1,2,3
Thermal fluctuations lead to rapid decay of currents
Crossover from thermal to quantum tunneling
Thermalphase slip
Phys. Rev. Lett. (2004)
Decay of current by thermal fluctuations
Dynamics of interacting bosonic systemsprobed in interference experiments
Interference of two independent condensates
Andrews et al., Science 275:637 (1997)
Interference experiments with low d condensates
2D condensates: Hadzibabic et al., Nature 441:1118 (2006)
x
Time of
flight
z
long. imaging
trans.imaging
Longitudial imaging Transverse imaging
1D condensates: Schmiedmayer et al., Nature Physics (2005,2006)
Studying dynamics using interference experiments Motivated by experiments and discussions with
Bloch, Schmiedmayer, Oberthaler, Ketterle, Porto, Thywissen
J
Prepare a system by splitting one condensate
Take to the regime of finiteor zero tunneling Measure time evolution
of fringe amplitudes
Studying coherent dynamics of strongly interacting systemsin interference experiments
Coupled 1d systems
J
Interactions lead to phase fluctuations within individual condensates
Tunneling favors aligning of the two phases
Interference experiments measure only the relative phase
Coupled 1d systems
J
Relative phase Particle number imbalance
Conjugate variables
Small K corresponds to strong quantum fluctuations
Quantum Sine-Gordon model
Quantum Sine-Gordon model is exactly integrable
Excitations of the quantum Sine-Gordon model
Hamiltonian
Imaginary time action
soliton antisoliton many types of breathers
Dynamics of quantum sine-Gordon model
Hamiltonian formalism
Quantum action in space-time
Initial state
Initial state provides a boundary condition at t=0
Solve as a boundary sine-Gordon model
Boundary sine-Gordon model
Limit enforces boundary condition
Exact solution due to Ghoshal and Zamolodchikov (93)Applications to quantum impurity problem: Fendley, Saleur, Zamolodchikov, Lukyanov,…
Sine-Gordon+ boundary condition in space
quantum impurity problem
Sine-Gordon+ boundary condition in time
two coupled 1d BEC
BoundarySine-GordonModel
space and timeenter equivalently
Initial state is a generalized squeezed state
creates solitons, breathers with rapidity
creates even breathers only
Matrix and are known from the exact solutionof the boundary sine-Gordon model
Time evolution
Boundary sine-Gordon model
Coherence
Matrix elements can be computed using form factor approachSmirnov (1992), Lukyanov (1997)
Quantum Josephson Junction
Initial state
Limit of quantum sine-Gordon model when spatial gradientsare forbidden
Time evolution
Eigenstates of the quantum Jos. junction Hamiltonian are given by Mathieu’s functions
Coherence
E2-E0 E4-E0
E6-E0
powerspectrum
Dynamics of quantum Josephson Junction
Main peak
Smaller peaks
“Higher harmonics”
Power spectrum
Dynamics of quantum sine-Gordon model
Coherence
Main peak
“Higher harmonics”
Smaller peaks
Sharp peaks
Dynamics of quantum sine-Gordon model
powerspectrum
main peak
“higher harmonics”
smaller peaks
sharp peaks (oscillations without decay)
Conclusions
Dynamic instability is continuously connected to thequantum SF-Mott transition. Quantum and thermalfluctuations are important
Interference experiments can be used to do spectroscopy of the quantum sine-Gordon model