. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Anderson localization and Mott insulator phase in the time domain
Krzysztof Sacha
Marian Smoluchowski Institute of Physics, Jagiellonian University in Krak´
- w
Anderson localization and Mott insulator phase in the time domain - - PowerPoint PPT Presentation
Anderson localization and Mott insulator phase in the time domain Krzysztof Sacha Marian Smoluchowski Institute of Physics, Jagiellonian University in Krak ow . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Eigenstates of a time-independent Hamiltonian H are also eigenstates of a time translation operator e−iHt
KS, PRA 91, 033617 (2015).
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Floquet Hamiltonian HF (t) = − 1 2 ∂2 ∂z2 + z + λz cos(2πt/T) − i ∂ ∂t HF ψn(z, t) = En ψn(z, t) En – quasi-energy ψn(z, t) – time periodic function
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Floquet Hamiltonian HF (t) = − 1 2 ∂2 ∂z2 + z + λz cos(2πt/T) − i ∂ ∂t HF ψn(z, t) = En ψn(z, t) En – quasi-energy ψn(z, t) – time periodic function
2 : 1 resonance λ = 0.06, T = 5.7
0,3 0,3 0,3
probability density
0,3 10 20
z
0,3 10 20
z
t=0 0.1T 0.2T 0.3T 0.5T 0.7T T 0.4T 0.6T 0.8T
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
In the s : 1 resonance case:
These quasi-energies form a band when s → ∞.
For s → ∞, the wavepackets φj (z, t) become analogues of Wannier states but in the time domain.
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
In the s : 1 resonance case:
These quasi-energies form a band when s → ∞.
For s → ∞, the wavepackets φj (z, t) become analogues of Wannier states but in the time domain. Example for s = 4:
30 60 90 120
z
0,05 0,1
probability density
t=0.25T
1 2 3 4
t=0.3T
1 2 3 4
t / T
0,2 0,4 0,6
probability density
z=121
1 2 3 4
Restricting to the Hilbert subspace ψ =
s
∑
j=1
aj φj , EF =
sT
∫ dt⟨ψ|HF |ψ⟩ ≈ − J 2
s
∑
j=1
(a∗
j+1aj + c.c.)
J = −2
sT
∫ dt⟨φj+1|HF |φj ⟩ The lowest and higher quasi-energy bands can be considered.
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
s
j=1
j+1aj + c.c.) + s
j=1
with εj =
sT
∫ dt⟨φj |H′(t)|φj ⟩, where H′(t) is a perturbation that fluctuates in time but H′(t + sT) = H′(t). Example for s = 4:
1 2 3 4
t / T
10
10
10
10
probability density
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
s
j=1
j+1aj + c.c.) + s
j=1
with εj =
sT
∫ dt⟨φj |H′(t)|φj ⟩, where H′(t) is a perturbation that fluctuates in time but H′(t + sT) = H′(t). Example for s = 4:
1 2 3 4
t / T
10
10
10
10
probability density
space t=const |ψ(z)|
2
L 2L (s-1)L Space Crystal time z=const T 2T (s-1)T |ψ(t)|
2
Time Crystal
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
s
j=1
j+1ˆ
s
i,j=1
with Uij = g0
sT
∫ dt
∞
∫ dz|φi |2 |φj |2, where |Uii | > |Uij | for i ̸= j.
long-time phase coherence is lost. 0 time
T 2T (s-1)T
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
EF = − J 2
s
∑
j=1
(a∗
j+1aj + c.c.) + s
∑
j=1
εj |aj |2 where H′(t) is a perturbation that fluctuates in time but H′(t + sT) = H′(t). H′(t) = z
4
∑
n=1
αn cos { 2π [ n t 4T − sin ( 2π t 4T )]} . εj are chosen randomly, e.g. according to a Lorentzian distribution (Lloyd model), then αn are chosen so that εj =
sT
∫ dt⟨φj |H′(t)|φj ⟩. Example for s = 4:
1 2 3 4
t / T
10
10
10
10
probability density
space t=const |ψ(z)|
2
L 2L (s-1)L Space Crystal time z=const T 2T (s-1)T |ψ(t)|
2
Time Crystal
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .