quantum simulations: from ground to excited states
DESCRIPTION
Quantum Simulations: From Ground to Excited States. AFM. ?. AFM. AFM. Phil Richerme Monroe Group University of Maryland and NIST iQsim Workshop Brighton, UK December 18, 2013. ?. AFM. AFM. AFM. From Ground to Excited States. - PowerPoint PPT PresentationTRANSCRIPT
Quantum Simulations: From Ground to Excited States
Phil RichermeMonroe Group
University of Maryland and NIST
iQsim WorkshopBrighton, UK
December 18, 2013
?AFM
AFM AFM
AFM AFM?
AFM
From Ground to Excited States
Current System: Fully-connected Ising model with d20 spins, for study of:• Ground-state phase diagrams [1]• Quantum phase transitions [2]• Studies of frustration [3,4]
[1] E. E. Edwards et. al., PRB 82, 060412 (2010)[2] R. Islam et. al., Nat. Comm. 2, 377 (2011)[3] K. Kim et. al., Nature 465, 590 (2010)
[4] R. Islam et. al., Science 340, 583 (2013)
From Ground to Excited States
Current System: Fully-connected Ising model with d20 spins, for study of:• Ground-state phase diagrams [1]• Quantum phase transitions [2]• Studies of frustration [3,4]• Quantum fluctuations in a classical system [5]• Many-body Hamiltonian spectroscopy• Correlation propagation after global quenches
This Talk
[4] R. Islam et. al., Science 340, 583 (2013)[5] P. Richerme et. al., PRL 111, 100506 (2013)
[1] E. E. Edwards et. al., PRB 82, 060412 (2010)[2] R. Islam et. al., Nat. Comm. 2, 377 (2011)[3] K. Kim et. al., Nature 465, 590 (2010)
From Ground to Excited States
Current System: Fully-connected Ising model with d20 spins, for study of:• Ground-state phase diagrams [1]• Quantum phase transitions [2]• Studies of frustration [3,4]• Quantum fluctuations in a classical system [5]• Many-body Hamiltonian spectroscopy• Correlation propagation after global quenches• Scaling up the number of interacting spins• Non-equilibrium phase transitions• Studies of dynamics and thermalization
Future Work
[1] E. E. Edwards et. al., PRB 82, 060412 (2010)[2] R. Islam et. al., Nat. Comm. 2, 377 (2011)[3] K. Kim et. al., Nature 465, 590 (2010)
[4] R. Islam et. al., Science 340, 583 (2013)[5] P. Richerme et. al., PRL 111, 100506 (2013)
200m
2S1/2
nHF = 12 642 812 118 Hz + 311B2 Hz/G2
|z = |0,0
|z = |1,0 |1,1|1,-1
171Yb+
2 m
2S1/2
2P1/2
370 nm
12.6 GHz|z
g/2p = 20 MHz
F=1
F=0
F=1
F=0
|z
2.1 GHz
HF
200m
2S1/2
nHF = 12 642 812 118 Hz + 311B2 Hz/G2
|z = |0,0
|z = |1,0 |1,1|1,-1
171Yb+
2 m
2.1 GHz
12.6 GHz2S1/2
2P1/2
370 nm
|z
g/2p = 20 MHz
F=0
F=1
F=0
|zF=1
HF
Generating Spin-Spin Couplings
+HF
Beatnote frequency
Axialmodes
HF
Transversemodes
Axialmodes
Transversemodes
Carrier
μμ
)()(, ˆˆ jx
ix
ji
jieff JH
+HF
||2)( 0
22
2,
jiJbb
mk
Jk k
kj
kijiji
12.6 GHz2S1/2
2P1/2
|z
|z
33 THz
HF
+HF
K. Mølmer and A. Sørensen, PRL 82, 1835 (1999)
+i
itB )(ˆ)(
Studying Frustrated Ground States
+ i
iyy
jx
ix
ji
jixeff tBJH )()()(, ˆ)(ˆˆ
Step 1: Initialize all spins along yx
y
Step 2: Turn on By and Jxi,j and adiabatically lower By
time
By
Jxi,j
ampl
itude
Step 3: Measure all spins along x
>0
AFM ground state order 222 events
Antiferromagnetic Néel order of N=10 spins
441 events out of 2600 = 17% Prob of any state at random =2 x (1/210) = 0.2%
219 events
All in state
All in state
2600 runs, =1.12
Distribution of all 210 = 1024 states
Prob
abili
ty
0 341 682 1023
NominalAFMstate
B = 0
0101010101 1010101010
Prob
abili
ty
0.10
0.08
0.06
0.04
0.02
Initialparamagnetic
state
B >> J
Distribution of all 214 = 16383 states
Prob
abili
ty
0 341 682 1023
NominalAFMstate
B = 0
0101010101 1010101010
Prob
abili
ty
0.10
0.08
0.06
0.04
0.02
Initialparamagnetic
state
B >> J
Most prevalent state should always be the ground state
P. Richerme et. al., PRA 88, 012334 (2013)
14 ions
AFM Ising Model with a Longitudinal Field
So far:
Now:
vary strength of Bx
N/2 classical phase transitions as Bx is increased
+ i
iyy
jx
ix
ji
jix tBJH )()()(, ˆ)(ˆˆ
P. Richerme et. al., PRL 111, 100506 (2013)
++ i
iyy
i
ixx
jx
ix
ji
jix tBBJH )()()()(, ˆ)(ˆˆˆ
Study frustrated ground states of AFM Ising Model
ramp adiabatically
AFM Ising Model with a Longitudinal Field
== P. Richerme et. al., PRL 111, 100506 (2013)
+ i
ixx
jx
ix
ji
jix BJH )()()(, ˆˆˆ
AFM Ising Model with a Longitudinal Field
==
Steps are only present for AFM Ising models with long-range interactions
P. Richerme et. al., PRL 111, 100506 (2013)
+ i
ixx
jx
ix
ji
jix BJH )()()(, ˆˆˆ
AFM Ising Model with a Longitudinal Field
== P. Richerme et. al., PRL 111, 100506 (2013)
+ i
ixx
jx
ix
ji
jix BJH )()()(, ˆˆˆ T = 0
No thermal fluctuations to drive phase transitions
System remains in the same phase
AFM Ising Model with a Longitudinal Field
== P. Richerme et. al., PRL 111, 100506 (2013)
+ i
ixx
jx
ix
ji
jix BJH )()()(, ˆˆˆ T = 0
No thermal fluctuations to drive phase transitions
System remains in the same phase
Add quantum fluctuations to drive the phase transitions
Experimental Protocol
++ i
iyy
i
ixx
jx
ix
ji
jix tBBJH )()()()(, ˆ)(ˆˆˆ
Step 1: Initialize all spins along BBx
By
B
Step 2: Turn on By , Bx , and Jxi,j and adiabatically lower By
time
By
Jxi,j
ampl
itude
Bx
Step 3: Measure all spins along x
P. Richerme et. al., PRL 111, 100506 (2013)
AFM Ising Model with a Longitudinal Field: 6 ions
P. Richerme et. al., PRL 111, 100506 (2013)
010010
AFM Ground States
2-Bright Ground State
1-Bright Ground States
0-Bright Ground State
AFM Ising Model with a Longitudinal Field: 10 ions
0-Bright Ground State
1-Bright Ground States
2-Bright Ground States
3-Bright Ground States
4-Bright Ground States
5-Bright (AFM) Ground States
System exhibits a completedevil's staircase for N → ∞
P. Bak and R. Bruinsma, PRL 49, 249 (1982) P. Richerme et. al., PRL 111, 100506 (2013)
Quantum Fluctuations Drive Phase Transitions
++ i
iyy
i
ixx
jx
ix
ji
jix tBBJH )()()()(, ˆ)(ˆˆˆ
Ramp By
Ramp Bx
+ i
ixx
jx
ix
ji
jix tBJH )()()(, ˆ)(ˆˆ
P. Richerme et. al., PRL 111, 100506 (2013)
No Thermal FluctuationsNo Quantum Fluctuations
No Thermal FluctuationsQuantum Fluctuations
From ground to excited states
• Difficult (impossible?) to calculate excited state behavior for N > 20-30
• Excited states are interesting:• Hamiltonian spectroscopy• Propagation of quantum
correlations• Non-equilibrium phase
transitions• Thermalization
Begin studying excited states of our system
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin
Can drive transitions between states if:
• Matrix element couples the states
• Drive frequency matches energy splitting
01ˆ2 )( i
iy
Experimental Protocol:Step 1: Initialize in FM or AFM state
small perturbation
C. Senko et. al., in preparation
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin
Can drive transitions between states if:
• Matrix element couples the states
• Drive frequency matches energy splitting
01ˆ2 )( i
iy
Experimental Protocol:Step 1: Initialize in FM or AFM state
small perturbation
C. Senko et. al., in preparationAFM
FM
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin
Can drive transitions between states if:
• Matrix element couples the states
• Drive frequency matches energy splitting
01ˆ2 )( i
iy
Experimental Protocol:Step 1: Initialize in FM or AFM stateStep 2: Apply driving field for 3 ms
small perturbation
C. Senko et. al., in preparationAFM
FM
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin
Can drive transitions between states if:
• Matrix element couples the states
• Drive frequency matches energy splitting
01ˆ2 )( i
iy
Experimental Protocol:Step 1: Initialize in FM or AFM stateStep 2: Apply driving field for 3 ms
small perturbation
C. Senko et. al., in preparationAFM
FM
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin
Can drive transitions between states if:
• Matrix element couples the states
• Drive frequency matches energy splitting
01ˆ2 )( i
iy
Experimental Protocol:Step 1: Initialize in FM or AFM stateStep 2: Apply driving field for 3 msStep 3: Scan to find resonances
small perturbation
C. Senko et. al., in preparationAFM
FM
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin
Can drive transitions between states if:
• Matrix element couples the states
• Drive frequency matches energy splitting
01ˆ2 )( i
iy
Experimental Protocol:Step 1: Initialize in FM or AFM stateStep 2: Apply driving field for 3 msStep 3: Scan to find resonances
small perturbation
C. Senko et. al., in preparation
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin
Can drive transitions between states if:
• Matrix element couples the states
• Drive frequency matches energy splitting
01ˆ2 )( i
iy
Experimental Protocol:Step 1: Initialize in FM or AFM stateStep 2: Apply driving field for 3 msStep 3: Scan to find resonances
small perturbation
C. Senko et. al., in preparation
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin small perturbation
Start from AFM states:
From ground to excited states)()(, ˆˆ j
xix
ji
jixJH
+i
iyy tB )(ˆsin small perturbation
Start from FM states:
From ground to excited states – 18 ions
2621430
131071
111111111111111111
From ground to excited states – 18 ions
2621430
131071
2621430
131071
011111111111111111
From ground to excited states – 18 ions
2621430
131071
2621430
131071
011111111111111111
)...
(2
,11,1
3,12,1
NN JJ
JJE
+++
++
Direct Measurement of Spin-Spin Couplings
~N2 terms in Jij matrix, need ~N2 measurements of E
Spectroscopy Method:~N levels for single scan
~N2 levels for ~N scans
)...
(2
,11,1
3,12,1
NN JJ
JJE
+++
++
Probe frequency (kHz) Probe frequency (kHz)
Direct Measurement of Spin-Spin Couplings
~N2 terms in Jij matrix, need ~N2 measurements of E
Spectroscopy Method:~N levels for single scan
~N2 levels for ~N scans
)...
(2
,11,1
3,12,1
NN JJ
JJE
+++
++
Spectroscopy at non-zero transverse field
Spectroscopy at non-zero transverse field
Spectroscopy can measure (or constrain) critical gap
From ground to excited states
Begin studying excited states of our system
• Difficult (impossible?) to calculate excited state behavior for N > 20-30
• Excited states are interesting:• Hamiltonian spectroscopy• Propagation of quantum
correlations• Non-equilibrium phase
transitions• Thermalization
Correlation Propagation with 11 ions
Step 1: Initialize all spins along z
Step 2: Quench to Ising or XY model at t = 0 and let system evolve
Step 3: Measure all spins along z
Step 4: Calculate correlation function
P. Richerme et. al., in preparation
Global Quench: Ising Model
P. Richerme et. al., in preparation
Global Quench: Ising Model
boun
dbo
und
P. Richerme et. al., in preparation
Global Quench: XY Model
Global Quench: XY Model
Scaling Up
4 K Shield
40 K Shield
300 K
To camera
Ion trap
Conclusion
Recent Results:• Quantum fluctuations to drive
classical phase transitions• Spectroscopic method for
Hamiltonian verification• Propagation of correlations after a
global quenchCurrent Pursuits:• Non-equilibrium phase transitions• Thermalization• Larger numbers of ions with a
cryogenic trap
www.iontrap.umd.edu
P.I.Prof. Chris Monroe
PostdocsChenglin CaoTaeyoung ChoiBrian NeyenhuisPhil Richerme
Clayton CrockerShantanu DebnathCaroline FiggattDavid HuculVolkan InlekKale Johnson
JOINTQUANTUMINSTITUTE
Aaron LeeAndrew ManningCrystal SenkoJacob SmithDavid WongKen Wright
Graduate Students Recent AlumniWes CampbellSusan ClarkCharles ConoverEmily EdwardsDavid HayesRajibul IslamKihwan KimSimcha KorenblitJonathan Mizrahi
Theory CollaboratorsJim FreericksBryce Yoshimura
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Geoffrey JiUndergraduate Students