decoherence in flux qubits - umdkosborn/index_files/disq/071206... · 2007. 12. 10. · decoherence...
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Decoherence in flux qubits
Yasunobu Nakamura
NEC Nano Electronics Research LaboratoriesRIKEN Frontier Research SystemCREST-JST
• Measurement of T1, T2 – qubit as a spectrum analyzer• Longer T1 samples• Flux qubit in a cavity
YuriPashkin
AnttiNiskanen
ShenTsai
OlegAstafiev
KhalilHarrabi
MichioWatanabe
TsuyoshiYamamoto
FumikiYoshihara
KazuakiMatsuba
TiefuLi
YasuNakamura
HyunsikIm
FarrukhAbdumalikov
Study of decoherence
= Characterization of environment• Qubit as a tool for investigating its environment
environment
interaction
qubit
tunabletunable
Charge-flux: Cottet 2002, Ithier 2005 (Saclay)Charge: Astafiev 2004 (NEC), Duty 2004 (Chalmers)Flux: Bertet 2005 (Delft), Yoshihara 2006 (NEC), Kakuyanagi 2007 (NTT)Phase: Simmonds 2004, Cooper 2005, Martinis 2005 (NIST/UCSB)
Steffen 2006, Bialczak 2007 (UCSB), Claudon 2006 (Grenoble)
Possible decoherence sources
phonons?
photons?
magnetic-field noise?
charge fluctuations?
paramagnetic/nuclear spins?
trapped vortices?
charge/Josephson-energy fluctuations?
quasiparticletunneling?
environment circuit modes?
Flux qubit: Hamiltonian and energy levels
J.E. Mooij et al. Science 285, 1036 (1999)
0.8 1.0 1.2-100
0
100
Energy (GHz)
γq/πnφ/nφ* nφ*=0.5
Sensitivity to noises
relaxation
dephasing
transverse coupling
longitudinal coupling
nφ-nφ*
Estimation of decoherence time
• EJ-fluctuation can be the largest contribution
4JJ flux qubit @ optimal bias point
preliminaryJ. Koch et al. PRA 76, 042319 (2007)
cf. transmon and CPB
constraints:
Flux qubit: experimental setup
Rabi oscillationsresonant microwave pulse
visibility~79.5%
Energy relaxation
relaxation and excitation
for weak perturbation: Fermi’s golden rule
ex. Johnson noise in ohmic resistor R
spontaneous emission
absorption
zero-point fluctuation of environment
• qubit energy E01 variable• relaxation ∝ S(+E01 ) and excitation ∝ S(-E01 )⇒ quantum spectrum analyzer
U. Gavish et al.R. Aguado and L. KouwenhovenR. Schoelkopf et al.O. Astafiev et al.
T1 vs f: flux bias dependence
80
70
60
50
Switc
hing
pro
babi
lity
(%)
1.61.20.80.40.0Time ( µs)
π ~ 4ns
delay readout pulse
E01 /h (G
Hz)
E01
initialization to ground state is better than 90%⇒ relaxation dominant⇒ classical noise is not important
at qubit frequency ~ 5 GHz
nφ
Γ1 vs E01: qubit energy dependence
• Data from both sides of spectroscopy coincide
• Floor at high-frequency
• Random high-frequency peaks• Broad structure at low frequency
• Depends on SQUID bias pointE01/h (GHz)sample3
E01/h (GHz)sample5
Gamma_1 at different flux bias
Dephasing
free evolution of the qubit phase
dephasing
sensitivity of qubit energy to the fluctuations of external parameter
tunable
information of S(ω) at low frequencies
tunablefor Gaussian fluctuations
Dephasing: T2Ramsey, T2echo measurement
π/2~2ns π/2
t
correspond to detuning
readout pulse
Ramsey interference (free induction decay)
0.01 0.1 1 10 100freq.
0.20.40.60.8
1
thgiew
[1/t]
π/2π ~ 4ns
t/2
readout pulse
π/2~2ns
t/2
spin echo
0.01 0.1 1 10 100freq.
0.20.40.60.8
1
thgiew
[1/t]
Optimal point to minimize dephasing
Ib
nφ• two bias parameters– External flux: nφ=Φex/Φ0
– SQUID bias current Ib
nφ
E01 (GHz)
Ib
G. Burkard et al. PRB 71, 134504 (2005); P. Bertet et al. PRL 95, 257002 (2005).
T1 and T2echo at optimal point nφ=nφ*, Ib=Ib*
T1=545±16ns
Echo decay time is limited by relaxation
Pure dephasing due to high frequency noise (>MHz) is negligible
Echo at nφ≠nφ*, Ib=Ib*
consistent with 1/f flux noise
do not fit
No high-frequency cut-off (soft nor hard)below ~1 MHz
1/f noise cut off dependence
ΓϕRamsey, Γϕecho vs nφ : flux bias dependence
Red lines: fit
For
Flux noise, not charge noise nor critical current noise
F. Yoshihara et al. PRL 97, 167001 (2006)
Dephasing due to photon number fluctuations in SQUID plasma mode
D.I. Schuster et al. PRL 94, 123602 (2005); P. Bertet et al. Phys. Rev. Lett. 95, 257002 (2005).
thermal fluctuation of photon number in resonator ⇒ dephasing of qubit
κ: cavity decay
exponential decay
Red: dephasing due to 1/f flux noisequbit + resonator
1/f flux noise: sample dependence
3 4.58 242.9 11.0 1.63
5 5.08 246.4 9.68 1.406 3.85 229.5 18.7 2.90
11 6.07 232.6 10.1 1.5514 5.45 132 4.9 1.32Loop area ~3 µm2
7±3x10-6 [Φ0] SQUID~2500-160000 µm2 F.C.Wellstood et al. APL50, 772 (1987)1.5x10-6 [Φ0] phase qubit ~10000 µm2 (gradiometer) R.C. Bialczak et al. PRL 99, 187006 (2007)~ 1x10-6 [Φ0] flux qubit ~1000 µm2 (Berkeley, unpublished)~ 1x10-6 [Φ0] flux qubit ~ 25 µm2 K. Kakuyanagi et al. PRL 98, 047004 (2007)
Loop size independent?
Optimal point to minimize dephasing
Ib
nφ• two bias parameters– External flux: nφ=Φex/Φ0
– SQUID bias current Ib
nφ
E01 (GHz)
Ib
G. Burkard et al. PRB 71, 134504 (2005); P. Bertet et al. PRL 95, 257002 (2005).
Γ1, ΓϕRamsey, Γϕecho vs Ib : bias current dependence
relaxation:
Increase |Ib-Ib*| ⇒ selectively introduce Ib noise coupling
F. Yoshihara et al. PRL 97, 167001 (2006).
•exponential decay
dephasing:
•inefficient echo
Yu. Makhlin and A. Shnirman, PRL92, 178301 (2004);G. Burkard et al. PRB71, 134504 (2005).
Summary• T1, T2 measurement in flux qubit, T1,T2echo~ several µs• dependence on flux bias and SQUID-current bias conditions⇒ characterization of environment
Optimal point nφ=nφ*, Ib=Ib*
T1 limited echo decayPure dephasing due to low freq. noise
nφ=nφ*, Ib≠Ib*
‘white’ Ib noise dominant
nφ≠nφ*, Ib=Ib*
1/f flux noise dominant
Open questions: -T1 vs flux bias-residual dephasing at optimal point-origin of 1/f flux noise
Effect of environment circuit design
R-environmentwith large Cshunt
LC-environmentwith less Cshunt
Single qubit 06-06-06 with on-chip LC filter
SQUIDplasmamode
Res
onan
ce in
the
LC
filte
r
Rabi measurements at optimal point
0 1 2 3 4-5
0
5
t(µ s)0 1 2 3 4
-5
0
5
t(µ s)
0 1 2 3 4-5
0
5
t(µ s)0 1 2 3 4
-5
0
5
t(µ s)
0 1 2 3 470
75
80
t(µ s)0 1 2 3 4
80
85
90
t(µ s)
Psw
(%)
strong driving
weak driving
T2Rabi ~ 6 µs(corrected for drift)
Relaxation at optimal point last logs of T1T2 B=opt Ipre=0.311opt2.lvd
0 5 10 15 20 25 3029
30
31
32
33
34
35
36
37
38
time (µ s)
Psw
(%)
T1 = 6.3 µs
Ramsey at optimal point last logs of T1T2 B=opt Ipre=0.311opt2.lvd
0 0.5 1 1.5 2 2.5 331
32
33
34
35
36
37
38
39
time (µ s)
Psw
(%)
T2Ramsey = 2.7 µs
Echo at optimal point last logs of T1T2 B=opt Ipre=0.311opt2.lvd
0 5 10 15 20 25 3031.5
32
32.5
33
33.5
34
34.5
35
35.5
36
time (µ s)
Psw
(%)
T2echo = 3.7 µs
Sample with best coherence
On-chip resistors were replaced by superconducting leads by mistake
∆/h=2.557 GHz, IP=157 nA2.3 µΦ0/Hz1/2 @ 1Hz
A. Abdumalikov, Jr.O. AstafievFlux qubit in a cavity: sample design
Nb – main part of the resonator
Qubit
SOG – isolator, used only for test structures
Al – adjust coupling of the resonator and qubit
Resonator quality factor is defined by the form of this Al island
chip size: 2.5 × 5 mm
Spectroscopy
• Plot shows the change of the phasedip when peak when
Vacuum Rabi splitting
fit:
Relaxation time (continuous measurement)
• measured by sweeping the pulse period– Pulse width was 10 ns
• T1= 0.73 µs – Qubit frequency
E01/h = 8.4 GHz– Coupling to cavity
gsinθ/h = 30 MHz
• E01 dependence
Remarks
•Qubit is powerful tool to analyze its environment
What we have tried and we have been trying
• Flux bias point dependence (nφ*=0.5, 1.5, 2.5; up to 20 Gs)• T1 depends on bias point – coupling to the SQUID is different• T2echo, T2Ramsey are almost independent ~ 20% variation
• Area dependence• 4 times larger qubit – flux noise 3.6 µΦ0/Hz-1/2
• Qubit with small ∆/h~50 MHz• Long T1 ~ 5 ms• Consistent with flux noise contribution• However, does not necessarily mean flux noise contribution
• Spin locking• Temperature dependence of T1• Qubit with variable ∆• Superconducting leads