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The flux qubit revisited to enhance coherence and reproducibility

  • Nature Communications 7, Article number: 12964 (2016)
  • doi:10.1038/ncomms12964
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Abstract

The scalable application of quantum information science will stand on reproducible and controllable high-coherence quantum bits (qubits). Here, we revisit the design and fabrication of the superconducting flux qubit, achieving a planar device with broad-frequency tunability, strong anharmonicity, high reproducibility and relaxation times in excess of 40 μs at its flux-insensitive point. Qubit relaxation times T1 across 22 qubits are consistently matched with a single model involving resonator loss, ohmic charge noise and 1/f-flux noise, a noise source previously considered primarily in the context of dephasing. We furthermore demonstrate that qubit dephasing at the flux-insensitive point is dominated by residual thermal-photons in the readout resonator. The resulting photon shot noise is mitigated using a dynamical decoupling protocol, resulting in T2≈85 μs, approximately the 2T1 limit. In addition to realizing an improved flux qubit, our results uniquely identify photon shot noise as limiting T2 in contemporary qubits based on transverse qubit–resonator interaction.

Introduction

Over the past 15 years, superconducting qubits have achieved a remarkable five-order-of-magnitude increase in their fundamental coherence metrics, including the energy-decay time T1 , the Ramsey free-induction decay time T2* , and the refocused Hahn-echo decay time T2E. This spectacular trajectory is traceable to two general strategies that improve performance: (1) reducing the level of noise in the qubit environment through materials and fabrication improvements, and (2) reducing the qubit sensitivity to that noise through design advancements1.

The charge qubit evolution is a quintessential example2. Early demonstrations (Cooper-pair box) exhibited nanosecond-scale coherence times3. Since then, operation at noise-insensitive bias points (quantronium)4, the introduction of capacitive shunting (transmon)5, the use of two-dimensional6 and three-dimensional (3D)7 resonators to modify the qubit electromagnetic environment, the development of high-Q capacitor materials and fabrication techniques8,9, and the introduction of alternative capacitor geometries (Xmon)10 have incrementally and collectively raised coherence times to the 10–100 μs range10,11 and beyond12,13. In addition, the capacitive shunt has generally improved device-to-device reproducibility. The trade-off, however, is a significant reduction in the charge qubit intrinsic anharmonicity (that is, the difference in transition frequencies f01 and f12 between qubit states 0, 1 and 1, 2) to 200–300 MHz for contemporary transmons, complicating high-fidelity control and exacerbating frequency crowding in multi-qubit systems14.

In contrast, the performance of the persistent-current flux qubit15,16 has progressed more slowly over the past decade. Device asymmetry was identified early on to limit flux qubit coherence17 and, since 2005, symmetric designs have generally achieved 0.5–5 μs (refs 18, 19) with a singular report of T2E=23 μs ≈2T1 (ref. 20). Despite respectable performance for individual flux qubits, however, device-to-device reproducibility has remained poor. An early attempt at capacitive shunting21 improved reproducibility, but coherence remained limited to 1–6 μs (refs 22, 23). Recently, flux qubits embedded in 3D (ref. 24) and coplanar25 resonators exhibited more reproducible and generally improved relaxation and coherence times: T1=6–20 μs, T2*=2–8 μs. Nonetheless, further improvements in these times and in reproducibility are necessary if the flux qubit is to be a competitive option for quantum information applications.

In this context we revisit the design and fabrication of the flux qubit. Our implementation, a capacitively shunted (C-shunt) flux qubit21 coupled capacitively to a planar transmission-line resonator, exhibits significantly enhanced coherence and reproducibility, while retaining an anharmonicity varying from 500–910 MHz in the four devices with the highest relaxation times. We present a systematic study of 22 qubits of widely varying design parameters—shunt capacitances Csh=9–51 fF and circulating currents Ip=44–275 nA—with lifetimes at the flux-insensitive bias point ranging from T1<1 μs (small Csh, large Ip) to T1=55 μs (large Csh, small Ip). Over this entire range, the measured T1 values are consistent with a single model comprising ohmic charge noise, 1/f-flux noise, and Purcell-enhanced emission into the readout resonator. We furthermore investigated and identified quasiparticles as a likely source of observed T1 temporal variation. For the highest coherence devices, the Hahn-echo decay time T2E=40 μs<2T1 does not reach the 2T1 limit, as is also often observed with transmons coupled transversally to resonators7,10,26. We demonstrate that this is due to dephasing caused by the shot noise of residual photons in the resonator (mean photon number ), observing a lorentzian noise spectrum with a cutoff frequency consistent with the resonator decay rate. We then use Carr–Purcell–Meiboom–Gill (CPMG) dynamical decoupling to recover T2CPMG≈2T1 in a manner consistent with the measured noise spectrum.

Results

C-shunt flux qubit

Our circuits each contain two C-shunt flux qubits—with different frequencies—placed at opposite ends of a half-wavelength superconducting coplanar waveguide resonator (Fig. 1a). The resonator, ground plane and capacitors (Fig. 1b) were patterned from MBE-grown aluminium deposited on an annealed sapphire substrate8 (Supplementary Note 1). We used both square capacitors (Fig. 1b) and interdigital capacitors (IDCs, not shown) coupled capacitively to the centre trace of the coplanar waveguide resonator to enable qubit control and readout. In a second fabrication step, the qubit loop and its three Josephson junctions (Fig. 1c) were deposited using double-angle, electron-beam, shadow evaporation of aluminium. One junction is smaller in area (critical current) by a factor α, and each of its leads contacts one electrode of the shunt capacitor. An equivalent circuit is illustrated in Fig. 1d (Supplementary Note 2).

Figure 1: C-shunt flux qubit.
Figure 1

(a) Optical micrograph of the 2.5 × 5.0 mm2 chip, aluminium (black) on sapphire substrate (white, where the aluminium has been etched away), featuring two qubits (A and B) and a λ/2 coplanar waveguide resonator (ωr/2π=8.27 GHz). Scale bar, 0.5 mm. (b) SEM image of the shunt capacitor (Csh,A=51 fF) for qubit A. Each square plate of the capacitor is 200 × 200 μm2. The lower plate capacitively couples the qubit to the λ/2 resonator. Scale bar, 50 μm. (c) Magnified view of the shadow-evaporated qubit loop and its three Josephson junctions. The left junction area is smaller by a factor αA=0.42. Scale bar, 1 μm. (d) Device and measurement schematic. Experiments are performed in a dilution refrigerator at 20 mK. A global magnetic field B provides a magnetic flux bias Φb to each qubit. A qubit drive tone (ωd), readout tone (ωro) and externally generated noise (Padd, see Figs 5 and 6) enter the λ/2 resonator defined by capacitances Cin and Cout. The resonator is capacitively coupled (Cg,A/B) to qubits A and B. The qubit junctions (‘x’) have internal capacitance, CJ,A/B and αA/BCJ,A/B, and are externally shunted by capacitance Csh,A/B. Each qubit loop supports a circulating persistent current Ip,A/B. Readout signals at the resonator output pass three isolators (‘→’), are amplified at cryogenic and room temperatures, and subsequently detected. See supplementary online material for more information.

Varying the qubit design enables us to explore a range of qubit susceptibilities to flux and charge noise with impact on both T1 and T2 (ref. 21). Compared with the conventional persistent-current flux qubit15,16, our best C-shunt flux qubits have two key design enhancements. First, a smaller circulating current—achieved by reducing the area and critical current density of the Josephson junctions (Fig. 1c)—reduces the qubit sensitivity to flux noise, a dominant source of decoherence in flux qubits. Second, a larger effective junction capacitance—achieved by capacitively shunting the small junction (Fig. 1b)—reduces the qubit sensitivity to charge noise, and improves device reproducibility by reducing the impact of both junction fabrication variation and unwanted stray capacitance. Furthermore, the use of high-quality fabrication techniques and physically large shunt capacitors reduces the density and electric participation of defects at the various metal and substrate interfaces1.

The system is operated in the dispersive regime of circuit quantum electrodynamics and is described by the approximate Hamiltonian27

where, the three terms are respectively the qubit (represented as a two-level system), resonator and qubit–resonator interaction Hamiltonians, is the Pauli operator defined by the qubit energy eigenbasis, ωr is the resonator angular frequency and is the resonator photon-number operator. The qubit angular frequency ωqb) is set by the magnetic flux bias Φb, measured relative to an applied flux (m+1/2)Φ0 where m is an integer and Φ0 is the superconducting flux quantum, and attains its minimum value ωq(0)≡Δ at the flux-insensitive point Φb=0. The quantity χb) is the qubit-state-dependent dispersive shift of the resonator frequency, which is used for qubit readout. In the Supplementary Notes 3–5, we discuss further the two-level system approximation for the C-shunt flux qubit, an approximate analytic treatment which goes beyond equation (1), and the numerical simulation of the full qubit–resonator Hamiltonian used to make quantitative comparisons with our data.

T 1 relaxation and noise modelling

We begin by presenting the T1 characterization protocol for the device in Fig. 1. We first identify the resonator transmission spectrum (Fig. 2a) by scanning the readout-pulse frequency ωro about the bare resonator frequency ωr/2π≈8.27 GHz. Using standard circuit quantum electrodynamics readout, qubit-state discrimination is achieved by monitoring the qubit-state-dependent transmission through the resonator27. Next, we add a qubit driving pulse of sufficient duration to saturate the ground-to-excited-state transition and sweep the pulse frequency ωd (Fig. 2b). The resulting spectra for qubits A and B (Fig. 1a) exhibit minima ΔA/2π≈4.4 GHz and ΔB/2π≈4.7 GHz at the qubit flux-insensitive points and increase with magnetic flux (bias current) away from these points. Finally, using a single π-pulse to invert the qubit population, we measure the T1 relaxation of qubit A (T1=44 μs) and qubit B (T1=55 μs) at their flux-insensitive points (Fig. 2c). High-power spectroscopy (see Supplementary Note 6) reveals transitions among the first four qubit energy levels that are well matched by simulation, and identifies anharmonicities of 500 MHz in the two measured devices.

Figure 2: Spectroscopy and T1 of two capacitively shunted flux qubits.
Figure 2

(a,b) Resonator and qubit spectra versus bias current used to induce the global magnetic field B. The qubit transition frequencies ωq/2π have minima ΔA/2π=4.36 GHz and ΔB/2π=4.70 GHz at the qubit flux-insensitive points, which are intentionally offset in bias current (magnetic flux) by using different qubit-loop areas. (c) Energy-decay functions of qubits A and B measured at their respective degeneracy points using the inversion-recovery pulse sequence (inset). Solid lines are exponential fits with decay constant T1.

Using this protocol, we investigated 22 C-shunt flux qubits from five wafers (fabrication runs), spanning a range of capacitance values (Csh=9–51 fF) and qubit persistent currents (Ip=44–275 nA) and featuring two capacitor geometries (interdigital and square). The junction critical currents were adjusted to maintain Δ/2π≈0.5–5 GHz (see Supplementary Note 7).

The data were analysed using simulations of the full system Hamiltonian and a Fermi’s golden rule expression for the exited state decay rate21,

where |g〉(|e〉) indicates the qubit ground (excited) states, and the sum is over four decay mechanisms: flux noise in the qubit loop, charge noise on the superconducting islands, Purcell-enhanced emission to the resonator mode, and inelastic quasiparticle tunnelling through each of the three junctions. The operator is a transition dipole moment, and Sλ(ωq) is the symmetrized noise power spectral density for the fluctuations which couple to it. For example, is a loop current operator for flux noise SΦ(ω), and is an island voltage operator for charge noise SQ(ω) (Supplementary Notes 8 and 9).

We considered both Sλ(ω)1/ωγ (inverse-frequency noise) and Sλ(ω)ω (ohmic noise)—the two archetypal functional forms of noise in superconducting qubits20,28,29,30,31,32,33—for our magnetic flux and charge noise models, and used the frequency dependence of T1 for specifically designed devices to distinguish between them. While the following results are presented using symmetrized power spectral densities, we are careful to account for the distinction between classical and quantum noise processes in making this presentation (Supplementary Note 9).

For example, in Fig. 3a, Qubit C (Csh=9 fF) has a large persistent current (Ip=275 nA) and a small qubit frequency (Δc/2π=0.82 GHz), making it highly sensitive to flux noise. Consequently, the measured T1 is predominantly limited by flux noise over a wide frequency range. This T1-trend constrains the flux noise model to the form SΦ)≡AΦ2(2π × 1 Hz)γ over the range 0.82–3 GHz (black dashed line, Fig. 3a). For comparison, the functional form for ohmic flux noise (grey dashed line), scaled to match T1 at Δc/2π=0.82 GHz (green dot), is clearly inconsistent with all other data over this frequency range. The noise parameters AΦ2=(1.4 μΦ0)2/Hz and γ=0.9 used to match the data in Fig. 3a are derived from independent measurements—Ramsey interferometry31 and T noise spectroscopy32 (Supplementary Note 10)—made at much lower frequencies in the context of classical noise related to qubit dephasing (Fig. 3b). These values are commensurate with earlier work on qubits20,31,32,33 and d.c. Superconducting QUantum Interference Devices (SQUIDs)34. The consistency between the magnitude and slope of the flux noise power spectra, spanning more than twelve decades in frequency—millihertz to gigahertz—is remarkable, made even more so by the fact that the data in Fig. 3b were measured with a different device (qubit B, Fig. 3c).

Figure 3: T1 variation with qubit frequency and noise modelling.
Figure 3

(a) Energy-relaxation time T1 versus qubit frequency for Qubit C (Csh,C=9 fF, Ip,C=275 nA, Δc/2π=0.82 GHz) plotted with simulated T1 values for individual (dashed lines) and aggregate (solid line) charge, flux and Purcell noise mechanisms. Absence of data around 4 GHz is related to an ancillary qubit level crossing the readout resonator, prohibiting qubit readout and is not a systematic issue. Qubit C is limited by flux noise below about 4.5 GHz. For comparison, the functional form for ohmic flux noise (grey dotted line) is incompatible with the data below 3 GHz; above 3 GHz, its role cannot be readily distinguished from charge noise (see text). Shaded region indicates the range of predicted T1 in the presence of 0–1.0 quasiparticles. (b) Flux noise spectroscopy performed on Qubit B using Ramsey interferometry (red) and T1ρ spin-locking (blue) to determine parameters AΦ2=(1.4 μΦ0)2/Hz and γ =0.9 for the inverse-frequency flux noise (black dashed line) for qubit C (a). Green and black dots: inferred ohmic flux noise SΦ based on measured T1 in a. (c) Energy-relaxation time T1 versus qubit frequency for qubit B (Csh,B=51 fF, Ip,B=49 nA, ). T1 is sensitive predominantly to ohmic charge noise within 5–6.5 GHz range. Scatter in T1 is attributed to quasiparticle fluctuations. Cluster of lower T1 values near 5.5 GHz is due to interaction with the f12 transition. Shaded region indicates the range of predicted T1 in the presence of 0–1.0 quasiparticles. (d) T1 values for 22 qubits with widely varying design parameters, measured at their degeneracy points and plotted against predicted T1 values (dashed line) determined from numerical simulations using a single model with fixed noise levels (see main text). Practically indistinguishable data points (eight in total) are indicated with arrows.

In contrast, Qubit B (Csh=51 fF) has a much smaller persistent current (Ip=49 nA) and larger qubit frequency (ΔB/2π=4.7 GHz). Its value of T1 is most strongly influencedby charge noise (magenta dashed line, Fig. 3c) in the 5.0–6.5 GHz range, consistent with an ohmic charge noise model of the form SQ(ω)≡AQ2ω/(2π × 1 GHz) with the parameter AQ2=(5.2 × 10−9e)2/Hz adjusted to match the data. In addition to flux and charge noise, the predicted value of T1 due to Purcell loss (light blue dashed line) is also included in Fig. 3a,c and involves no free parameters (see Supplementary Note 8). The resulting net value of T1 due to all three mechanisms (inverse-frequency flux noise, ohmic charge noise and Purcell loss) is indicated with a red solid line and is in relatively good agreement with the ceiling of measured T1 values. As we describe below, quasiparticles are responsible for reducing the T1 below this ceiling.

Using these models, Fig. 3d shows a comparison of the measured and predicted T1 values for all 22 qubits. The flux noise model (from Fig. 3a,b) is applied to all qubits, and the Purcell loss is included with no free parameters. For the charge noise model, to achieve agreement across all devices, it was necessary to use AQ,SQ2=(5.2 × 10−9e)2/Hz for square capacitors (from Fig. 3b) and AQ,IDC2=(11.0 × 10−9e)2/Hz for IDCs, presumably reflecting the larger electric participation of the surface and interface defects for the IDC geometry1. The agreement is noteworthy, given that these qubits span a wide range of designs across five fabrication runs (see Supplementary Note 7).

We note that inverse-frequency charge noise was incompatible with these data over the entire frequency range investigated (not shown), implying that the cross-over between inverse-frequency and ohmic charge noise occurred at a frequency below 0.82 GHz. However, while ohmic flux noise SΦ(ω)ω was inconsistent with T1 over the frequency range 0.82–3 GHz, its functional form is plausibly consistent with data above 3 GHz when appropriately scaled (upper dashed grey line, Fig. 3a) and, therefore, cannot be conclusively distinguished from ohmic charge noise. Although the best agreement across all 22 qubits (Fig. 3d) did not require ohmic flux noise, we could not rule out its presence in the 3–7 GHz range. In Supplementary Note 11, we compare models that use ohmic charge noise (as in Fig. 3) and ohmic flux noise. Differentiating between such charge and flux noise at higher frequencies will be the subject of future work. Indeed, for both ohmic flux noise SΦ(ω)ω and inverse-frequency charge noise SQ(ω)1/ω, it is certainly possible (even expected) that the former (latter) dominates the flux (charge) noise at sufficiently higher (lower) frequencies.

The measured data for qubit B (Fig. 3c) exhibit fluctuations in the range T1=20–60 μs for qubit frequencies ωq/2π=4.7–6.5 GHz. To investigate their temporal nature, we measured T1 repeatedly at the qubit flux-insensitive point over a 10-h period and collected the data into sets of 50 individual decay traces. Fig. 4a,b show the results of two such experiments, with set 2 being taken 17 h after set 1. The average of all traces from set 1 exhibits a purely exponential decay, whereas the corresponding average for set 2 exhibits a faster short-time decay and clear non-exponential behaviour (Fig. 4a). Histograms of the T1 values for individual traces exhibit a tight, Gaussian-shaped distribution centred at 55 μs for set 1 and a broader, quasi-uniform distribution centred near 45 μs for set 2. Over the course of several weeks, we observed transitions between these two characteristic modes of behaviour every few days for this device35.

Figure 4: T1 temporal variation and quasiparticles.
Figure 4

(a) Energy-relaxation measurements (set 1 and set 2) at ωqB for qubit B. Each set comprises the average of 50 individual decay traces acquired sequentially in 4-min intervals. Set 1 exhibits purely exponential decay with T1=55 μs, whereas set 2 (acquired 17 h after set 1) exhibits a non-exponential decay function. The black line is a fit to equation (3) assuming the non-exponential decay is due to quasiparticle fluctuations (see text). Inset: tabulation of the values obtained from fitting functions. The ‘*’ indicates an assumed value from set 2 (not a fit value). (b) Histograms of T1 values obtained by exponential fits of the individual traces forming the two data sets in a. For set 2, the fitting is restricted to the first 40 μs to capture primarily the fast initial decay. (c) Energy-relaxation measurements at ωqC for qubit C. The exponential decay function is manifest as a linear fit on the log plot with time constant T1=0.49 μs. (d) Histograms of T1 values obtained from repeated measurements of qubit C. Both the exponential decay function (c) and the consistently tight T1 distribution (d) indicate a relative insensitivity to quasiparticle number fluctuations.

We attribute the temporal fluctuations and non-exponential decay function to excess quasiparticles—above the thermal equilibrium distribution—near the qubit junctions36,37,38,39. Following ref. 40, we define as the average relaxation time associated with a single quasiparticle and take the quasiparticle number nqp to be Poisson-distributed with mean value . This results in a qubit polarization decay function,

where T1R captures the residual exponential decay time in the absence of quasiparticles . The non-exponential decay function observed for set 2 is well described by equation (3) (black line in Fig. 4a) with fitting parameters , and T1R=60 μs.

We use a quantum treatment of quasiparticle tunnelling to model the impact of single quasiparticles on the T1 of qubit B (Supplementary Note 8). Using a quasiparticle density xqp=4 × 10−7 (per superconducting electron), the calculated recovers the fitted value μs at the flux-insensitive point. Both and xqp are comparable to the quasiparticle-induced relaxation rates and quasiparticle density reported for similar devices24,41. The shaded region in Fig. 3a,c indicates the range of predicted T1 in the presence of quasiparticle. Most T1 data lie within this region, supporting the hypothesis that their scatter (particularly for qubit B in Fig. 3c) and the observed temporal T1 variation (Fig. 4b) arise from the common mechanism of quasiparticle tunnelling. In addition, the residual relaxation time T1R for set 2 is similar to the exponential time constant obtained for set 1, indicating an underlying consistency in the noise models between the two data sets in the absence of quasiparticles. Unlike qubit B, qubit C consistently exhibited an exponential decay function (Fig. 4c) with little temporal variation (Figs 3a and 4d), indicating that quasiparticles did not strongly influence this device.

The results of Figs 3 and 4 demonstrate clearly that 1/f-type flux noise is the dominant source of qubit relaxation for frequencies below 3 GHz. To further strengthen this claim, it is instructive to compare relaxation times for qubits with similar frequencies and shunting capacitances, but where the persistent current (and thereby the sensitivity to flux noise) differs. We find that by reducing Ip from 170 nA to 60 nA, we improve the measured T1 from 2.3 to 12 μs (see qubits 11 and 13 in Supplementary Table 1 in Supplementary Note 7).

Pure dephasing and thermal-photon noise

We now address the transverse relaxation time T2 and our ability to refocus coherent dephasing errors. Efficient refocusing implies that T2 is limited entirely by T1, since 1/T2=1/2T1+1/Tϕ, where Tϕ is the dephasing time. Generally, T2 is maximal at the flux-insensitive point for conventional flux qubits18,19,20, and the device reported in ref. 20 was efficiently refocused with a single echo pulse (T2E=23 μs≈2T1). In the current work, however, a single refocusing pulse is no longer completely efficient (T2E<2T1). This suggests that an additional, higher-frequency noise channel has been introduced. Unlike the device in ref. 20, which was coupled to a d.c. SQUID for readout, our C-shunt flux qubits are transversally coupled to a resonator (Fig. 1). Such inefficient refocusing is also reported for transmons similarly coupled to resonators7,10,26.

As we show below, the main source of dephasing in C-shunt flux qubits biased at their flux-insensitive point is photon-number fluctuations (shot noise) in the resonator, which vary the qubit frequency via the a.c. Stark effect (as in the transmon case26,27). Given a small thermal-photon population <<1 in the resonator (see Supplementary Note 12), the photon-induced frequency shift ΔStarkth and dephasing rate of the qubit are42

The factor η=κ2/(κ2+4χ2) effectively scales the photon population seen by the qubit due to the interplay between the qubit-induced dispersive shift of the resonator frequency χ and the resonator decay rate κ. Both the strong dispersive (2χ>>κ) and weak dispersive (2χ<<κ) regimes have been previously addressed26,43,44. Here, we use qubit B to focus primarily on the intermediate dispersive regime (2χ/2π=0.9 MHz, κ/2π=1.5 MHz, see Fig. 5a) relevant for high-fidelity qubit readout45.

Figure 5: Calibration of engineered noise.
Figure 5

(a) Resonator transmission spectra measured with the qubit prepared in the ground and excited states. In contrast to typical transmon qubits with ωq<ωr, an excited-state C-shunt flux qubit shifts the resonator to higher frequencies because of interactions with higher-level qubit transitions. (b) Engineered thermal-photon noise source. A coherent tone near the resonator frequency is mixed with white-noise of nominally equal power from two independent arbitrary waveform generators (AWGs) applied to the in-phase (I) and quadrature (Q) ports of the I/Q mixer. The AWG noise bandwidth (80 MHz) is much greater than the cavity linewidth, creating effectively a thermal-photon noise source with power Padd. (c) Qubit spectral line shape (dots) and lorentzian fits (solid lines) for various added noise powers Padd. The equivalent photon population added to the resonator is derived from d. The blue trace corresponds to no added noise from the source in b. (d) Stark-shifted qubit frequency versus applied noise power (dots). Coloured dots correspond to traces in c. Combining the linear fit (solid line) with the first-order dependence of Stark shift on photon population (equation (4)) yields the power-per-added-photon in the low-power limit. Inset: wider range of applied noise powers; dashed box indicates the range in the main panel. At large photon populations the frequency shift becomes nonlinear, following equation 43 in ref. 40 (solid line). (e) Spin-echo decay (dots) with exponential fit (solid lines) for several values of added photons. Inset: spin-echo pulse sequence. (f) Spin-echo pure-dephasing rate (echo decay rate without the T1 contribution) plotted versus injected photon population (dots). The linear fit (solid line) has slope , in agreement with the value of 2.5 × 106 s−1 calculated from equation (5). The intercept indicates a residual photon population in the resonator.

We begin by intentionally injecting additional thermal-photons into the resonator from an external noise generator with power Padd (Fig. 5b and Supplementary Note 2). In the small- limit, the measured qubit spectrum exhibits a linear relationship between the effective qubit frequency and the generator power Padd (Fig. 5c,d). For completeness, we have included the Lamb shift ΔLamb, a fixed frequency offset due to the resonator zero-point energy. Combining the extracted slope with equation (4), we calibrate the dependence of the added-photon population (in the resonator) on the generator power Padd.

Next, we measure the Hahn-echo dephasing rate for several photon populations using the calibrated . All echo traces (Fig. 5e) feature exponential decay rates Γ2E=1/T2E, indicating little (if any) impact from 1/f noise (charge, flux and so on) and consistent with photon shot noise featuring a short correlation time 1/κ<<T2E. The extracted pure dephasing rate scales linearly with photon population (Fig. 5f). The extracted slope agrees with equation (5) to within 5%. The non-zero dephasing rate at corresponds to a residual photon population , equivalent to an effective temperature Teff=80 mK. By comparison, the qubit effective temperature determined from its first excited-state population is 35 mK (ref. 13).

To confirm that the noise arises from residual thermal-photons, we directly measure the noise power spectral density (PSD) using the T1ρ (spin-locking) method32. This method (inset Fig. 6a) collinearly drives the qubit along the y-axis with a long Y pulse, which ‘locks’ the qubit state in the rotating frame. Measuring the qubit relaxation rate in the rotating frame, Γ1ρRabi)=SzRabi)/2+Γ1/2, effectively samples the noise PSD Sz(ω) seen by the qubit at the locking (Rabi) frequency ΩRabi (see Supplementary Note 10). By varying the locking drive amplitude, which is proportional to ΩRabi, we sample the noise spectrum over the range ω/2π=0.1–100 MHz (Fig. 6a). Below 10 MHz, the resolved noise spectra for all (including ) have similar shapes: flat (white) at low frequencies with a 3-dB high-frequency cutoff at the resonator decay rate ω=κ. This form is consistent with the expected lorenzian PSD for thermal-photons in a resonator as seen by the qubit (see Supplementary Note 10),

Figure 6: PSD of photon fluctuations in the resonator.
Figure 6

(a) Noise power spectral densities (PSDs) extracted from spin-locking (T1ρ) relaxation experiments (Inset, top-left: T1ρ pulse sequence) measured for different locking (Rabi) frequencies (0.1–100 MHz) and added noise photons . Coloured dashed lines indicate expected lorentzian noise spectra (see equation (6)) assuming a constant white-noise offset. The vertical grey line indicates the 3-dB point of the lorentzians, coinciding with the resonator decay rate κ/2π=1.5 MHz. Inset, bottom-left: T1ρ decay traces for different photon populations at fixed locking (Rabi) frequency ω/2πR/2π=500 kHz. Inset, top-right: T1ρ decay traces at different locking (Rabi) frequencies for nadd=0.115. (b) Decay times T2CPMG for the CPMG sequence measured versus number of π-pulses, Nπ, with nadd=0 (no added noise photons). The CPMG pulse sequence (inset) acts as a bandpass noise filter centred at a frequency proportional to Nπ through the pulse spacing Δτ (see main text). At Nπ=200, the filter frequency approximately equals the cavity decay rate (dashed line). For Nπ<200, the filter samples the flat low-frequency portion of the lorentzian PSD, yielding a constant decay time T2CPMG≈40 μs. For Nπ>200, the filter traverses the roll-off region of the lorentzian. As the sampled noise decreases, the decay times increase, approaching the limit set by energy relaxation (T2CPMG≈2T1) for Nπ>1,000. Error bars indicate 95% confidence intervals on the fitting algorithm used to extract these data.

which includes the dispersive coupling χ and the filtering factor η [see equations (4 and 5)]. Equation (6) agrees with the measured PSDs for all photon populations , with the residual photon number extracted from equation (6). This agreement eliminates the driving or readout field as the source of the residual photons, because such coherent-state photons follow Poisson statistics with a resulting cutoff frequency κ/2 (half the observed value)46,47.

Finally, we apply dynamical decoupling techniques to validate the functional form of the measured noise PSD and to recover T2≈2T1. We use the CPMG (inset Fig. 6b) pulse sequence, comprising a number Nπ of equally spaced π-pulses. The application of π-pulses in the time domain can be viewed as a bandpass filter in the frequency domain which shapes the noise spectra seen by the qubit21,48,49,50. Since the filter passband is centred at a frequency inversely related to the temporal spacing Δτ between adjacent pulses, increasing Nπ for a fixed sequence length will shift this passband to higher frequencies (see Supplementary Note 13).

Figure 6b shows the measured CPMG decay time T2CPMG versus π-pulse number Nπ with no added noise . From Nπ=1 (Hahn-echo) to Nπ=100, the decay time T2CPMG remains near 40 μs, consistent with the white-noise (flat) portion of the noise PSD in Fig. 6a. Above Nπ=100, the passband frequency traverses the cutoff region of the PSD and, as the integrated noise level decreases, T2CPMG rises. For Nπ>1,000, the refocusing becomes efficient with . The close correspondence between the noise spectral density in Fig. 6a and the mitigation of that noise by CPMG in Fig. 6b strongly supports our methods and interpretations.

Discussion

The C-shunt flux qubit is a planar device with broad-frequency tunability, relatively strong anharmonicity and high reproducibility, making it well suited to both gate-based quantum computing and quantum annealing. The anharmonicity can be significantly higher than that of transmon qubits, allowing for faster (even subnanosecond51,52) control pulses and reduced frequency crowding in multi-qubit systems. The addition of a high-quality-factor shunt capacitance to the flux qubit, together with a reduced qubit persistent current, has enabled us to achieve values of T1 as high as 55 μs at the qubit flux-insensitive point. We are able to account for measured T1 values across 22 qubits with a single model involving ohmic charge noise, 1/f-flux noise, and the Purcell effect, with temporal variation in T1 explained by quasiparticle tunnelling. On the basis of this model, we anticipate further design optimization leading to even higher coherence will be possible. Finally, we used spin-locking to directly measure the photon shot noise spectral density, and we verified its functional form using a CPMG pulse sequence to reach a T2 of 85 μs—limited by 2T1—at the flux-insensitive point. These measurements identify photon shot noise as the dominant source of the observed dephasing, and have direct implications for any qubit in which the readout involves its transverse coupling to a resonator.

The role of high-frequency 1/f-flux noise in qubit relaxation is intriguing. Our T1 data and their frequency dependence across 22 different qubits strongly support the conclusion that 1/f-flux noise contributes to qubit relaxation up to at least 3 GHz in our devices. Above 3 GHz, there is some ambiguity between ohmic flux and ohmic charge noise, and clarifying the roles of these respective noise sources is the subject of future work. A detailed understanding of such a broadband 1/f-flux noise mechanism and its transition from classical to quantum behaviour is of great practical interest and awaits theoretical explanation.

Data availability

The data that support the findings of this study may be made available from the corresponding author upon request and with the permission of the US Government sponsors who funded the work.

Additional information

How to cite this article: Yan, F. et al. The flux qubit revisited to enhance coherence and reproducibility. Nat. Commun. 7, 12964 doi: 10.1038/ncomms12964 (2016).

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Acknowledgements

We gratefully acknowledge A. Blais, A. Clerk, and Y. Nakamura for useful discussions and P. Baldo, V. Bolkhovsky, G. Fitch, P. Murphy, B. Osadchy, K. Magoon, R. Slattery and T. Weir at MIT Lincoln Laboratory for technical assistance. This research was funded in part by the Office of the Director of National Intelligence (ODNI), Intelligence Advanced Research Projects Activity (IARPA) and by the Assistant Secretary of Defense for Research & Engineering via MIT Lincoln Laboratory under Air Force Contract No. FA8721-05-C-0002; by the U.S. Army Research Office Grant No. W911NF-14-1-0682; and by the National Science Foundation Grant No. PHY-1415514. The views and conclusions contained herein are those of the authors and should not be interpreted as necessarily representing the official policies or endorsements, either expressed or implied, of ODNI, IARPA or the US Government.

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Affiliations

  1. Research Laboratory for Electronics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

    • Fei Yan
    • , Simon Gustavsson
    • , Archana Kamal
    • , Terry P. Orlando
    •  & William D. Oliver
  2. Department of Physics, University of California, Berkeley, California 94720-7300, USA

    • Jeffrey Birenbaum
    •  & John Clarke
  3. MIT Lincoln Laboratory, Quantum Information and Integrated Nanosystems Group, 244 Wood Street, Lexington, Massachusetts 02420, USA

    • Adam P Sears
    • , David Hover
    • , Ted J. Gudmundsen
    • , Danna Rosenberg
    • , Gabriel Samach
    • , S Weber
    • , Jonilyn L. Yoder
    • , Andrew J. Kerman
    •  & William D. Oliver
  4. Department of Electrical Engineering and Computer Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

    • Terry P. Orlando
  5. Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

    • William D. Oliver

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Contributions

F.Y., A.K., S.G., J.B., A.P.S. and D.H. performed the experiments. S.G., A.P.S., A.K., D.H., A.J.K. and W.D.O. designed the devices.T.J.G., J.L.Y. and J.B. fabricated the devices. A.J.K., S.G., F.Y., D.H., D.R., G.S., S.W. performed device simulations. S.G., T.P.O., J.C., A.J.K. and W.D.O. supervised the project. All authors contributed to the conception, execution and interpretation of the experiments.

Competing interests

The authors declare no competing financial interests.

Corresponding author

Correspondence to William D. Oliver.

Supplementary information

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    Supplementary Information

    Supplementary Figures 1-11, Supplementary Table 1, Supplementary Notes 1-13 and Supplementary References.

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