Photon Shot Noise Dephasing in the Strong-Dispersive Limit of Circuit QED
Abstract
We study the photon shot noise dephasing of a superconducting transmon qubit in the strong-dispersive limit, due to the coupling of the qubit to its readout cavity. As each random arrival or departure of a photon is expected to completely dephase the qubit, we can control the rate at which the qubit experiences dephasing events by varying in situ the cavity mode population and decay rate. This allows us to verify a pure dephasing mechanism that matches theoretical predictions, and in fact explains the increased dephasing seen in recent transmon experiments as a function of cryostat temperature. We investigate photon dynamics in this limit and observe large increases in coherence times as the cavity is decoupled from the environment. Our experiments suggest that the intrinsic coherence of small Josephson junctions, when corrected with a single Hahn echo, is greater than several hundred microseconds.
pacs:
03.67.Lx, 42.50.Pq, 85.25Solid-state superconducting quantum systems offer convenient and powerful platforms for quantum information processing. Rapid progress Houck et al. (2008); Neeley et al. (2008); Steffen et al. (2009) is being made in engineering qubits and effectively isolating them from the surrounding electromagnetic environment. Despite these efforts, the measurement apparatus will always be used to contact the environment and is therefore a potential source for decoherence.
Recently Paik et al. (2011) superconducting qubits have been created inside a three-dimensional (3D) resonator, leading to more than an order of magnitude increase in coherence time. Interestingly, the energy relaxation time has increased even more than the phase coherence time , pointing to a new or newly important mechanism for dephasing Houck et al. (2009). These devices have a single Josephson junction, eliminating the sensitivity to flux noise Wellstood et al. (1987), and surprisingly show only a weak temperature-dependent dephasing, inconsistent with some predictions based on extrapolations of junction critical current noise Van Harlingen et al. (2004); Eroms et al. (2006). In these devices, the qubit state is detected by observing the dispersive frequency shift of a resonant cavity. However, it is known Bertet et al. (2005); Gambetta et al. (2006); Serban et al. (2007) that in the strong-dispersive regime the qubit becomes very sensitive to stray cavity photons, which cause dephasing due to their random ac-Stark shift Schuster et al. (2005). It requires increasing care to prevent this extrinsic mechanism from becoming the dominant source of dephasing as qubit lifetimes increase. Experiments elsewhere Rigetti et al. (2012) and in our lab Sun et al. (2010) have shown that pure dephasing times can be many hundreds of microseconds with careful thermalization and more extensive filtering.
In this Letter, we quantitatively test the dephasing of a qubit due to photon shot noise in the strong-dispersive coupling limit with a cavity. In this novel regime where the ac-Stark shift per photon is many times greater than the qubit linewidth and the cavity decay rate Schuster et al. (2007), the passage of any photon through the cavity performs a complete and unintended measurement of the qubit state. This limit also allows a precise determination of the photon number in the cavity using Rabi experiments on the photon number-split qubit spectrum Johnson et al. (2010). With a simulated thermal bath injecting photons into the cavity and in situ mechanical adjustment of the cavity , we find a pure dephasing of the qubit that quantitatively matches theory Gambetta et al. (2006). Furthermore, we verify that the qubit is strongly coupled to photons in several cavity modes and find that the dephasing from these modes accounts for the reduced coherence times as a function of cryostat temperature. Our measurements at 10 mK demonstrate that decreasing leads to longer qubit coherence times, suggesting that existing dephasing in superconducting qubits is due to unintended and preventable measurement by excess photons in higher frequency modes.
The experiments were performed (see Fig. 1) with a transmon qubit coupled in the strong-dispersive limit to a 3D cavity, and well approximated by the Hamiltonian Nigg et al. (2012):
(1) |
where the operator creates a cavity photon and the operator creates a qubit excitation. Then is the cavity frequency, and are the qubit frequency and anharmonicity, and MHz is the light shift per photon which can be 1000 times larger than the qubit linewidth of kHz, and the cavity linewidth kHz. The large dispersive shift leads to the well-resolved peaks in the qubit spectrum shown in Fig. 1c, allowing us to conditionally manipulate the qubit depending on the cavity photon number Johnson et al. (2010). Measuring the height of a given photon number-split qubit peak (or the amplitude of a Rabi oscillation at frequency ) allows a direct determination of the probability for the cavity to have a particular photon number.
Dephasing of the qubit can be caused by a random change in cavity photon number, which shifts the qubit energy by per photon and leads to a large rate of phase accumulation relative to . Then the pure dephasing rate , obtained in a Ramsey experiment for the qubit, depends on the stability of the photon cavity state. When the cavity is connected to a thermal bath, the probability follows a system of equations Walls and Milburn (1994) for the rate of change into and out of the photon state: , where the cavity decay rate is the inverse of its decay time , is the average number of photons, and
(2) |
combines the spontaneous emission of photons with the stimulated emission due to thermal photons. Then, in the strong-dispersive regime (and neglecting other sources of dephasing) the dephasing rate becomes , and the success of an experiment that relies on phase predictability of the qubit requires a constant photon number in the cavity throughout each cycle.
To verify this prediction for quantitatively, we first calibrate our thermal bath and then obtain with experiments on the photon peaks of the qubit. We can determine the cavity decay rate by exciting the cavity with a short coherent pulse while measuring the repopulation of the ground state (i.e. the amplitude of the zero-photon Rabi oscillations) over timescale . Alternatively, exciting the cavity with a wideband noise source that covers the cavity transition frequency but not the qubit transition frequency, creates an average photon number . Here, is the linear power loss from additional cold attenuation, is the Bose-Einstein population of the load of the noise source at effective temperature , located outside the cavity. The total cavity quality factor has an inverse which is the sum of the inverses of the coupling quality factor of the noise source port, all other port couplings, and the internal quality factor . In steady state and for uncorrelated noise, the probability of finding the qubit in an environment with photons is a thermal distribution , as verified by the data in Fig. 1d. With these measurements we obtain the scaling of as a function of applied noise power for each different value of , allowing a comparison with Eq. 2 using no adjustable parameters.
To observe the influence of photon dephasing on our qubit, we test Eq. 2 over a wide range of values for both and as shown in Fig. 2. The photon number is varied by adjusting the attenuation following our noise source, while is controlled by retracting the resonator output coupler using a Kevlar string connected to the top of the fridge, exponentially increasing the as it is withdrawn. For large , photons enter and leave quickly, so long periods uninterrupted by a transit are rare even if the average occupation is low, and the phase coherence time is short. In the Ramsey data shown in Fig. 2 the dephasing rate is universally proportional to injected and , with an offset due to spontaneous decay (if ), and residual photons or other intrinsic dephasing. These experiments confirm our understanding of the qubit dephasing rate in the strong-dispersive limit, and point to the importance of excess photons or an effective temperature of a mode for qubit coherence.
Importantly, we use slow Gaussian pulses to control the qubit in order to exploit the photon-dependence of our Hamiltonian. With a width of ns, the narrow frequency span of the pulses means that Ramsey experiments add signal contrast only when the chosen photon number has remained in the cavity throughout the experiment, a type of post-selection evident in the different scalings of Fig. 2b-d. Once conditioned, photon transitions during the experiment lead to an incoherent response in our qubit readout, when at a random point in time an initially prepared superposition changes: for time . Our qubit readout Reed et al. (2010) traces over all photon states, and the unknown final phase of the superposition produces a decay in the Ramsey fringes, as the experiment records the qubit excitation despite any cavity transition. Additionally, a characteristic bump and slope are visible in the data and must be removed before fitting the Ramsey signal with the usual decaying sine function. These features can be understood as the re-equilibration of the cavity photon number after the first qubit manipulation conditionally prepares a certain photon number, and are well fit (see Fig. 3 of the Supplement) by a simple master equation which includes the incoherent cavity drive as well as qubit and cavity decay.
While the fundamental mode of our 3D resonator serves both as the qubit readout channel and as a mechanism for dephasing, the rectangular cavity in fact supports a set of modes Poole (1967) whose influence we must consider. Then a more comprehensive Hamiltonian than Eq. 1 must incorporate many different cavity frequencies, each with a coupling strength that depends on antenna length and the positioning of the qubit in the cavity Nigg et al. (2012). This coupling is large for odd- modes where the electric field has an antinode at the qubit, while the even- modes have greatly diminished coupling to the qubit due to a node along the qubit antenna. For our parameters, the fundamental mode GHz, GHz, and MHz, the qubit anharmonicity MHz leads to an ac-Stark shift of MHz. Similarly, the first odd harmonics with GHz has a large MHz. In fact, with this mode we can perform high fidelity readout, measure the photon mode population (using longer ns width pulses), and observe its influence on decoherence by injecting noise near . In general, we should consider all cavity modes that have a non-zero coupling to the qubit as sources of significant decoherence. For example, the odd- modes at frequency and detuning , have a coupling and an ac-Stark shift which decrease only slowly as . Consequently, there may be many modes with significant dispersive shifts that can act as sources of extrinisic qubit decoherence. Moreover, since the coupling quality factors of these modes typically decreases with frequency, even very small photon occupancies (which are usually ignored, not measured or as carefully filtered) must be suppressed to obtain maximum coherence.
The photon shot noise from multiple cavity modes provides a simple explanation for the anomalous qubit dephasing previously observed Paik et al. (2011) as a function of cryostat temperature. In this case, each cavity mode should be populated with the Bose-Einstein probability and these thermal photons can make an unintended measurement of the qubit, disrupting phase-sensitive experiments. The predicted occupancies for the and modes are shown (green lines) in the inset of Fig. 3, along with their predicted dephasing (blue lines). Having confirmed the dephasing rates for all modes individually we can now combine the effect of all modes that strongly couple to the qubit: . This total thermal decoherence rate is shown as the red dashed line in the inset of Fig. 3, for typical parameters. Since these modes have , the predicted dephasing time is in excess of 100 microseconds below 80 mK due to the exponentially suppressed number of blackbody photons. However, since any particular mode coupling to the qubit in the strong-dispersive limit may have a relatively fast decay time , even very small () non-thermal populations could easily satisfy , limiting the coherence through pure dephasing alone to . The measured coherence times as a function of temperature are well fit (see Fig. 3) by the combined dephasing of thermal occupancy of the and modes, plus a parameter adjusted to represent the residual dephasing in each experiment. This excess could be due to another mechanism intrinsic to the qubit, or simply due to insufficient filtering or thermalization of the apparatus, leading to a small non-thermal photon population.
Further evidence that the true intrinsic coherence limits of the 3D transmons have not yet been observed is provided by the data shown in Fig. 4, where the qubit relaxation time (), Ramsey time (), and Hahn echo time () at 10 mK are shown as a function of the cavity decay time. We see that the relaxation time is relatively unaffected by cavity lifetime, since this qubit is sufficiently detuned from the cavity to minimize the Purcell effect Houck et al. (2008). However, we observe a general trend where and increase as the cavity lifetime increases. This is consistent with a decoherence due to residual photons with ever slower dynamics, but not expected due to e.g. junction critical current noise, which should be independent of cavity properties. The maximum echo time (45 ) observed here indicates that coherence of small Josephson junction qubits is in excess of several hundred microseconds when corrected by a single Hahn echo.
In conclusion, we have performed experiments involving precise thermal photon populations to quantitatively induce qubit dephasing in good agreement with simple theory. We find that photons in the fundamental and at least one harmonic mode of the cavity strongly couple to a transmon qubit and note that at the nominal base temperature of our cryostat they produce a negligible amount of dephasing. However, the sensitivity of the qubit to photons at many frequencies requires that we either keep all modes of the cavity in their ground state, or else minimize the influence of non-thermal populations by reducing their measurement rate Hatridge et al. (2010). Inclusion of the cavity harmonics in dephasing calculations leads to an understanding of the earlier, anomalous, temperature-dependent decoherence in our devices Paik et al. (2011). Finally, we find evidence that interactions with the residual photons in our 3D cavity likely mask the intrinsic coherence time of the Josephson junction, whose limits are much longer than qubit coherence times seen so far. As qubit linewidths shrink in the future, other effects such as quasiparticle parity Schreier et al. (2008); Sun et al. (2012); Naaman and Aumentado (2006) or nuclear spins Schuster et al. (2010) may further split the qubit spectrum, enabling probes of their state dynamics using these procedures.
We thank Michel Devoret for valuable discussions. L. F. acknowledges partial support from CNR-Istituto di Cibernetica. This research was funded by the Office of the Director of National Intelligence (ODNI), Intelligence Advanced Research Projects Activity (IARPA), through the Army Research Office, as well as by the National Science Foundation (NSF DMR-1004406). All statements of fact, opinion or conclusions contained herein are those of the authors and should not be construed as representing the official views or policies of IARPA, or the U.S. Government.
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