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Exploring the Jaynes-Cummings Hamiltonian with Qiskit Pulse
Physics Background
The Jaynes-Cummings model describes a two-level system (qubit) interacting with a single-mode of an electromagnetic cavity (resonator). When a two-level system is placed in a cavity, it couples to the cavity with strength , spontaneously emits its excitation with rate , while the cavity decays with rate . In this tutorial we measure the parameters of a system consisting of a superconducting qubit coupled to a superconducting resonator using Qiskit Pulse.
This qubit-cavity interaction can be described using the Jaynes-Cummings (JC) Hamiltonian:
Let's break down this Hamiltonian in different parts: The first part of the Hamiltonian describes the resonator. The resonator can be treated as a quantum harmonic oscillator, where is the resonator frequency, and and are the raising a lowering operators of the resonator photons. Note that for simplicity we have omitted the zero point energy of the harmonic oscillator. The next term in the JC Hamiltonian describes the qubit. Here, is the qubit frequency, and is the Pauli-Z operator. The final term of the Hamiltonian describes the interaction between the resonator and the qubit: is the coupling strength between the qubit and the resonator, and the operators and represent exciting and de-exciting the qubit. Based on this interaction term we can see that the process of exciting a qubit leads to a photon loss in the resonator and vice-versa.
In the limit that detuning between the qubit and the resonator is less than the coupling strength between the two, , the resonator-qubit system becomes hybridized, leading to coherent excitation swaps which can be useful for certain two-qubit operations. However, for optimal readout, we want to operate the system in the dispersive limit, where the qubit-resonator detuning is much larger than the coupling rate and the resonator decay rate: . In this limit the interaction between the qubit and resonator influences each of their frequencies, a feature that can be used for measuring the state of the qubit. We can apply the dispersive approximation in the limit of few photons in the resonator, and approximate the JC Hamiltonian using second-order perturbation theory as:
where is the dispersive shift (the negative sign is due to the fact that the transmon has a negative anharmonicity), and is the modified qubit frequency, experiencing a Lamb shift.
The circuit quantum electrodynamics derivations are discussed in another chapter.
0. Getting started
We'll first get our basic dependencies and helper functions set up and ready to go.
Warning
This experiment is not available in the current ibmq_armonk
device owing to the measurement apparatus configuration. You cannot find cavity resonance within the reasonable scanning range. Try with other devices if you have access to.
We then extract the default backend configuration and settings for the selected chip.
Next we define some helper functions that we will use for fitting and interpreting our data.
1. Measuring
Photons decay out of imperfect electromagnetic cavities. The decay rate for the resonator cavity can be measured by calculating the linewidth of the resonance peak in a resonator spectroscopy scan. Larger values of imply that the resonator cavity is more lossy. The resonator loss can be quantified using the quality factor ; higher indicates a lower rate of energy loss from the cavity.
Here we send our pulse sequence to the hardware.
And then we access the measurement data. The resonator in the backend we use for this tutorial is measured reflectively, so the spectroscopy data is encoded in the phase of the output signal. We fit a Lorentzian function to the data to extract the resonator frequency and linewidth.
2. Measuring and
Next, we measure the qubit-resonator coupling. One method for measuring the dispersive shift () and subsequently the qubit-resonator coupling () is to compare the resonator frequency in the dispersive limit with the frequency in the non-interactive regime, where the resonator does not get shifted by . In the non-interactive limit the resonator photon number is larger than . In experiment we can populate the resonator with more photons by driving it with more power.
Here we send our pulse sequence to the hardware.
And then we access the measurement data for the high power resonator spectroscopy scan.
Finally we plot the high power resonator spectroscopy next to the low power scan from the previous section and use the shift in resonator frequency to calculate .
3. Measuring
A qubit coupled to a resonator will spontaneous emit photons into the cavity, and therefore relaxing from an excited state to the ground state. The spontaneous emission of photons gets enhanced by the qubit environment, a phenomenon known as the Purcell effect. We can measure the qubit decay rate by exciting the qubit with a microwave drive, and measuring the decay rate of the qubit excitation. This experiment is a common method method for measuring qubit coherence properties as discussed in this chapter. For this experiment our microwave drive doesn't have to be -pulse.
Here we send our pulse sequence to the hardware.
And then we access the measurement data. We fit an exponential to the data to extract the decay time constant.
In this chapter, we introduce the Jaynes-Cummings model and we consider the relevant quantities for a system consisting of a qubit coupled to a cavity. We use Qiskit Pulse to extract the qubit-resonator coupling strength , the qubit spontaneous emission rate , and the cavity decay rate . These parameters combined with the qubit frequency and the resonator frequency that we measured in a previous chapter allow us to describe our qubit-resonator system.