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Circuit quantum electrodynamics, or circuit QED, couples superconducting artificial atoms to quantized microwave resonators and transmission lines. For open-system physics it is one of the cleanest platforms: the resonator is both a quantum degree of freedom and a measurement port, microwave loss channels are engineered with known rates, and continuous voltage records can be modeled with input–output theory and stochastic master equations.

We follow a readout signal from qubit-dependent resonator motion to the measured voltage, keeping track of the dephasing and relaxation caused by the same coupling. Circuit QED Overview explains the hardware and device design.

The simplest idealized circuit-QED Hamiltonian is the Jaynes–Cummings model,

HJCℏ=ωra†a+ωq2σz+g(a†σ−+aσ+),\frac{H_{\mathrm{JC}}}{\hbar} = \omega_r a^\dagger a + \frac{\omega_q}{2}\sigma_z + g \left( a^\dagger\sigma_- + a\sigma_+ \right),

where aa annihilates a resonator photon, ωr\omega_r is the resonator frequency, ωq\omega_q is the qubit transition frequency, and gg is the transverse coupling. For the closed-system spectrum, see Jaynes–Cummings Model.

The minimal open-system version adds resonator decay, qubit relaxation, and qubit dephasing:

ρ˙=−iℏ[H,ρ]+κD[a]ρ+γ1D[σ−]ρ+γϕ2D[σz]ρ+⋯ .\dot\rho = - \frac{i}{\hbar} [H,\rho] + \kappa\mathcal D[a]\rho + \gamma_1\mathcal D[\sigma_-]\rho + \frac{\gamma_\phi}{2} \mathcal D[\sigma_z]\rho + \cdots .

Here κ\kappa is the resonator energy-decay rate, γ1=1/T1\gamma_1=1/T_1 is qubit relaxation, and γϕ\gamma_\phi is pure dephasing. The ellipsis may include thermal photons, leakage levels, additional ports, quasiparticle loss, flux noise, or engineered dissipation.

Most superconducting qubit readout operates in the dispersive regime, where the detuning

Δ=ωq−ωr\Delta = \omega_q-\omega_r

is large compared with the photon-enhanced coupling over the occupied photon-number range:

∣Δ∣≫gn+1.\lvert\Delta\rvert\gg g\sqrt{n+1}.

For an ideal two-level qubit, a second-order transformation gives the approximate dispersive Hamiltonian

Hdispℏ=(ωr+χσz)a†a+ωq+χ2σz,\frac{H_{\mathrm{disp}}}{\hbar} = \left( \omega_r+\chi\sigma_z \right) a^\dagger a + \frac{\omega_q+\chi}{2}\sigma_z,

with

χ≃g2Δ\chi \simeq \frac{g^2}{\Delta}

in the simplest two-level approximation. For a weakly anharmonic transmon with α=ω12−ω01<0\alpha=\omega_{12}-\omega_{01}<0, the leading expression is χ≃g2α/[Δ(Δ+α)]\chi\simeq g^2\alpha/[\Delta(\Delta+\alpha)]. Both relevant transitions must remain dispersive. The two-level estimate also fails as photon number approaches its critical scale ncrit∼Δ2/(4g2)n_{\mathrm{crit}}\sim\Delta^2/(4g^2).

The physical content is that the resonator frequency depends on the qubit state:

ωr(g)≃ωr−χ,ωr(e)≃ωr+χ.\omega_r^{(g)} \simeq \omega_r-\chi, \qquad \omega_r^{(e)} \simeq \omega_r+\chi.

A microwave probe near the resonator therefore acquires a qubit-dependent phase and amplitude. Measuring the outgoing field becomes an indirect measurement of σz\sigma_z.

Input–output theory supplies the connection between the intracavity field and the measured traveling microwave field. For a single port with no other cavity loss,

bout(t)=bin(t)+κ a(t),b_{\mathrm{out}}(t) = b_{\mathrm{in}}(t) + \sqrt{\kappa}\,a(t),

up to the phase convention used for the port. The same coupling gives the dissipator κD[a]ρ\kappa\mathcal D[a]\rho when the output field is not retained. See Input–Output Theory.

During a dispersive readout pulse, the resonator relaxes toward different coherent amplitudes depending on the qubit state:

αg(t),αe(t).\alpha_g(t), \qquad \alpha_e(t).

The outgoing field contains information about which pointer state the resonator occupies. The distinguishability of αg\alpha_g and αe\alpha_e controls both the measurement signal and the dephasing caused by information leaking into the output field.

In steady state, for the ideal linear dispersive model with vacuum loss channels, the qubit coherence decays at the measurement-induced rate

Γϕmeas=κ2∣αe−αg∣2.\Gamma_\phi^{\mathrm{meas}} = \frac{\kappa}{2} \left| \alpha_e-\alpha_g \right|^2.

During ring-up and ring-down, qubit coherence is also reduced by distinguishability still stored inside the resonator. For an initially common coherent cavity state, no qubit flips, and total vacuum linewidth κ\kappa, define δα(t)=αe(t)−αg(t)\delta\alpha(t)=\alpha_e(t)-\alpha_g(t). The magnitude is

∣ρge(t)∣∣ρge(0)∣=exp⁡[−∣δα(t)∣22−κ2∫0t∣δα(s)∣2 ds].\frac{|\rho_{ge}(t)|}{|\rho_{ge}(0)|} =\exp\left[-\frac{|\delta\alpha(t)|^2}{2} -\frac{\kappa}{2}\int_0^t|\delta\alpha(s)|^2\,ds\right].

The first term is the intracavity overlap; the second is the accumulated output-field overlap. Therefore κ∣δα∣2/2\kappa|\delta\alpha|^2/2 alone is not the complete instantaneous reduced-qubit dephasing rate during a transient. Collection inefficiency reduces accessible information, not the dephasing already caused by all output ports. Gambetta et al. treat the dispersive dynamics.

Dispersive readout is approximately a quantum nondemolition measurement of σz\sigma_z when the Hamiltonian commutes with σz\sigma_z and unwanted transitions are negligible. In that limit, the measurement dephases superpositions of ∣g⟩\lvert g\rangle and ∣e⟩\lvert e\rangle without directly changing their populations.

If the resonator field becomes correlated with the qubit,

cg∣g⟩∣αg⟩+ce∣e⟩∣αe⟩,c_g\lvert g\rangle\lvert\alpha_g\rangle + c_e\lvert e\rangle\lvert\alpha_e\rangle,

then tracing out the intracavity field gives an overlap factor ⟨αe∣αg⟩\langle\alpha_e|\alpha_g\rangle in the qubit coherence; emitted fields supply an additional overlap factor. The overlap of the field records decreases as the two pointer amplitudes separate. Thus readout backaction is not a mysterious extra effect; it is the loss of phase coherence caused by information about σz\sigma_z becoming available outside the qubit.

This is the platform version of Measurement Backaction and Diffusive Trajectories.

When the resonator is fast compared with the qubit dynamics, one often eliminates it and writes an effective continuous measurement of σz\sigma_z. A schematic homodyne stochastic master equation is

dρc=Lρc dt+ηΓm H[σz]ρc dWt,d\rho_c = \mathcal L\rho_c\,dt + \sqrt{\eta\Gamma_m}\, \mathcal H[\sigma_z]\rho_c\,dW_t,

with record

dYt=2ηΓm ⟨σz⟩c dt+dWt.dY_t = 2\sqrt{\eta\Gamma_m}\, \langle\sigma_z\rangle_c\,dt + dW_t.

Choose L\mathcal L to include ΓmD[σz]\Gamma_m\mathcal D[\sigma_z]. Its off-diagonal decay rate is 2Γm2\Gamma_m, so in the steady dispersive limit above Γm=κ∣αe−αg∣2/4\Gamma_m=\kappa|\alpha_e-\alpha_g|^2/4. Here η\eta includes collection and detector loss, the homodyne phase is aligned with the pointer separation, and dWt2=dtdW_t^2=dt. Averaging over records recovers this unconditional dephasing.

This reduced equation is powerful, but it hides the resonator dynamics. It is least reliable when the readout pulse is short, the resonator is not adiabatically eliminated, the photon number is high, or dressed-state transitions matter.

The resonator also provides a decay channel for the qubit. In the dispersive regime, the qubit-like excitation has a small resonator component. If the resonator decays at rate κ\kappa, this admixture gives the approximate Purcell decay rate

γP≃κ(gΔ)2\gamma_{\mathrm P} \simeq \kappa \left( \frac{g}{\Delta} \right)^2

for an ideal two-level model far from resonances and filters. Real devices use Purcell filters, multilevel corrections, and frequency-dependent impedances, so this expression is a scaling estimate, not a complete design rule.

The conceptual lesson is open-system: an engineered measurement port can also be an unwanted relaxation bath. Increasing readout bandwidth can improve measurement speed while worsening radiative decay unless the environment is shaped carefully.

Circuit-QED models often organize noise into a few experimentally meaningful rates:

Channel Model term Typical physical sources
resonator decay κD[a]ρ\kappa\mathcal D[a]\rho external coupling, internal loss
qubit relaxation γ1D[σ−]ρ\gamma_1\mathcal D[\sigma_-]\rho dielectric loss, Purcell loss, quasiparticles
pure dephasing γϕD[σz]ρ/2\gamma_\phi\mathcal D[\sigma_z]\rho/2 flux noise, charge noise, photon-number fluctuations
thermal excitation γ↑D[σ+]ρ\gamma_\uparrow\mathcal D[\sigma_+]\rho hot modes, nonequilibrium quasiparticles
leakage multilevel dissipators finite transmon anharmonicity, strong drives

The familiar relation

1T2=12T1+1Tϕ\frac{1}{T_2} = \frac{1}{2T_1} + \frac{1}{T_\phi}

is a rate-level summary, not a microscopic derivation. It assumes Markovian exponential decay and a clean separation between relaxation and pure dephasing.

Circuit-QED calculations often rely on:

  • rotating-wave approximation for the qubit-resonator coupling;
  • dispersive expansion in g/Δg/\Delta;
  • two-level truncation of a weakly anharmonic transmon;
  • Markovian treatment of transmission-line ports;
  • adiabatic elimination of a fast resonator;
  • Gaussian or white-noise approximation for selected noise sources;
  • semiclassical treatment of strong readout drives.

Each approximation has a failure mode. Strong drives can populate levels outside the qubit subspace. Small detuning can invalidate dispersive elimination. Slow flux noise is not a broadband Markov bath. Residual thermal photons can dephase an apparently idle qubit. A careful model records which approximation is being used rather than hiding all imperfections inside fitted T1T_1 and T2T_2 values.

Starting from the Jaynes–Cummings model with detuning Δ=ωq−ωr\Delta=\omega_q-\omega_r, estimate the resonator frequency shift in the dispersive regime for an ideal two-level qubit.

Solution

For ∣Δ∣≫g|\Delta|\gg g, second-order perturbation theory gives energy shifts of order g2/Δg^2/\Delta. The effective dispersive Hamiltonian is

Hdispℏ=(ωr+χσz)a†a+ωq+χ2σz,\frac{H_{\mathrm{disp}}}{\hbar} = \left( \omega_r+\chi\sigma_z \right)a^\dagger a + \frac{\omega_q+\chi}{2}\sigma_z,

with

χ≃g2Δ\chi\simeq\frac{g^2}{\Delta}

for the ideal two-level model. Therefore the resonator frequency is shifted to approximately ωr−χ\omega_r-\chi for ∣g⟩\lvert g\rangle and ωr+χ\omega_r+\chi for ∣e⟩\lvert e\rangle.

If a readout pulse produces pointer amplitudes αg\alpha_g and αe\alpha_e and the resonator decays at rate κ\kappa, what is the steady-state measurement-induced dephasing rate in the ideal dispersive model? Why is a short pulse different?

Solution

The outgoing field carries information about the qubit through the separation of the two pointer amplitudes. In steady state,

Γϕmeas=κ2∣αe−αg∣2.\Gamma_\phi^{\mathrm{meas}} = \frac{\kappa}{2} \left| \alpha_e-\alpha_g \right|^2.

Thus dephasing grows with the rate at which distinguishable information about the qubit leaves through the resonator port. If αe=αg\alpha_e=\alpha_g, the output field does not distinguish the qubit states and this contribution vanishes. During a short pulse, the changing intracavity overlap must also be included, as in the transient expression above.

Explain why the Purcell decay rate scales as κ(g/Δ)2\kappa(g/\Delta)^2 in the dispersive limit.

Solution

In the dispersive regime, a mostly qubit-like excitation contains a small resonator-like admixture of amplitude of order g/Δg/\Delta. Decay through the resonator port is proportional to the resonator weight, which is the squared amplitude:

(gΔ)2.\left( \frac{g}{\Delta} \right)^2.

Multiplying by the resonator decay rate gives the scaling estimate

γP≃κ(gΔ)2.\gamma_{\mathrm P} \simeq \kappa \left( \frac{g}{\Delta} \right)^2.

A qubit has T1=40 μsT_1=40\,\mu\mathrm{s} and pure dephasing time Tϕ=80 μsT_\phi=80\,\mu\mathrm{s}. Under the Markovian rate model, what is T2T_2?

Solution

Use

1T2=12T1+1Tϕ.\frac{1}{T_2} = \frac{1}{2T_1} + \frac{1}{T_\phi}.

Substituting,

1T2=180 μs+180 μs=140 μs.\frac{1}{T_2} = \frac{1}{80\,\mu\mathrm{s}} + \frac{1}{80\,\mu\mathrm{s}} = \frac{1}{40\,\mu\mathrm{s}}.

Therefore

T2=40 μs.T_2=40\,\mu\mathrm{s}.
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