Four-Wave Mixing SMPD Efficiency

Based on Balembois et al., “Cyclically operated Single Microwave Photon Counter with 10−22 W/√Hz sensitivity”, arXiv:2307.03614. Implements Eq. (3) (four-wave mixing transfer efficiency), Appendix G (optimal detection time), and the total-efficiency product ηtheory = η4wm · ηRO · ηD · ηqubit.
Glossary — what each variable means
χb, χw Dispersive shifts of the transmon qubit with respect to the buffer (b) and waste (w) resonators. Quoted as χ/2π in MHz.
κb, κw Total linewidths (energy decay rates) of the buffer and waste resonators. Quoted as κ/2π in MHz. κw provides the irreversible dissipation that makes the click event irreversible.
|ξ| Pump amplitude (dimensionless, in units of √photons) of the off-resonant pump tone that activates the four-wave-mixing process. Controls the parametric coupling g3 = 2|ξ|√(χbχw).
C Cooperativity of the four-wave-mixing process, C = 4|ξ|2χbχw/(κbκw). Unit transfer efficiency is reached at C = 1.
η4wm Transfer efficiency of a buffer photon into a qubit excitation via the four-wave-mixing process (Eq. 3). Peaks at 1 when C = 1.
T1 Qubit energy-relaxation time (|e⟩ → |g⟩). Sets how long an absorbed excitation survives in the qubit.
Td Detection window: duration during which the pump is on and an incoming photon can trigger a qubit excitation.
Tm Measurement window: duration of the dispersive readout pulse on the waste resonator that checks the qubit state.
Tr Reset window: conditional reset back to |g⟩ (π-pulse + re-measurement if the qubit was found excited). Use the average reset time.
Tcycle Td + Tm + Tr, the total duration of one detect–measure–reset cycle.
ηD Duty-cycle efficiency = fraction of time the detector is actually listening, Td/Tcycle.
ηqubit Probability that a qubit excitation created during detection survives until measurement, averaged over the detection window: (T1/Td)(1 − e−Td/T1).
ηRO Single-shot readout fidelity for the excited state — probability of reading “click” given the qubit is in |e⟩.
ηtheory Total predicted operational efficiency: η4wm · ηRO · ηD · ηqubit.
1. Four-wave mixing efficiency η4wm

η4wm = 4C/(1+C)2,   C = 4|ξ|2 χbχw/(κbκw). The 2π factors cancel in the ratio, so χ/2π and κ/2π in MHz may be entered directly.

2. Optimal detection time (Appendix G)

ηD = Td/(Tm+Tr+Td),   ηqubit = (T1/Td)(1 − e−Td/T1). Optimum: Tdopt ≈ √(2(Tm+Tr)T1)  (Eq. G3).

3. Total detection efficiency

ηtheory = η4wm · ηRO · ηD · ηqubit. Uses η4wm(|ξ|) from section 1 and ηD, ηqubit from section 2.

  

Formulas

QuantityExpression
Cooperativity C 4|ξ|2 χbχw/(κbκw)
4WM efficiency η4wm 4C/(1+C)2   (Eq. 3)
Optimal pump |ξ|opt √(κbκw/(4χbχw))   (C=1)
Duty-cycle efficiency ηD Td/(Tm+Tr+Td)
Qubit efficiency ηqubit (T1/Td)(1 − e−Td/T1)
Optimal detection time Tdopt ≈ √(2(Tm+Tr)T1)   (Eq. G3)
Total efficiency ηtheory = η4wm · ηRO · ηD · ηqubit
How to compare to an experiment

Two kinds of measurement map onto the efficiencies on this page. Which one you look at determines which factors appear.

(a) End-of-detection qubit population pe (Fig. 2a-style). Read the qubit immediately after the detection window. In the weak-signal regime (⟨nph⟩ ≪ 1 per cycle):

pe(|ξ|)  ≈  pebg + η4wm(|ξ|) · ηqubit · ⟨nph

with ⟨nph⟩ = Φin · Td the mean number of signal photons during the detection window. Only η4wm and ηqubit enter — ηRO and ηD do not, because you are reading the population directly rather than converting to a per-second rate. Normalizing the curve to its peak gives the shape η4wm(|ξ|) independent of the absolute calibration of Φin.

(b) Click rate vs incoming photon rate (Fig. 3b-style — recommended). Record the detector click rate R for several input photon rates Φin and fit a line:

R  =  η · Φin  +  α

  • Slope η = η4wm · ηRO · ηD · ηqubit — the full operational efficiency from section 3 of this calculator.
  • Intercept α — the dark count rate (incl. thermal photons in the input line, pump-induced qubit heating, and thermal qubit population).

The linear fit extracts η and α simultaneously from one dataset, so dark counts are absorbed into the intercept and you do not need a separately calibrated “signal off” baseline (nor an accurate subtraction, which can drift between runs). For reliable numbers, sweep Φin over at least a decade and include a point or two deep enough that η · Φin ≫ α as well as a point near Φin = 0 to anchor the intercept.

The power sensitivity then follows from Eq. 1 of the paper:  𝒮 = ℏω√α / η.

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