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Interconnects and Transduction

An interconnect transfers quantum information or distributes entanglement between physical nodes. A transducer changes the carrier or frequency used along that path. A cold microwave cable can connect superconducting modules without conversion; a microwave–optical converter can bridge their frequencies to optical fibre. In either case, preserving a coherent classical tone is a weaker test than preserving an unknown qubit or entanglement.

Three quantities must be distinguished: how much signal reaches the output, how much reaches the receiver’s mode, and how much unwanted excitation arrives with it. This page develops these hardware questions. Quantum Teleportation and Quantum Repeaters explain the protocols that use such links.

Required background. Hardware Overview introduces device operations; Bits, Qubits, Qudits, and Modes distinguishes encodings; Quantum Channels and Noise provides the channel description of a lossy transfer.

Coherent transfer and heralded entanglement

Section titled “Coherent transfer and heralded entanglement”

For direct transfer, the receiver starts in a known state. In a single-rail encoding, an ideal operation has the action

(α∣0⟩A+β∣1⟩A)∣0⟩B⟼∣0⟩A(α∣0⟩B+eiϕβ∣1⟩B).(\alpha|0\rangle_A+\beta|1\rangle_A)|0\rangle_B \longmapsto |0\rangle_A(\alpha|0\rangle_B+e^{i\phi}\beta|1\rangle_B).

The phase ϕ\phi must be stable and corrected or tracked. Emission, conversion, propagation, and capture together determine this map; efficient conversion inside one resonator does not establish efficient transfer between nodes. Cirac and colleagues give a cavity-based construction, while Kurpiers and colleagues demonstrate shaped microwave emission and capture.

Loss in the vacuum/one-photon encoding produces amplitude damping: an absent photon is indistinguishable from the logical ∣0⟩|0\rangle. In a dual-rail one-photon encoding, the two-mode vacuum lies outside the code and can in principle identify loss. A practical nondestructive flag requires an appropriate detector, ancillary system, or subsequent protocol; destructive photon detection cannot leave the same unknown flying qubit available for use.

In heralded entanglement, photons correlated with two local memories interfere at a measurement station. A suitable joint outcome announces an entangled memory pair. Cleanly rejected loss lowers the accepted rate; false detections, multiphoton emission, distinguishability, and memory decoherence can also lower the fidelity of accepted pairs. The successful event must not reveal which component of the intended superposition occurred.

The pair can subsequently support teleportation of a data qubit. Its quality can be estimated on separately measured sample pairs; ordinary tomography does not certify each pair while also leaving that same pair intact. Classical notification and memory storage remain necessary. Physical transport of an ion, atom, or electron is another way to connect zones: carrier conversion is absent, but heating, leakage, loss, and path-dependent phase still affect the transported state.

Let [ain(t),ain†(t′)]=δ(t−t′)[a_{\rm in}(t),a_{\rm in}^\dagger(t')]=\delta(t-t'). A normalized envelope defines one bosonic mode,

Af=∫dt f∗(t)ain(t),∫dt ∣f(t)∣2=1.\begin{aligned} A_f&=\int dt\,f^*(t)a_{\rm in}(t), \\ \int dt\,|f(t)|^2&=1. \end{aligned}

Then [Af,Af†]=1[A_f,A_f^\dagger]=1. If the emitted photon has envelope ff and the receiver accepts gg, the captured probability in the absence of other loss is

μ=∫dt g∗(t)f(t),ηmode=∣μ∣2.\mu=\int dt\,g^*(t)f(t), \qquad \eta_{\rm mode}=|\mu|^2.

The phase of μ\mu matters for superpositions of vacuum and one photon, and relative phases matter between two encoded rails. Noise or excitations in orthogonal modes cannot automatically be treated as vacuum loss; the vacuum environment assumption must be justified.

For stationary, linear conversion, express frequencies as offsets Ω\Omega from each port’s carrier in its rotating frame. In a number-conserving model,

bout(Ω)=Sba(Ω)ain(Ω)+∑jSbj(Ω)vj(Ω).b_{\rm out}(\Omega) =S_{ba}(\Omega)a_{\rm in}(\Omega) +\sum_j S_{bj}(\Omega)v_j(\Omega).

The vjv_j include unused and dissipative input ports. With all such ports included, preservation of the output commutator requires

∣Sba(Ω)∣2+∑j∣Sbj(Ω)∣2=1.|S_{ba}(\Omega)|^2+\sum_j|S_{bj}(\Omega)|^2=1.

Gardiner and Collett develop this input–output description of damped modes.

Here “number conserving” concerns signal excitations after treating the pumps classically. The pumps supply the difference between input and output photon energies. A full active linear transformation can also contain creation operators. A phase-preserving amplifier must introduce idler noise; an ideal single-mode squeezer instead changes the two quadrature noises unequally and need not add an independent environmental mode. See Caves and Continuous-Variable Platforms.

For normalized spectral amplitudes f(Ω)f(\Omega) and g(Ω)g(\Omega), the signal probabilities, with noise counted separately, are

ηtotal=∫dΩ ∣Sba(Ω)f(Ω)∣2,ηcapture=∣∫dΩ g∗(Ω)Sba(Ω)f(Ω)∣2≤ηtotal.\begin{aligned} \eta_{\rm total}&=\int d\Omega\,|S_{ba}(\Omega)f(\Omega)|^2, \\ \eta_{\rm capture}&= \left|\int d\Omega\,g^*(\Omega)S_{ba}(\Omega)f(\Omega)\right|^2 \\ &\le\eta_{\rm total}. \end{aligned}

This distinction is useful even for a lossless device. Take a Gaussian spectral intensity of variance σΩ2\sigma_\Omega^2, a quadratic spectral phase Sba=eiβΩ2/2S_{ba}=e^{i\beta\Omega^2/2}, and a receiver still matched to the original g=fg=f. Gaussian integration gives

ηtotal=1,ηcapture=11+β2σΩ4.\eta_{\rm total}=1, \qquad \eta_{\rm capture}= \frac{1}{\sqrt{1+\beta^2\sigma_\Omega^4}}.

Dispersion has moved part of the signal into modes the receiver rejects. Matching the receiver to the dispersed waveform, or compensating the phase, restores unit capture in this ideal example. Total converted power alone misses the problem.

With undepleted classical pumps, resonant rotating frames, and a valid rotating-wave approximation, many converters reduce to

Hconvℏ=Gab†+G∗a†b.\frac{H_{\rm conv}}{\hbar} =G a b^\dagger+G^*a^\dagger b.

Here GG has units of angular frequency. The closed two-mode Heisenberg equations are a˙=−iG∗b\dot a=-iG^*b and b˙=−iGa\dot b=-iGa, so, for constant G=∣G∣eiφG=|G|e^{i\varphi},

a(τ)=cos⁡(∣G∣τ)a(0)−ie−iφsin⁡(∣G∣τ)b(0),b(τ)=cos⁡(∣G∣τ)b(0)−ieiφsin⁡(∣G∣τ)a(0).\begin{aligned} a(\tau)&=\cos(|G|\tau)a(0) -i e^{-i\varphi}\sin(|G|\tau)b(0),\\ b(\tau)&=\cos(|G|\tau)b(0) -i e^{i\varphi}\sin(|G|\tau)a(0). \end{aligned}

At ∣G∣τ=π/2|G|\tau=\pi/2, an input ∣n⟩a∣0⟩b|n\rangle_a|0\rangle_b becomes (−ieiφ)n∣0⟩a∣n⟩b(-ie^{i\varphi})^n|0\rangle_a|n\rangle_b. The conversion probability is one, but the number-dependent phase still needs correction for an arbitrary superposition. This is why a pump phase reference is part of coherent state transfer. Lauk and colleagues review the interactions that produce this effective Hamiltonian.

Conversion through an intermediate oscillator

Section titled “Conversion through an intermediate oscillator”

Consider two signal resonators a,ba,b coupled to an intermediate mode mm by number-conserving couplings Ga,GbG_a,G_b. Let κa,κb\kappa_a,\kappa_b be total photon-number decay rates and γm\gamma_m the intermediary’s number decay rate; field amplitudes decay at half these rates. Define

Ca=4∣Ga∣2κaγm,Cb=4∣Gb∣2κbγm.C_a=\frac{4|G_a|^2}{\kappa_a\gamma_m}, \qquad C_b=\frac{4|G_b|^2}{\kappa_b\gamma_m}.

For steady, resonant, weak signals in the passive linear model, solving the three Langevin equations gives

ηdevice=ηa,extηb,extηint,ηint=4CaCb(1+Ca+Cb)2,ηj,ext=κj,extκj.\begin{aligned} \eta_{\rm device} &=\eta_{a,\rm ext}\eta_{b,\rm ext}\eta_{\rm int}, \\ \eta_{\rm int} &=\frac{4C_aC_b}{(1+C_a+C_b)^2}, \\ \eta_{j,\rm ext}&=\frac{\kappa_{j,\rm ext}}{\kappa_j}. \end{aligned}

This is a photon-flux efficiency, not an optical-to-microwave power ratio. The derivation assumes Markov damping, no unwanted parametric gain, and signals narrow enough to use the on-resonance value. In a mechanical device, red-detuned drives and resolved sidebands can justify the number-conserving approximation. Off resonance, counter-rotating processes, heating, and finite pulses require the frequency-dependent model rather than this scalar formula.

Eliminating the signal amplitudes at resonance shows the origin of the denominator: the intermediary’s inverse susceptibility is γm(1+Ca+Cb)/2\gamma_m(1+C_a+C_b)/2. Both couplings help transfer a signal, but increasing one alone also changes the intermediary’s response. At fixed CaC_a,

∂ηint∂Cb=4Ca(1+Ca−Cb)(1+Ca+Cb)3,Cbopt=1+Ca,ηintmax=Ca1+Ca.\begin{aligned} \frac{\partial\eta_{\rm int}}{\partial C_b} &=\frac{4C_a(1+C_a-C_b)}{(1+C_a+C_b)^3}, \\ C_b^{\rm opt}&=1+C_a, \qquad \eta_{\rm int}^{\rm max}=\frac{C_a}{1+C_a}. \end{aligned}

Equal, large cooperativities approach unit efficiency. At finite fixed CaC_a, however, exact optimal matching includes the intermediary’s intrinsic loss: Cb=CaC_b=C_a is only an approximation. Pumping the second leg arbitrarily hard eventually reduces conversion. Andrews and colleagues and the Lauk review describe this mechanism.

Conversion efficiency as a function of the second cooperativity, with peaks at two and eleven for first cooperativities one and ten.

On-resonance internal photon conversion in the passive three-mode model. At fixed CaC_a, increasing CbC_b helps only up to Cb=1+CaC_b=1+C_a; beyond that point the two conversion legs become mismatched. The horizontal axis is logarithmic. External coupling loss and added thermal photons are not included.

The thermal occupation of a mode at angular frequency ω\omega is

nˉth=1eℏω/(kBT)−1.\bar n_{\rm th}= \frac{1}{e^{\hbar\omega/(k_{\rm B}T)}-1}.

At ordinary laboratory temperatures optical modes have negligible thermal occupation. A well-thermalized 5 GHz5\ {\rm GHz} mode at 20 mK20\ {\rm mK} is also nearly in vacuum, whereas a 10 MHz10\ {\rm MHz} mechanical mode at the same temperature has nˉth≃41\bar n_{\rm th}\simeq41. Mechanical damping and cooling must therefore be evaluated at the actual mode frequency. Pump absorption can raise local occupation above the refrigerator thermometer’s value.

For one specified input/output mode pair with signal transmission η>0\eta>0, use the normally ordered photon-number convention

nadd=nout(0)η.n_{\rm add}=\frac{n_{\rm out}^{(0)}}{\eta}.

Here nout(0)n_{\rm out}^{(0)} is the physical output occupation with vacuum signal input and the converter operating, including its pumps. Vacuum contributes zero in this convention. A separately calibrated detector background can be removed when inferring the converter’s output; pump-induced photons cannot be subtracted away while claiming a quieter physical channel. Symmetrized quadrature-noise conventions contain vacuum half-quanta and must be converted before comparison. Zeuthen and colleagues formulate the signal/noise distinction for linear transducers.

For a phase-insensitive thermal attenuator,

b=η a+1−η e,nadd=(1−η)nˉeη,\begin{aligned} b&=\sqrt\eta\,a+\sqrt{1-\eta}\,e, \\ n_{\rm add}&=\frac{(1-\eta)\bar n_e}{\eta}, \end{aligned}

where 0<η<10<\eta<1 and ee is an independent thermal mode. Holevo’s Gaussian channel criterion gives a precise threshold in this model: it is entanglement breaking exactly when nadd≥1n_{\rm add}\ge1. Below that threshold, some input entanglement can survive, but high-fidelity transfer and a positive unassisted quantum capacity do not follow. For example, pure loss has nadd=0n_{\rm add}=0 even at very low transmission. A noise number alone does not establish that an arbitrary, possibly non-Gaussian or phase-sensitive device obeys the thermal-attenuator model.

Pure loss also does not literally replace every input by vacuum with a state-independent probability. A coherent state remains a pure attenuated coherent state. For a single-rail qubit it is amplitude damping, with Kraus operators

K0=∣0⟩⟨0∣+η∣1⟩⟨1∣,K1=1−η∣0⟩⟨1∣.\begin{aligned} K_0&=|0\rangle\langle0|+\sqrt\eta|1\rangle\langle1|, \\ K_1&=\sqrt{1-\eta}|0\rangle\langle1|. \end{aligned}

The average fidelity to ideal transfer over Haar-uniform pure qubits is

Favg=2+∑j∣Tr⁡Kj∣26=3+2η+η6.F_{\rm avg} =\frac{2+\sum_j|\operatorname{Tr}K_j|^2}{6} =\frac{3+2\sqrt\eta+\eta}{6}.

This includes all trials and assumes vacuum environment, matched modes, and corrected phase. It is not a conditional detected-photon benchmark. With thermal noise, extra photons can also leave the qubit subspace.

For independent, phase-insensitive stages satisfying nout,j=ηj(nin,j+nj)n_{{\rm out},j}=\eta_j(n_{{\rm in},j}+n_j) in compatible modes,

naddtotal=n1+n2η1+n3η1η2+⋯ .n_{\rm add}^{\rm total} =n_1+\frac{n_2}{\eta_1} +\frac{n_3}{\eta_1\eta_2}+\cdots.

This follows by substituting each output occupation into the next stage’s input. Earlier loss makes later noise larger when referred back to the original input. Correlated reservoirs, phase-sensitive noise, or frequency mixing require covariance matrices or a full channel model instead.

Likewise, scalar transmissions multiply only for successive matched modes without coherent feedback or multiple-path interference. Two 10%10\% converters and a 50%50\% fibre path then yield 0.5%0.5\% transmission. Input coupling, filters, and final capture further reduce it. Quoting only internal conversion leaves out these losses. Power transmission differs from photon transmission by ωout/ωin\omega_{\rm out}/\omega_{\rm in}, with energy supplied or removed by the pump.

For suitable phase-matched three-wave mixing in a second-order nonlinear medium, a classical pump can produce ωout=ωin±ωp\omega_{\rm out}=\omega_{\rm in}\pm\omega_p. Four-wave Bragg scattering instead exchanges photons between two pumps:

ωout=ωin+ωp1−ωp2.\omega_{\rm out}=\omega_{\rm in}+\omega_{p1}-\omega_{p2}.

Both processes can yield the number-conserving interaction above. In contrast, degenerate-pump pair generation with ωs+ωi=2ωp\omega_s+\omega_i=2\omega_p produces a signal–idler pair and has a two-mode-squeezing interaction. These are different uses of nonlinear mixing, with different vacuum-noise consequences. Tanzilli and colleagues and McGuinness and colleagues provide examples of state-preserving optical frequency conversion.

Polarization conversion requires matched amplitudes and phases for both polarizations; time-bin conversion requires pump coherence between bins; frequency-bin conversion requires controlled relative spectral phases. Strong pumps can add leakage, Raman photons, and spontaneous pairs. Filtering suppresses some noise but can also reduce capture and distort the waveform. Conversion to telecom wavelengths is helpful only when the resulting fibre advantage outweighs these additional losses and noise for the intended task.

Microwave, mechanical, and atomic interfaces

Section titled “Microwave, mechanical, and atomic interfaces”
Mechanism How the modes couple Main physical constraint
Direct microwave link Shaped emission into a cold line and absorption at another circuit Thermal photons, reflections, and capture shape
Electro-optic conversion A classical optical pump enhances a Pockels interaction Weak vacuum coupling, resonance matching, optical heating
Mechanical intermediary Electrical or piezoelectric coupling and optomechanical coupling share a vibrational mode Thermal occupation, sideband resolution, and matching the two conversion legs
Atomic or spin-mediated conversion Driven transitions connect microwave and optical excitations Population preparation, line broadening, spatial overlap, and fluorescence
Matter–photon interface State-dependent emission entangles a stationary qubit with light Collection efficiency and photon indistinguishability

In a direct microwave link, tunable couplers can shape emission for time-reversed absorption. The line and its terminations must remain cold; attenuation at a warm stage injects thermal noise. Cryogenic packaging, isolation, and propagation delay matter even without frequency conversion.

Electro-optic devices avoid a mechanical intermediary. Mechanical devices can provide strong enhanced coupling, but a cold refrigerator is insufficient when the mechanical frequency is low or pump absorption heats the device. Pulsing can reduce average heat at the cost of recovery time and repetition rate. The Han review and Clerk and colleagues develop these alternatives; Mirhosseini and colleagues illustrate coupling a superconducting qubit to a mechanically mediated optical converter.

An ensemble’s collective coupling is gcol=∑j∣gj∣2g_{\rm col}=\sqrt{\sum_j|g_j|^2} for a properly prepared common ground state and a bright single-excitation mode. It becomes N∣g∣\sqrt N|g| only for equal couplings. This enhancement does not automatically apply to every leg of a multilevel conversion scheme: the populations and the two states connected by that leg matter. Inhomogeneous detunings can transfer the bright excitation into dark collective modes. Cavity QED and Cavity and Circuit QED Frontiers explain the light–matter and hybrid-system mechanisms.

For two independent matter–photon nodes, brightness alone is insufficient. The photons must overlap in spectrum, polarization, and arrival time at the joint measurement. Spectral diffusion, phonon sidebands, and multiphoton emission can degrade the heralded memory state. Photonic Qubits develops interference and detection; Defect and Solid-State Spin Qubits discusses representative emitters.

From a transfer probability to a usable rate

Section titled “From a transfer probability to a usable rate”

Suppose independent attempts, each with acceptance probability pp, repeat once per fixed interval τ\tau. The interval includes all preparation, notification, and reset that prevent the next attempt. In this model,

R=pτ,E[Tfirst]=τp.R=\frac p\tau, \qquad \mathbb E[T_{\rm first}]=\frac\tau p.

These are consequences of a Bernoulli sequence and a geometric waiting time, not general bounds for arbitrary queues, correlated attempts, or pipelined hardware. The propagation time and the classical return path also depend on where the herald is generated. A midpoint station and a far-end receiver have different notification delays; Quantum Memories gives explicit examples.

For MM independent usable modes in one round,

P≥1=1−(1−p)M,E[Nsuccesses]=Mp.\begin{aligned} P_{\ge1}&=1-(1-p)^M, \\ \mathbb E[N_{\rm successes}]&=Mp. \end{aligned}

The first quantity describes availability of at least one success; the second counts all successes. A receiver that can store only one cannot use the latter as its delivered-pair probability. Mode preparation, switching, detector recovery, memory capacity, and controller timing can all limit multiplexing. See Modular Architectures and Quantum Network Architectures for scheduling and multi-node operation. Kimble gives the broader network setting for these matter–photon interfaces.

Useful measurements therefore pair transfer and noise with a specified mode, input ensemble, phase reference, and trial count. Measure the operating pump noise, not just the pump-off detector floor; include rejected trials in rates and distinguish them from accepted-state fidelity. Check the two directions separately when reflections or pump leakage can disturb the source. These physical tests establish what the link can preserve, beyond showing a coherent output tone.

A source emits into a line with probability 0.820.82. Input coupling to a converter is 0.700.70, internal conversion is 0.550.55, output coupling and filtering together are 0.600.60, fibre transmission is 0.400.40, and target capture is 0.750.75. Find the end-to-end transmission.

Solution

The reference-plane factors multiply:

ηe2e=(0.82)(0.70)(0.55)×(0.60)(0.40)(0.75)≃0.0568.\begin{aligned} \eta_{\rm e2e} &= (0.82)(0.70)(0.55) \times (0.60)(0.40)(0.75)\\ &\simeq 0.0568. \end{aligned}

Only about 5.7%5.7\% of source-module trials produce a captured target excitation. Quoting the 55%55\% internal conversion alone would overstate the link transmission by nearly a factor of ten.

Two stages have η1=0.25\eta_1=0.25, η2=0.50\eta_2=0.50, and input-referred added noises n1=0.05n_1=0.05, n2=0.10n_2=0.10. What is the total added noise referred to the first input?

Solution

For two stages,

naddtot=n1+n2η1=0.05+0.100.25=0.45.\begin{aligned} n_{\rm add}^{\rm tot} &= n_1 + \frac{n_2}{\eta_1} \\ &= 0.05 + \frac{0.10}{0.25} \\ &= 0.45. \end{aligned}

The second stage’s noise is magnified by the first stage’s loss. The second stage does not contribute merely 0.100.10 when the result is referred to the original source.

Using h/kB≃48.0 mK/GHzh/k_{\rm B}\simeq48.0\ {\rm mK/GHz}, estimate the thermal occupation of a 5 GHz5\ {\rm GHz} mode at 20 mK20\ {\rm mK} and at 4 K4\ {\rm K}.

Solution

The dimensionless ratio is

hνkBT=(48.0 mK/GHz)(5 GHz)T.\frac{h\nu}{k_{\rm B}T} = \frac{ (48.0\ {\rm mK/GHz})(5\ {\rm GHz}) }{ T }.

At 20 mK20\ {\rm mK} the ratio is 1212, so

nˉth≃1e12−1≃6.1×10−6.\bar n_{\rm th} \simeq \frac{1}{e^{12}-1} \simeq 6.1\times10^{-6}.

At 4 K4\ {\rm K} the ratio is 0.0600.060, so

nˉth≃1e0.060−1≃16.2.\bar n_{\rm th} \simeq \frac{1}{e^{0.060}-1} \simeq 16.2.

The same frequency is nearly in its ground state at a well-thermalized 20 mK20\ {\rm mK} port and highly occupied at 4 K4\ {\rm K}.

Evaluate the idealized internal efficiency for (Ca,Cb)=(10,10)(C_a,C_b)=(10,10) and (10,2)(10,2). Then optimize CbC_b with Ca=10C_a=10 held fixed.

Solution

For equal cooperativities,

ηint=4(10)(10)(1+10+10)2=400441≃0.907.\eta_{\rm int} = \frac{4(10)(10)}{(1+10+10)^2} = \frac{400}{441} \simeq 0.907.

For the mismatched case,

ηint=4(10)(2)(1+10+2)2=80169≃0.473.\eta_{\rm int} = \frac{4(10)(2)}{(1+10+2)^2} = \frac{80}{169} \simeq 0.473.

At fixed Ca=10C_a=10, the derivative changes sign at Cb=11C_b=11, where ηint=10/11≃0.909\eta_{\rm int}=10/11\simeq0.909. Equal cooperativities are close to, but not exactly at, this finite-cooperativity optimum. Increasing CbC_b beyond 1111 decreases conversion in this model.

5. Convert pure loss to average qubit fidelity

Section titled “5. Convert pure loss to average qubit fidelity”

An otherwise ideal single-rail transfer has survival probability η=0.36\eta=0.36. Find the average fidelity to the identity for uniformly distributed input qubit states.

Solution

Because η=0.60\sqrt{\eta}=0.60,

Favg=3+2η+η6=3+1.20+0.366=0.76.\begin{aligned} F_{\rm avg} &= \frac{3+2\sqrt{\eta}+\eta}{6} \\ &= \frac{3+1.20+0.36}{6} \\ &= 0.76. \end{aligned}

This 76%76\% includes amplitude damping. Selecting only trials in which a photon is detected selects the logical ∣1⟩|1\rangle component and destroys an unknown single-rail superposition. It is not a successful heralded transfer of that qubit. Loss flagging must be analyzed with the encoding and the measurement backaction included.

The emitted and accepted modes are normalized and have overlap μ=0.92ei0.3\mu=0.92e^{i0.3}. What fraction of the emitted excitation is in the accepted mode? What does the phase mean?

Solution

The mode efficiency is

ηmode=∣μ∣2=(0.92)2≃0.846.\eta_{\rm mode} = |\mu|^2 = (0.92)^2 \simeq 0.846.

About 84.6%84.6\% lies in the accepted mode. The phase 0.30.3 radians is a coherent phase shift of that mode. It can be corrected if stable and calibrated; random drift would instead cause dephasing.

Each node produces a usable photon with probability 0.120.12 per attempt. Each path and detector together transmit with probability 0.250.25. A linear-optical Bell measurement succeeds for half of the two-photon arrivals. Attempts occur at 20 kHz20\ {\rm kHz}. Ignore dark events and dead time. Find the heralding rate.

Solution

The probability for one node to deliver a detected photon is

p1=(0.12)(0.25)=0.03.p_1 = (0.12)(0.25) = 0.03.

The two-photon acceptance probability is

pacc=12p12=12(0.03)2=4.5×10−4.p_{\rm acc} = \frac12 p_1^2 = \frac12(0.03)^2 = 4.5\times10^{-4}.

Therefore

Racc=(2.0×104 s−1)(4.5×10−4)=9 s−1.\begin{aligned} R_{\rm acc} &= (2.0\times10^4\ {\rm s}^{-1}) (4.5\times10^{-4}) \\ &= 9\ {\rm s}^{-1}. \end{aligned}

The two paths were assumed independent, and the one-half Bell acceptance was specified for this measurement. The quadratic dependence makes modest source or path losses expensive; it is not the scaling of every heralding protocol.

Each of M=20M=20 independent frequency bins succeeds with probability p=0.015p=0.015 in one round. Find the probability of at least one success and compare it with the small-MpMp approximation.

Solution

The exact probability is

P≥1=1−(1−0.015)20=1−(0.985)20≃0.261.\begin{aligned} P_{\ge1} &= 1-(1-0.015)^{20} \\ &= 1-(0.985)^{20} \\ &\simeq 0.261. \end{aligned}

The linear approximation gives Mp=0.30Mp=0.30. It overestimates the exact result because it counts multiple successes in the same round separately. The expected number of successes is exactly 0.300.30; it is not the probability of at least one success.

A converter has internal efficiency 0.800.80 and internal input-referred noise 0.40.4 photons. Add vacuum-loss input coupling 0.050.05 and output coupling 0.100.10. Find the external signal efficiency and external input-referred noise, assuming independent matched stages.

Solution

The external efficiency is

ηext=(0.05)(0.80)(0.10)=0.004.\eta_{\rm ext}=(0.05)(0.80)(0.10)=0.004.

For vacuum external input the converter generates 0.80(0.4)=0.320.80(0.4)=0.32 photons at its internal output; 0.10(0.32)=0.0320.10(0.32)=0.032 reach the external output. Thus

naddext=0.0320.004=8.n_{\rm add}^{\rm ext}=\frac{0.032}{0.004}=8.

Output loss attenuates signal and noise equally in this ratio. Input loss attenuates the signal before the internal noise is introduced. Consequently, the internal “less than one added photon” statement does not survive moving the input reference plane. If the full channel is a phase-insensitive thermal attenuator, this external channel is entanglement breaking. Without that model, two scalar measurements alone do not determine its entire action.

For G=∣G∣eiφG=|G|e^{i\varphi} and ∣G∣τ=π/2|G|\tau=\pi/2, find the output of (α∣0⟩a+β∣1⟩a)∣0⟩b(\alpha|0\rangle_a+\beta|1\rangle_a)|0\rangle_b. Give a number-phase rotation that restores the input amplitudes at bb.

Solution

In the one-excitation basis (∣1,0⟩,∣0,1⟩)(|1,0\rangle,|0,1\rangle),

H/ℏ=(0G∗G0).H/\hbar=\begin{pmatrix}0&G^*\\G&0\end{pmatrix}.

Exponentiating at the swap time gives

∣0⟩a(α∣0⟩b−ieiφβ∣1⟩b).|0\rangle_a\bigl(\alpha|0\rangle_b-ie^{i\varphi}\beta|1\rangle_b\bigr).

Apply exp⁡[i(π/2−φ)nb]\exp[i(\pi/2-\varphi)n_b]. The same correction removes the factor (−ieiφ)n(-ie^{i\varphi})^n for every number state, so it also works for a bosonic superposition within the ideal two-mode model. Conversion probability cannot detect a sign error in this phase; a superposition measurement can.

11. Distinguish dispersion from photon loss

Section titled “11. Distinguish dispersion from photon loss”

A normalized photon has Gaussian spectral intensity with variance σΩ2\sigma_\Omega^2. A converter adds only the phase eiβΩ2/2e^{i\beta\Omega^2/2}. For βσΩ2=3\beta\sigma_\Omega^2=\sqrt3, calculate the captured probability in the original mode and the total transmitted probability. How can capture be recovered?

Solution

Writing x=Ω/σΩx=\Omega/\sigma_\Omega and c=βσΩ2c=\beta\sigma_\Omega^2,

μ=12π∫dx e−(1−ic)x2/2=(1−ic)−1/2.\begin{aligned} \mu&=\frac{1}{\sqrt{2\pi}}\int dx\,e^{-(1-ic)x^2/2} \\ &=(1-ic)^{-1/2}. \end{aligned}

Hence ∣μ∣2=(1+c2)−1/2=1/2|\mu|^2=(1+c^2)^{-1/2}=1/2, whereas total transmission is one. Half of the probability is in modes orthogonal to the receiver’s original mode. Compensating the known spectral phase or changing the receiver to g(Ω)=eiβΩ2/2f(Ω)g(\Omega)=e^{i\beta\Omega^2/2}f(\Omega) recovers unit capture. This recovery is possible because the example contains coherent distortion alone, not absorption or uncontrolled phase fluctuations.

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