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Exponential enhancement of multi-photon entanglement rate via quantum interference buffering Evan Meyer-Scott, 1 Nidhin Prasannan, 1 Ish Dhand, 2 Christof Eigner, 1 Viktor Quiring, 1 Sonja Barkhofen, 1 Benjamin Brecht, 1 Martin B. Plenio, 2 and Christine Silberhorn 1 1 Integrated Quantum Optics Group, Applied Physics, University of Paderborn, 33098 Paderborn, Germany 2 Institut f¨ ur Theoretische Physik and Center for Integrated Quantum Science and Technology (IQST), University of Ulm, 89069 Ulm, Germany Multi-photon entangled states of light are key to advancing quantum communication [1, 2], com- putation [3], and metrology [4]. Current meth- ods for building such states are based on stitch- ing together photons from probabilistic sources [5, 6]. The probability of N such sources firing simultaneously decreases exponentially with N [7], imposing severe limitations on the practically achievable number of coincident photons [6]. We tackle this challenge with a quantum interference buffer (QIB), which combines three functionali- ties: firstly, it stores polarization qubits, enabling the use of polarization-entangled states as re- source; secondly, it implements entangled-source multiplexing, greatly enhancing the resource- state generation rates; thirdly, it implements time-multiplexed, on-demand linear optical net- works for interfering subsequent states. Using the QIB, we multiplex 21 Bell-state sources and demonstrate a nine-fold enhancement in the gen- eration rate of four-photon GHZ states. The en- hancement scales exponentially with the photon number; larger states benefit more strongly. Mul- tiplexed photon entanglement and interference will find diverse applications in quantum photon- ics, allowing for practical realisations of multi- photon protocols. textitIntroduction – Entangling multi-partite quantum systems is an important task in quantum technologies [8], where large entangled photonic states are key to multi- party communication. They provide a distinct advantage over pairwise entanglement [9], if the cost of the multi- photon state preparation is not too high [10]. Large entangled states are also critical for obtaining a quan- tum advantage in cluster-state linear optical quantum computation [11] and quantum-enhanced metrology [12]. Current sources of multi-photon entangled states do not fulfill the demanding requirements of these applications, because they are primarily based on the simultaneous generation of many entangled photon pairs and their subsequent interference in linear optical networks. A prime example for this is the probabilistic generation of multi-photon GHZ states [5, 6], where N photon pairs are probabilistically combined to produce a 2N -photon state. Typically, individual sources generate entangled photon pairs with probability p 1. The probability of N sources producing pairs simultaneously in an average number of M trials is then Mp N ; it decreases exponentially with increasing number of sources. This scaling can be overcome by source multiplexing, which refers to the method of using multiple effective sources and feed-forward to increase generation rates. This idea has initially been put forward for the generation of single photons [13] but generalises to other states (e.g. photon pairs), given that heralding is possible. When a generation event is heralded from one source, the gener- ated photon pair (or a part thereof) is stored in a quantum memory. This is implemented for all N sources, giving each source M chances to produce a pair; after all sources have fired, the stored states are released and processed further. In this case, the generation probability grows as (Mp) N , thus providing an M N-1 enhancement [14]. To date, source multiplexing has been demonstrated for the enhanced generation of heralded single photons [1416]. Entangled state multiplexing, however, is still an outstanding challenge. Independently of this, the storage of polarization qubits – a requirement for the mul- tiplexed generation of polarization-entangled states – has only been demonstrated in solid state quantum memories [1720], which cannot yet implement entangled-source multiplexing due to low efficiencies and/or low rates. Fi- nally, time-multiplexing, which exploits many time bins as opposed to the more typical spatial modes as qubit register, has been shown to facilitate the resource efficient implementation of linear optical networks; by cycling through a loop architecture, the networks become inher- ently stable and homogeneous [2123]. But they have so far been limited to interfering consecutive time bins. Examples of such networks have been used for generat- ing GHZ states, however without the rate enhancement provided by source multiplexing [24, 25]. Here, we introduce the quantum interference buffer (QIB), a device that brings together all the above func- tionalities and enables the multiplexed generation of multi- photon entangled states. The QIB combines efficient and low-noise polarization qubit storage, entangled-source multiplexing, and feed-forward time-multiplexed linear optical networks. It thus facilitates the resource-efficient generation of large entangled states while at the same time keeping the experimental overhead constant regardless of the size of the generated states. Operating scheme – The operating scheme of the QIB is summarised in Fig. 1. We focus on the generation of 2N -photon shared GHZ states, where Alice keeps N arXiv:1908.05722v1 [quant-ph] 15 Aug 2019

N arXiv:1908.05722v1 [quant-ph] 15 Aug 2019 · Exponential enhancement of multi-photon entanglement rate via quantum interference bu ering Evan Meyer-Scott, 1Nidhin Prasannan, Ish

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  • Exponential enhancement of multi-photon entanglement rate via quantuminterference buffering

    Evan Meyer-Scott,1 Nidhin Prasannan,1 Ish Dhand,2 Christof Eigner,1 Viktor Quiring,1

    Sonja Barkhofen,1 Benjamin Brecht,1 Martin B. Plenio,2 and Christine Silberhorn1

    1Integrated Quantum Optics Group, Applied Physics,University of Paderborn, 33098 Paderborn, Germany

    2Institut für Theoretische Physik and Center for Integrated QuantumScience and Technology (IQST), University of Ulm, 89069 Ulm, Germany

    Multi-photon entangled states of light are keyto advancing quantum communication [1, 2], com-putation [3], and metrology [4]. Current meth-ods for building such states are based on stitch-ing together photons from probabilistic sources[5, 6]. The probability of N such sources firingsimultaneously decreases exponentially with N[7], imposing severe limitations on the practicallyachievable number of coincident photons [6]. Wetackle this challenge with a quantum interferencebuffer (QIB), which combines three functionali-ties: firstly, it stores polarization qubits, enablingthe use of polarization-entangled states as re-source; secondly, it implements entangled-sourcemultiplexing, greatly enhancing the resource-state generation rates; thirdly, it implementstime-multiplexed, on-demand linear optical net-works for interfering subsequent states. Usingthe QIB, we multiplex 21 Bell-state sources anddemonstrate a nine-fold enhancement in the gen-eration rate of four-photon GHZ states. The en-hancement scales exponentially with the photonnumber; larger states benefit more strongly. Mul-tiplexed photon entanglement and interferencewill find diverse applications in quantum photon-ics, allowing for practical realisations of multi-photon protocols.

    textitIntroduction – Entangling multi-partite quantumsystems is an important task in quantum technologies [8],where large entangled photonic states are key to multi-party communication. They provide a distinct advantageover pairwise entanglement [9], if the cost of the multi-photon state preparation is not too high [10]. Largeentangled states are also critical for obtaining a quan-tum advantage in cluster-state linear optical quantumcomputation [11] and quantum-enhanced metrology [12].

    Current sources of multi-photon entangled states do notfulfill the demanding requirements of these applications,because they are primarily based on the simultaneousgeneration of many entangled photon pairs and theirsubsequent interference in linear optical networks. Aprime example for this is the probabilistic generation ofmulti-photon GHZ states [5, 6], where N photon pairs areprobabilistically combined to produce a 2N -photon state.Typically, individual sources generate entangled photonpairs with probability p� 1. The probability ofN sourcesproducing pairs simultaneously in an average number of

    M trials is then MpN ; it decreases exponentially withincreasing number of sources.

    This scaling can be overcome by source multiplexing,which refers to the method of using multiple effectivesources and feed-forward to increase generation rates.This idea has initially been put forward for the generationof single photons [13] but generalises to other states (e.g.photon pairs), given that heralding is possible. When ageneration event is heralded from one source, the gener-ated photon pair (or a part thereof) is stored in a quantummemory. This is implemented for all N sources, givingeach source M chances to produce a pair; after all sourceshave fired, the stored states are released and processedfurther. In this case, the generation probability grows as(Mp)N , thus providing an MN−1 enhancement [14].

    To date, source multiplexing has been demonstratedfor the enhanced generation of heralded single photons[14–16]. Entangled state multiplexing, however, is stillan outstanding challenge. Independently of this, thestorage of polarization qubits – a requirement for the mul-tiplexed generation of polarization-entangled states – hasonly been demonstrated in solid state quantum memories[17–20], which cannot yet implement entangled-sourcemultiplexing due to low efficiencies and/or low rates. Fi-nally, time-multiplexing, which exploits many time binsas opposed to the more typical spatial modes as qubitregister, has been shown to facilitate the resource efficientimplementation of linear optical networks; by cyclingthrough a loop architecture, the networks become inher-ently stable and homogeneous [21–23]. But they haveso far been limited to interfering consecutive time bins.Examples of such networks have been used for generat-ing GHZ states, however without the rate enhancementprovided by source multiplexing [24, 25].

    Here, we introduce the quantum interference buffer(QIB), a device that brings together all the above func-tionalities and enables the multiplexed generation of multi-photon entangled states. The QIB combines efficient andlow-noise polarization qubit storage, entangled-sourcemultiplexing, and feed-forward time-multiplexed linearoptical networks. It thus facilitates the resource-efficientgeneration of large entangled states while at the same timekeeping the experimental overhead constant regardless ofthe size of the generated states.Operating scheme – The operating scheme of the QIB

    is summarised in Fig. 1. We focus on the generationof 2N -photon shared GHZ states, where Alice keeps N

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    c Experimental setup

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    FIG. 1. Operating principle of the QIB and experimental setup. a, Spatial realisation of source-multiplexed GHZ stategeneration. A 1×N switchyard routes a train of pump pulses to N entanglement sources. First, source 1 is pumped. When aBell-pair is generated, one photon is detected, whilst the other is stored in a quantum memory. Then the pump is switched tosource 2; this optimises the usage of pump power. This repeats until all N sources have fired, after which the stored photons arereleased and interfere pairwise in a linear optical network, whose outputs can be routed to N Bobs for entanglement sharing.The detection of a specific output pattern then confirms the successful generation of a GHZ state. b, The unique capabilitiesof the QIB facilitate a source-multiplexed and resource efficient setup. A stream of pulses pumps a single physical Bell-statesource. The detection of a herald photon triggers the storage of its sibling in the QIB, thus implementing source multiplexing.Subsequent detection of the next photon switches the QIB to interference, after which one photon leaves the QIB whereas one isbuffered; this is the time-multiplexed optical network. In this way, multi-photon GHZ states are subsequently built up. Afterthe herald detection and interference, the final photon is released from the QIB. Post-selection of one photon in each outputtime bin confirms the presence of the complete 2N -photon GHZ state. c, Experimental setup comprised of entangled photonpair source (green), qubit interference buffer (blue), and polarization analysis stages (yellow). For more information see the textand supplemental.

    photons for herself and sends the other N photons todistinct Bobs. Fig. 1a shows a spatially multiplexedapproach optimised for efficient use of pump power, whichperforms a similar operation as the QIB but experiencesa highly unfavourable scaling of experimental overheads;each additional pair of the final state requires its ownphysical source and memory and leads to reduced rates.Fig. 1b depicts the implementation of the QIB in time,maintaining optimal use of pump power. It is basedon source-multiplexed generation of Bell pairs and theirtime-multiplexed interference. The number of physicalresources is constant regardless of the size of the final

    GHZ state.

    Our experimental setup is shown in Fig. 1c. The Bell-state source is realised in a KTP waveguide in a Sagnacconfiguration, which is bidirectionally pumped with pulsesfrom a Ti:Sapph oscillator [26]. One of the photons issent to a polarization resolving detection stage, the otheris routed to the QIB. The QIB comprises another Sagnacloop and a retroreflective delay line, connected via apolarizing beam splitter. The internal roundtrip time ofthe QIB of 13.16 ns is synchronised to the repetition rateof the Ti:Sapph oscillator. Inside the QIB Sagnac loop,an electro-optic modulator (EOM) is triggered by feed-

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    FIG. 2. Results for storage of single and entangled qubits for up to 1 µs. a, The post-storage fidelity of polarizationqubits decreases slowly, in particular the minimum average fidelity is (97.8± 1.0) % in the region up to 20 roundtrips relevantfor GHZ state production. The model curves include multipair emissions, roundtrip losses, and a small imperfection in thequarter-wave plate angle of 0.27◦. b, The memory efficiency of the QIB falls exponentially with a roundtrip efficiency of(90.57± 0.06) % extracted from the fit, slightly below the single roundtrip value of 91.7 % (see supplemental) due to imperfectspatial mode matching at large storage times. The total efficiency is the efficiency to retrieve a photon at the polarizationanalysis stage (3) given one was present in the fibre at the source (1), cf. Fig. 1. The memory efficiency has the losses thataccrue even without activating buffer function (circulator, coupling losses) removed. c, HOM visibilities resulting from theinterference of two heralded photons one of which has been stored in the buffer for the given storage time before being interferedwith the other. The model curve assumes no imperfections except for asymmetric losses from storing one photon that is, thestored photon expects loss in the QIB which the freshly generated one does not. All error bars originate from Poissoniancounting statistics, apart from average fidelity, which comes from the standard deviation of the fidelity across the six input basisstates. Here as in all data presented, no accidental counts have been subtracted.

    forward logic from an FPGA, which in turn is triggered bythe detection of herald photons. The setting of the EOMdetermines the function of the QIB: fill and empty thestorage loop; buffer photons inside the loop; and interferea photon inside the loop with a freshly generated photon,see the supplement.

    Results – We characterise the QIB operation throughthree complementing measurements: firstly, the storage ofpolarization qubits; secondly, the storage of polarizationentanglement; finally, Hong-Ou-Mandel (HOM) interfer-ence between a stored and a freshly produced photon.For polarization-qubit storage, we generate unentangledphoton pairs, project one of the photons into a user-defined polarization state, store it for a certain numberof roundtrips, and perform a polarization tomographyafter releasing it. For the storage of entanglement, wegenerate polarization Bell pairs, store one partner of thepair, release it, and then perform a joint polarizationtomography on both photons. In the former case, wefind an average fidelity of (99.7± 0.1) % and a processfidelity of (97.72± 0.03) % for a storage time of 13.16 ns.In the latter case, the fidelity is (93.8± 0.1) %, limitedby the initial entanglement fidelity of the source, seeFig. 2a. The storage efficiency is shown in Fig. 2b, fromwhich we extract a storage efficiency of (90.57± 0.06) %.Finally, we measure the HOM interference visibilities be-tween subsequently generated photons, see Fig. 2c. Afterone roundtrip, we observe a visibility of (94.5± 1.8) % atlow pump power, limited by the source [26]. Note thatFig. 2c has been measured at high pump power for con-

    venience. The decrease in HOM visibility as a function ofthe number of roundtrips in the QIB is fully explained bythe imbalanced losses between the stored and the freshlygenerated photon.

    Next, we demonstrate the enhanced generation of four-photon GHZ states. Fig. 3a shows the main resultsof this Letter. The generation rate increases with thenumber of multiplexed sources, up to a maximum nine-fold increase for 21 multiplexed sources. At the same time,the state fidelity stays basically constant as a function ofthe number of multiplexed sources. This demonstratesthat source multiplexing with the QIB has no detrimentaleffect on the generated states. Fig. 3b highlights theincrease in four-photon GHZ state generation rate as afunction of pump power. This increase is faster for alarger number of multiplexed sources, which means thatfor a given target generation rate, the pump power canbe kept at a lower level thus reducing unwanted multi-photon components. The effect of this reduced pump-power requirement is seen in Fig. 3c, where the statefidelity for a given generation rate is always higher whenmultiplexing more sources.

    Discussion – We have demonstrated that the QIB facil-itates the multiplexed generation of multi-photon entan-gled states, increasing both the generation rate as well asthe state fidelity. Here, we will compare the QIB perfor-mance to that of other systems. All-optical polarization-independent storage loops have been proposed before, butnot yet implemented [27]. The storage efficiency of theQIB of (90.57± 0.06) % is currently slightly below that of

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    FIG. 3. Results for producing 4-photon GHZ states with QIB source multiplexing. a, With more multiplexedsources, the rate increases (sub-linearly due to roundtrip losses), up to a maximum nine times increase for 21 sources as comparedto the minimum two sources needed for four-photon GHZ. For up to 11 sources, the fidelity (inset) drops by only 3 % but therate increases 6.7 times. b, It is always possible to increase rates by increasing the pump power, where higher pump powersgenerally lead to reduced state fidelities due to multi-pair emissions. The additional benefit from multiplexing becomes obviouswhen noting that, for the case of 2 sources (i.e. no multiplexing, just 2 sources to produce 4 photons) and 11 multiplexed sources,the rate of the multiplexed source increases much faster with pump power. c, For any fourfold rate, the multiplexed source hasa higher fidelity as a result of the suppression of unwanted multi-pair emissions. For low pump powers, the fidelity increases byup to five percentage points. Error bars from Poissonian statistics are smaller than symbol size.

    other, polarization-selective storage loops [14]. This is dueto the double-pass through the polarizing beam splitterand number of mirrors used. In contrast, polarization-qubit storage has been realised in solid-state quantummemories. The QIB compares favourably to those, bothin terms of storage fidelity and operation bandwidth andwavelength (c.f. [17–20], also see the supplemental). Thelifetime of the QIB is shorter than for many solid-statequantum memories but suffices for the applications con-sidered here. We also want to highlight the outstandingnoise performance of the QIB. An established benchmarkfor this is the µ1 number, the ratio between the numberof noise photons and the memory efficiency [28]. TheQIB features a µ1 of 2.2× 10−6, with the dominant noisesource being dark counts in the detectors; a technical noisesource rather than a fundamental limitation. Finally, alimited EOM switching speed inside the QIB has limitedour demonstration to four-photon GHZ states; however,the operation principle of the QIB extends to larger states,and we expect more significant improvements for largerstates, e.g. a factor of up to 105 for 12-photon GHZstates.

    Conclusion – We have introduced a novel scheme forthe source-multiplexed and resource-efficient generation ofmulti-photon entangled states, the QIB. We have demon-

    strated polarization qubit storage with fidelities exceeding99 %, and a nine-fold increase in the generation rate offour-photon GHZ states. We predict significantly largerimprovements for larger states. In addition, the QIB isnot limited to GHZ-state generation, but can be adaptedto realise other classes of entangled states, e.g. tensornetwork states. These results put the QIB at the forefrontof approaches aiming to generate large, shared entangledstates for quantum information applications, and we ex-pect the QIB to have a large impact on future realisationsof state generation protocols.Acknowledgements – This work was supported by the

    ERC project QuPoPCoRN (no.725366), the ERC Synergygrant BioQ, the Alexander-von-Humboldt Foundation,the EU projects AsteriQs and Hyperdiamond and theBMBF projects DiaPol and Nanospin.

    Methods

    Source of entangled photon pairs. The entangledpairs are produced in a potassium titanyl phosphatewaveguide (ADVR Inc.) embedded in a Sagnac loop,pumped by a femtoscecond Ti:Sapphire laser (Mira 900f,Coherent). Full characterization of the source is provided

  • 5

    in [26]. The waveguide and pump bandwidth have beenengineered to produce nearly single-spectral-mode pho-tons, with an upper bound for the single-modeness fromthe measured joint spectral intensity of 98 %. In the cur-rent experiment the source has a Klyshko efficiency [29]of 33 % to 38 % on the heralding (Alice, signal) side, and13 % to 20 % on the QIB (Bob, idler) side, including trans-mission through the QIB. Variations are due to alignmentand differences in detector efficiency between the variouschannels. The source can produce Bell pairs with fidelityto the maximally-entangled state up to 96 %, limited byimperfect waveguide end-facet coatings [26]. The detec-tors are custom superconducting nanowire single-photondetectors from Photon Spot Inc. They have 75 % systemdetection efficiency with a dead time (98 % recovery) of13 ns.

    Quantum interference buffer. The QIB acts as anall-optical poarization-insensitive memory and reconfig-urable linear optical network. The QIB can rapidly switchbetween three functions: (i.) the store-release function, inwhich an incoming photon enters the Sagnac loop and anyphoton in the QIB exits it; (ii.) the buffer function, inwhich any photon in the QIB stays there and any incom-ing photon leaves the QIB unchanged; and finally (iii.)the interference function, in which the incoming photonand the stored photon interfere at a PBS-like interaction.

    The setup of the QIB is presented in Figure 1 in blueand comprises a retro-reflective delay line connected toa Sagnac loop. Light that enters the Sagnac loop issplit in polarization at the PBS and the two componentscounter-propagate around the loop. To realize the store-release function, the EOM is left off. Since there is nopolarization change, any light entering the Sagnac loopfrom the source gets transferred to the retro-reflective lineand vice versa.

    For the buffer function, the EOM is switched on whilethe photon is in the retro-reflective line. Then, after re-entering the Sagnac loop, both polarizations are flipped(|V 〉 → |H〉 and |H〉 → |V 〉), such that the photon isreturned to the retro-reflective line. To undo this flip,light that enters the retro-reflective line also undergoesa polarization flip thanks to a static quarter-wave plateat 45◦ passed twice. So long as the EOM remains on,the photon passes between the retro-reflective arm andSagnac loop and remains in the QIB.

    For interference, two photons enter the Sagnac loop, onefresh from the source and one from the retro-reflectiveline. Now the EOM is turned off after the clockwise-propagating components of the two photons have passedit, such that these receive a polarization flip but thecounter-clockwise components do not. This performs thesame mode-sorting action as a static PBS. For GHZ stategeneration, each photon now has a 50 % chance to leavethe QIB or return to the retro-reflective arm, leading tothe 50 % post-selection probability. To release the photonthat returned to the retro-reflective arm, the EOM is leftoff such that the photon couples out on the next roundtrip. For larger GHZ states, post-selection works when

    for each heralded photon that enters the QIB, one photonis found to exit on the next round trip.

    GHZ state measurements. We evaluate the fidelityvia the population and coherence as detailed in the sup-plement. See example raw count data and the populationand coherence in the supplement.

    Generation of tensor network states includingcluster states. In the main text, we have describedthe generation of GHZ states. The most general statesgenerated by the setup are one-dimensional tensor networkstates with bond dimension two as each of the photonsemitted from the setup has interfered with its precedingand succeeding photons at the beamsplitter. As detailedin the supplement and following the analysis of [30], such asequence of nearest-neighbour gates acting on qubits leadsto a tensor network with a bond dimension equalling thephysical dimension, which is two in this case. In particular,the setup can be modified straightforwardly to generatelinear cluster states. We also detail the generation ofcluster states using our setup in the supplement.

  • 1

    Supplementary material: Exponential enhancement of multi-photon entanglement rate via quantuminterference buffering

    Here we present detailed information about experimen-tal components and the theoretical design and analysis.The supplementary material is structured as follows. InSection S1, we describe the design of the the quantum in-terference buffer (QIB) used to store and interfere the pho-tons including a comparison with other quantum buffersand memories. Next in Sections S2 and S3, we presentthe schemes for generating GHZ and cluster states usingthe QIB in tandem with the source of entangled photonpairs. We show in Section S4 that the scheme leads toan exponential increase in the probabilities of the gen-erating N -photon entangled states. Section S5 presentsfurther details about the numerical simulations that theexperimental data is compared against. Section S6 pro-vides details about experimental aspects including feed-forwarding, timing, Pockels cells and the loss budget. Weconclude in Section S7 with additional experimental data.

    S1. ACTION OF QIB

    As described in the main text, the QIB includes thetwo actions of firstly a fast reconfigurable polarizationbeam splitter and secondly a quantum buffer. Here wedescribe the three functions that the QIB can perform.These include (i.) the store-release function, in whichan incoming photon enters the buffer and any photon inthe buffer exits it, (ii.) the buffer function, in which anyphoton in the buffer stays in the buffer and any incomingphoton leaves the QIB unchanged and finally (iii.) theinterference function, in which the incoming photon andthe stored photon interfere at a PBS-like interaction.

    In more detail, the setup of the QIB, depicted in Fig-ure S1a, comprises two key components: a fast reconfig-urable PBS (fast PBS, depicted as dashed box) and adelay line. The fast PBS is a four-port device. The twoinput ports are labelled ‘in’ and ‘from’ representing thephysical input and the mode arriving from the delay linerespectively. Likewise, the two output ports are labelled‘out’ and ‘to’ respectively, for the physical output andthe port leading towards the delay line. The fast PBSis built out of one fixed PBS, two fixed-angle half-waveplates w1 and w2, and two fast programmable electro-optic modulators (EOMSs) eom1 and eom2. The PBSand the EOMs are placed in an optical loop. In the figure,the counterpropagating paths around the Sagnac loophave been spatially separated for clarity. In other words,althought the figure depicts two spatially separated pathsfor the clockwise and anti-clockwise cycling light and thetwo EOMs acting on the spatially separated paths, in theimplementation these two paths coincide and the actionof the two EOMs is replaced by that of a single EOMwith two different settings at different times. For clarity,the setup is unravelled into the equivalent circuit depicted

    in

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    FIG. S1. Setup and action of the QIB: a, The dashed boxrepresents the fast PBS, which together with the retroreflectivedelay (red coiled line) line comprises the QIB. The blue andred lines represent paths with different colors depicting themodes cycling in different directions. b, An equivalent circuitto the fast-PBS setup. Passing time in the actual setup isrepresented as motion from left to right in this equivalentsetup.

    in Figure S1b, in which the left to right motion representsthe passage of time.

    Both wave plates are fixed at 45◦, which swaps the po-larization modes but leaves the light otherwise unchanged.Different settings of the EOM toggle different operatingfunctions of the QIB. We are interested in the followingthree functions of the QIB:

    1. If EOM eom1 is turned on to act as half-wave plateat 45◦, performing a polarization swap, but eom2 isturned off, then fast PBS effects a PBS transforma-tion between the incoming light (‘in’) and the lightstored in the buffer (‘from’). Specifically, the hor-izontal and vertical polarizations see the differenttransformations:

    |Hin〉 → |Hto〉 , |Hfrom〉 → |Hout〉 ,|Vin〉 → |Vout〉 , |Vfrom〉 → |Vto〉 .

    (S1)

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    Setup settings Operating Function

    eom1 eom2 (effected transformation)

    on off Interfere (PBS)on on Buffer (Identity)off off Store-release (Swap)

    TABLE I. Different operating functions of the QIB based ondifferent settings of the EOM.

    This is the ‘interfere’ function of the QIB.

    2. If both the EOMs are turned on to perform polar-ization swaps, then the fast PBS effects an identitytransformation between the input and the outputmodes. In other words, the light from the delay lineis directed back to the delay line and the light fromthe physical input is emitted “unchanged” from theoutput:

    |Hin〉 → |Hout〉 , |Hfrom〉 → |Hto〉 ,|Vin〉 → |Vout〉 , |Vfrom〉 → |Vto〉 .

    (S2)

    This is the buffer function, wherein light that is inthe delay line cycles in the QIB, i.e., through thefast PBS and back into the delay line, and effectivelyisolated from the input light.

    3. The final function is the store-release function,wherein light from the input ports of the fast PBS isswapped into the output ports without any changein the polarization:

    |Hin〉 → |Hto〉 , |Hfrom〉 → |Hout〉 ,|Vin〉 → |Vto〉 , |Vfrom〉 → |Vout〉 .

    (S3)

    The light stored in the QIB is released and the inputlight enters the QIB.

    Table I summarizes these three functions of the QIB.The EOMs can be programmed to toggle between thethree different functions for different incoming pulses. Dif-ferent functions of the QIB can be employed to generatephotonic entangled states with exponentially higher like-lihood as compared to usual setups as detailed in theSections S2 and S3.

    A. Comparison to quantum memories

    In this section, we aim to compare the performanceof our QIB with that of state of the art atomic quan-tum memories for polarization qubit storage. As alreadyeluded to in the main text, our performance benchmarks(except for storage time) compare favourably with atomicmemories. Some of the more recent demonstrations ofpolarization qubit storage are based on either electricallyinduced transparency (EIT) in cold caesium [19] and ru-bidium [20] ensembles, or atomic frequency combs (AFC)in neodymium [17] and europium [18].

    A comparison of performance benchmarks is given inTable II. We note that the µ1 for the atomic memoriesare extracted from the memory efficiencies and noiseproperties stated in the respective publications. Also, thestated bandwidths are the operation bandwidths, whichdo not necessarily strictly correspond to the maximumachievable memory bandwidths.

    It is to be expected that the QIB cannot compare withatomic systems with regards to memory lifetime. Wenote, however, that the lifetime of 131 ns (correspondingto 10 roundtrips in the QIB) is more than sufficient forthe applications considered here, namely the multiplexedgeneration of multi-photon entangled states. The oper-ation fidelity is state of the art and can be increased bya more precise tuning of the quarter-wave plate angle inthe retro-reflective delay line (cf. Fig. 2). Finally, theQIB outperforms other memories in terms of bandwidth,storage efficiency, and noise performance. We note thatthis is to be expected, since the bandwidth is not limitedby an atomic level structure, and there is virtually nonoise generated inside the QIB due to the absence of astrong control field. As a sidenote, we want to add thatthe QIB can, in principle, operate at any given wavelength(telecommunications wavelength in our case); this is incontrast to atomic memories, the operation wavelengthof which is governed by the atomic level structure of theunderlying material system and which, for the memoriesconsidered here, ranges between 580 nm and 880 nm.

    S2. GENERATION OF GHZ STATES

    GHZ states of 2N -photons can be generated using Nsources of entangled photon pairs, which are stitchedtogether using PBSs and post-selection [5, 6, 24, 31–33].As we have shown, a similar scheme can leverage the time-multiplexing enabled by the QIB to generate GHZ stateswith an exponential (in N) increase in the generationlikelihood.

    Our setup for generating GHZ states comprises twomain components as depicted in Fig. 1. Firstly, we use ahigh-performance source of entangled photon pairs basedon a hybrid integrated-bulk design that we have reportedin Ref. [26]. The source combines the advantages offeredby integrated sources, namely higher brightness and low-power operations, with those of bulk sources, namely highoutput-state quality and coupling efficiency. The sourceis used to generate light in the state |00〉+√p(|HH〉+|V V 〉)/

    √2, i.e., entangled photon pairs with probability

    p and vacuum otherwise.The source is connected to the QIB, which allows for

    time-multiplexing as follows. One mode (say the signalmode) of each pair is measured at a polarization-selectivedetector and either no photon is detected or a singlephoton is detected, in which case the polarization (H orV ) is known. Multi-photon emissions, in the first placekept low by pumping the source weakly, and in the secondplace partially obviated by removing the cases where both

  • 3

    Paper Type Bandwidth Efficiency Lifetime µ1 Fidelity

    [17] AFC in Nd 30 MHz ∼10 % not stated not stated 0.999[18] swAFC in Eu ∼1 MHz ∼4 % at 500 µs not stated 0.275 0.885[19] EIT in Cs 2.5 MHz ∼69 % ∼15 µs 7.2 · 10−4 0.977[20] EIT in Rb ∼0.4 MHz 86 % 3 µs 1.7 · 10−3 0.996

    This work QIB 0.52 THz 91 % 131 ns 2.2 · 10−6 0.997

    TABLE II. Comparison of performance benchmarks of state of the art atomic memories for polarization qubits and our QIB.The abbreviation swAFC signifies the full spin-wave storage protocol for an AFC on-demand memory. The µ1 number is theratio between noise photons and memory efficiency, an established performance benchmark for quantum memories. For moreinformation, see the text.

    |H〉 and |V 〉 detectors fire in the same mode, are ignoredin the subsequent analysis. The other mode, i.e., idler, ofthe pairs is impinged at the input port of the QIB andthe time delay introduced by the delay line is set equal tothe time delay between subsequent pulses emitted fromthe source.

    The first time a photon is detected in the signal mode,this information is fed forward to the EOMs in the QIB,which toggle it to the store-release function, so the photonfrom the entangled pair is directed towards the delay line.Until another photon is detected in the signal mode, theQIB is set to the buffer function. This way, the photonsent into the delay line stays cycling in the QIB.

    The next time a photon is detected in the signal mode,the QIB is switched to the interference function, and thestored light interferes with the idler mode of the generatedphoton pair. The interference results in photon pairswith same polarization having their photons emitted intodifferent outputs (one into ‘out’ and other into ‘to’) of theQIB but pairs with orthogonal polarization are emittedinto the same output port. That is, either both bunchinto ‘out’ or both into ‘to’. Only those events are post-selected in which one photon is detected in each mode.Consequently, only those two terms in which all photonshave identical polarization survive and the resulting stateis a GHZ state.

    The exponentially higher probability in N results fromthe fact that photons generated in many different pulsescan be made to interfere together. If the setup losses allowfor the cycling photon to be stored for M roundtrips,then there is an ≈MN−1-fold increase in the 2N -photongeneration likelihood. One way to see this is that each ofthe N − 1 interference events is ≈M times more likely tooccur. A detailed analysis of the generation probabilitiesis presented in Section S4.

    S3. GENERATION OF LINEAR CLUSTERSTATES

    Here we show that the QIB can be additionally ex-ploited to generate linear cluster states [34] with expo-nentially higher likelihood (in the number of photons)as compared to the situation without multiplexing. Weuse a scheme similar to that of Pilnyak et al. [25]. More

    in

    out

    tofrom

    w1w2

    eom3

    eom1

    eom2

    cw

    ccw

    FIG. S2. Generating cluster states requires an extra EOM atthe ‘from’ port of the QIB.

    specifically, the PBS in the scheme of [25] is replaced byour QIB, which is triggered by signal photons, and theoptical loop is replaced by our delay line.

    As we describe in the remainder of this section, astraightforward implementation of the scheme requires thesetup to have an extra EOM to act as a half-wave plateat 22.5◦ when there is a photon incoming and to switchoff when the QIB is to act as a buffer (See Section S3 A).The extra EOM is required to be placed after the delayline and in the ‘from’ port of the QIB as depicted inFigure S2. This EOM can be replaced by a static waveplate at the cost of reduced cluster-state generation rates(See Section S3 B).

    To generate linear cluster states, the source gener-ates photon pairs in the state |00〉 + √p |HH〉 in theleft and right modes. Here and henceforth we omit nor-malization for ease of notation. The left-going modesare detected and the detection events are only usedto herald the horizontally-polarized photon in the rightmode. The right-going modes impinge at the QIB afterpassing through a half-wave plate (w1) at 22.5

    ◦ so only|P 〉 = |H〉+ |V 〉 photons arrive at the QIB.

    The first detection of a photon in the left mode toggles

  • 4

    |H〉

    |H〉

    |0〉

    |H〉

    |H〉

    |0〉

    Interfere Buffer

    FIG. S3. Circuit for generating cluster states. Therounded dashed boxes represent the repeated action of thefast PBS and the green discs represent the EOMs at 22.5◦

    and half-wave voltage. The ordering of the fast PBS ports(clockwise starting from top left) is ‘from’, ‘out’, ‘to’ and ‘in’.At those temporal modes when a photon |H〉 is incident, theQIB is switched to the PBS function and the EOM is on. Forthe remaining temporal modes, the EOM is switched off andthe QIB acts as a buffer (depicted as rounded dashed boxwithout horizontal line). The red curve represents the modethat is cycling in the QIB. The brown circles at the outputrepresent the desired linear cluster state and the empty modesare discarded.

    the QIB to the interference function, and the reflected(‘out’) mode is discarded. This way, there is an |H〉photon in the loop with probability 1/2. The QIB isthen set to the buffer function so the |H〉 photon cyclesin the delay line and QIB. As soon as the next photonis detected in the left mode, the QIB is toggled to theinterference mode and the EOM p3 outside the loop isswitched on to its half-wave voltage at 22.5◦. After thisinterference, the QIB is switched back to the buffer modeand p3 is turned off till the next detection event at theleft mode. Post-selecting single-photon detection eventsgives the required linear cluster state.

    A. Cluster state generation with additional EOM

    Here we present more details about the cluster stategeneration procedure. The effective optical circuit forconstructing the cluster states is depicted in Fig. S3. Wewill only consider the modes in which the source emitteda photon pair as the remaining events are post-selectedout via heralding. The first interaction is between thehorizontally polarized photon |H1〉 from the buffer andthe incoming |H2〉 photon after these have undergonea polarization rotation to their respective plus states|Pi〉 = |Hi〉+ |Vi〉. Thus, the incoming state at the PBS

    is the |P1P2〉 state, or

    |H1H2〉+ |H1V2〉+ |V1H2〉+ |V1V2〉 . (S4)

    Under the action of the PBS, this state changes to

    |H2H1〉+ |H2V2〉+ |V1H1〉+ |V1V2〉 (S5)= |H1H2〉+ |H2V2〉+ |H1V1〉+ |V1V2〉 . (S6)

    As we choose states in which only one photon is emitted ineach mode, after this post selection, we need only consider

    |H1H2〉+ |V1V2〉 . (S7)

    The first qubit is emitted from the system and the secondis stored in the buffer till the next |H3〉 qubit arrives.Just before the arrival of the third qubit, the polarizationrotation at the output of the second mode converts thestate into a two qubit cluster state

    |H1H2〉+ |H1V2〉+ |V1H2〉 − |V1V2〉 . (S8)

    Before interacting, the third qubit sees a polarizationrotation, which gives

    (|H1H2〉+ |H1V2〉+ |V1H2〉 − |V1V2〉)(|H3〉+ |V3〉),(S9)

    which after the action of the PBS and post selection turnsto

    |H1H2H3〉+ |H1V2V3〉+ |V1H2H3〉 − |V1V2V3〉 . (S10)

    Once the third mode is acted upon by a polarizationrotation, this state is

    |H1H2H3〉+ |H1H2V3〉+ |H1V2H3〉 − |H1V2V3〉+ |V1H2H3〉+ |V1H2V3〉 − |V1V2H3〉+ |V1V2V3〉 , (S11)

    which is exactly the three-qubit cluster state.One can show more rigorously that the generated state

    is a linear cluster state because the input qubits are allin the |Pi〉 state. The circuit building block is a PBSfollowed by a half-wave plate at 22.5◦, and this buildingblock has the action of a controlled-phase gate on the|PiPi+1〉 qubits after post selection as can be seen from thetransformation from Eq. (S4) to Eq. (S8). This controlled-phase building block acts repeatedly on neighboring sitesthereby giving a linear cluster state [34].

    From arguments similar to those presented in the maintext and Sec. S4 A, time-multiplexing is expected to givea MN−1-fold enhancement in the success probability ofgenerating an N -mode cluster state if the circuit lossesallow for M round-trips without substantial loss in fidelity.

    B. Replacement of EOM with a static wave plate

    The EOM that implements 45◦ rotations in the clus-ter state procedure can be replaced with a static wave

  • 5

    |H〉

    |H〉

    |0〉

    |H〉

    |H〉

    |0〉

    FIG. S4. Static circuit for generating cluster states.Notice that the input of the fourth mode is a photon |H〉 butthis input is ignored as the buffer operation is incomplete. Thebrown circles represent the constituents of the multi-photonentangled state and the empty modes are discarded.

    plate at the cost of reducing the success probability butstill maintaining the exponential improvement over nonsource-multiplexed procedures. Recall that we had to usethe EOM because the phase rotation between subsequentmodes lead to an imperfect buffer function, i.e., insteadof effecting the desired identity operator, an identity fol-lowed by a Hadamard (45◦ rotation) is implemented ifthe rotation is not turned off.

    One method to circumvent this issue is based on observ-ing that the action of two such imperfect buffer operatorsis an identity operator. This means, that we retrieve thedesired identity operator if somehow the imperfect bufferoperators always occurred in pairs. We can force the im-perfect buffer operators to always act in pairs by ignoringsome of the incident modes. More precisely, subsequentto a temporal mode in which a photon is incident, wecount the number of cycles that have passed since thelast photon; if an odd number of cycles have passed, thenthe incoming mode is ignored irrespective of whether aphoton is incident or not. To ignore the incoming mode,we can switch the QIB to the buffer mode. Interferenceoccurs and the counter is reset to zero if a photon isincident in one of the even cycles.

    This situation is depicted in Fig. S4. Photons wereincident in the first and second temporal modes so theQIB is made to function as a PBS. After the second mode,the counter started and when no photon was observedin the third mode so the QIB functions as buffer andthe counter is set to 1. Because the counter is set toan odd value, the QIB is switched to buffer mode eventhough a photon was expected in the fourth mode. Nowthe counter increments to two and there is a photonexpected in the next mode so the QIB is switched toPBS mode thus resetting the counter. These previoustwo imperfect buffer operations cancel each other and anidentity operator results from the combined action of thesecond and third QIBs and EOMs, which is the desiredbehavior.

    Using a static wave plate instead of a EOM, theenhancement in the success probability because oftime-multiplexing is expected to drop from MN−1 to(M/2)N−1. This is because only half of the M feasibleround-trips, only half are relevant and the other half areignored. In the static case there are some temporal modes(when the counter is odd valued) in which a photon isemitted from the setup but this photon is not a part ofthe linear cluster state. Therefore, events involving thesetemporal modes would need to be discarded.

    In either of these two operations, an important dif-ference between our time-multiplexed GHZ generationprocedure and the time-multiplexed cluster-state proce-dure is that the signal photons in the GHZ state are apart of the full state, but the signal photons are only usedfor heralding in the linear cluster state. This means thatN photon-pair emission events will allow a generationof 2N -photon GHZ state but only an N -photon clusterstate.

    C. CPHASE gate with QIB

    Beyond effective CPHASE gates for cluster states, weshow the QIB can perform post-selected CPHASE gates ingeneral, with the addition of a fast polarization-insensitiveattenuator. We follow the prescriptions of Refs. [35, 36],giving a success probability 1/9 for each CPHASE gate.

    We describe the CPHASE operation on two generalqubits, coming from from and in, which we label 1 and2 respectively. The gate should apply a minus sign to the|V1V2〉 term and nothing else. The incoming state is

    (α1 |H1〉+ β1 |V1〉) (α2 |H2〉+ β2 |V2〉) , (S12)

    on which the mode 2 has its polarizations swapped togive

    (α1 |H1〉+ β1 |V1〉) (α2 |V2〉+ β2 |H2〉) . (S13)

    The PBS preserves the mode number for H photons, andswaps it for V photons, so the state is now

    (α1 |H1〉+ β1 |V2〉) (α2 |V1〉+ β2 |H2〉) . (S14)

    Now we apply a half-wave plate at 72.5◦ (counterclockwisefrom H) in mode 2 to produce(

    α1 |H1〉+ β1

    [−√

    2

    3|H2〉+

    √1

    3|V2〉

    ])(S15)(

    α2 |V1〉+ β2

    [√1

    3|H2〉+

    √2

    3|V2〉

    ]). (S16)

    Then we have to attenuate with transmission√

    13 in mode

    1 to even the terms out, giving

    1

    3

    (α1 |H1〉+ β1

    [−√

    2 |H2〉+ |V2〉])

    (S17)(α2 |V1〉+ β2

    [|H2〉+

    √2 |V2〉

    ]). (S18)

  • 6

    This requires that the HWP at 72.5◦ applies to mode2, but is back to identity by the time mode 1 reachesit, and that the attenuator in mode 1 is back to fulltransmission by the time mode 2 reaches it. Back at thePBS, the modes are swapped in V again, and mode 2 hasits polarizations flipped, to produce

    1

    3

    (α1 |H1〉+ β1

    [−√

    2 |V2〉+ |V1〉])

    (S19)(α2 |H2〉+ β2

    [|V2〉+

    √2 |V1〉

    ]). (S20)

    This is expanded to(α1α2 |H1H2〉+ α1β2 |H1V2〉+ α2β1 |H2V1〉 (S21)

    + β1β2

    [|V1V2〉 − 2 |V1V2〉+

    √2(|V1V1〉 − |V2V2〉)

    ]+√

    2 [α1β2 |H1V1〉 − α2β1 |H2V2〉]).

    Post selecting on one photon in mode 1 and one in mode2 gives

    1

    3(α1α2 |H1H2〉+ α1β2 |H1V2〉

    +α2β1 |H2V2〉 − β1β2 |V1V2〉) , (S22)which is the CPHASE gate.

    S4. EXPONENTIAL INCREASE INPROBABILITIES

    A. Scaling improvement, probability

    Now we calculate the improvement in success probabil-ity of generating a 2N -photon entangled state. To focuson the production rate, let us neglect higher-order photoncontributions and all losses (except storage loop losses,below). If one photon pair is produced with probability p,the probability for N sources to fire simultaneously, or Nsubsequent pairs to be produced in the time-multiplexedcase without feed-forward is pN . With the QIB, the scal-ing is improved as follows. Given a pair is produced in thezeroth time bin with probability p, then the probabilitythat a pair is produced in the time bin j + 1 with nonebefore is (1 − p)jp. The first pair is different from theothers because we must always wait until it is detected,rather than restart the protocol after some waiting timeM . Thus to find the probability of getting two pairs wesum over j as

    P2 = p

    M∑j=0

    (1− p)jp = p(1− (1− p)M+1

    )≈ p2(M + 1).

    (S23)

    Now to produce N pairs, allowing n chances for each pairthe probability is

    PN = p

    M∑j=0

    p(1− p)jN−1 ≈ p [p(M + 1)]N−1 (S24)

    for small p. Thus for n + 1 = 1/p, the exponentiallysmall probability of producing N pairs in enhanced by an(M + 1)N−1 factor.

    With losses in the delay line, we no longer have thesame factor of enhancement but we have a much morefavourable base [7] instead of p in pN . Each photon seesthe roundtrip loop loss j + 2 times, once for couplingin, once for interference, and j times while waiting forthe next pair. Here we assumed that the waiting is resetas soon as the next pair is detected; we do not wait Msteps every time. The last photon only sees two roundtriplosses since it is coupled out directly after interference.Given a roundtrip loss η, the probability of entangling Nphoton pairs is

    PN = pη2

    η2 M∑j=0

    p(1− p)jηjN−1 (S25)

    = pNη2N(

    1− (1− p)M+1ηM+1

    1− (1− p)η

    )N−1≈ pNη2N

    (1− ηM+1 + p(M + 1)ηM+1

    1− (1− p)η

    )N−1.

    In the large M limit we find

    PN = pNη2N

    (1

    1− (1− p)η

    )N−1. (S26)

    For a broad range of losses below a certain threshold,this scaling is better than the scaling without a QIB. Wesimply set

    pN < pNη2N(

    1

    1− (1− p)η

    )N−1(S27)

    to find, for large enough N that N−1N ≈ 1 and in the smallp limit,

    η >p− 1 +

    √p2 − 2p+ 52

    ≈ 0.62, (S28)

    which is easily met in our setup. Comparing to a time-multiplexing setup without buffering or feed-forward,which suffers the same η2 losses per photon, the advantageis for

    pNη2N < pNη2N(

    1

    1− (1− p)η

    )N−1, (S29)

    → η > 0.

    The QIB thus enhances the probabilities of producing a2N -photon entangled state.

    B. Rate improvement

    The above comparison of probabilities shows a distinctimprovement in generation probability using source mul-tipexing with the QIB, but unlike the spatial case this

  • 7

    0.6 0.810 3

    10 2

    10 1

    N = 1

    0.6 0.810 3

    10 2

    10 1

    N = 2

    Exp.

    rang

    e

    1

    10

    0.6 0.810 3

    10 2

    10 1

    N = 3

    1 10

    100

    0.6 0.810 3

    10 2

    10 1

    N = 4

    1

    10

    100

    1000

    0

    0.6 0.810 3

    10 2

    10 1

    N = 5

    1

    1010

    0

    1000

    0 1000

    000

    0.6 0.810 3

    10 2

    10 1

    N = 6

    110

    100

    1000

    010

    0000

    0

    0.0 0.2 0.4 0.6 0.8 1.0Loop efficiency

    0.0

    0.2

    0.4

    0.6

    0.8

    1.0

    Pair

    prod

    uctio

    n pr

    ob. p

    3 × 10 1

    4 × 10 1

    6 × 10 1

    10 1

    100

    101

    10 1100101102103

    100

    102

    104

    10 1

    101

    103105

    107

    10 1101103105107109

    FIG. S5. Advantage of multiplexing for multi-photon generation. For N = 1− 6 photon pairs producing 2N entangledphotons, we present the multiplicative increase to the production probability possible by source multiplexing. For 2N = 12photons a factor of one million is easily achievable. In each case loop efficiencies above 65 % are already sufficient for anadvantage. Our experimental parameter range is marked with red ‘x’ on the N = 2 plot. For our loop efficiency, the optimalmaximum number of roundtrips ranges from 10 to 60. All other losses and the post-selection probability (e.g. for GHZ states

    2−(N−1)) are assumed equivalent between setups.

    procedure takes more than a single laser pulse. Thus wenow examine the time taken by the QIB to generate Nphoton pairs, and show it still provides an overall rateadvantage over spatial- and temporal-schemes withoutmultiplexing.

    With the source clock frequency f , in the spatial casethe waiting time is just one pulse, so the rate per secondis R = fpN . In the time-multiplexed case without feed-forward the average waiting time in number of pulsesis

    tTM =

    ∑Nq=1 p

    q−1q (1− p) + pNN∑Nq=1 p

    q−1 (1− p) + pN. (S30)

    Then the rate per second is RTM = fpN/tTM . With small

    p, most attempts end immediately in failure, makingtTM ≈ 1, and thus making the rate very close to thespatially-multiplexed version.

    In the QIB case the average waiting time is (see belowfor a definition of P1)

    tQIB =1

    p+ (S31)∑N−1

    q=1 Pq−11 ((q − 1)〈M〉+M) (1− P1) + P

    N−11 (N − 1)〈M〉∑N−1

    q=1 Pq−11 (1− P1) + P

    N−11

    .

    The first term is the average waiting time for the firstpair, which is independent of any losses or the maximum

    roundtrip number M . For the subsequent pairs, theaverage wait time per pair 〈M〉 is related to the maximumwait time per pair M by

    〈M〉 =∑M−1j=0 (j + 1)(1− p)jp∑M−1

    j=0 (1− p)jp. (S32)

    This means, for the cases where we get a photon pair atall, we get it on average after 〈M〉 steps. Where we getno photon, we wait M steps then restart the protocol.

    This tQIB is the longest waiting time, (still ≈ 1 for rea-sonable parameters), but the probability PN of producingN pairs is much improved as seen above. The probabilityof getting a single pair in M time bins is

    P1 =

    M−1∑j=0

    (1− p)jp = 1− (1− p)M . (S33)

    In contrast to the previous section, here we account for thefirst photon in the waiting time, such that PN = P

    N−11

    rather than PN = pPN−11 . The rate with the QIB is then

    RQIB = fPN/tQIB . (S34)

    Adding losses in the delay line as in the above section,we find the rate for the standard time-multiplexed case

    is R = f(pη2)N

    /tTM . For the QIB, the probability of

  • 8

    2 4 6 8 10 12Number of photons 2N

    10 2

    100

    102

    104

    1062N

    -pho

    ton

    dete

    ctio

    ns /s

    Spatial GHZ source

    QIB multiplexing

    FIG. S6. Expected GHZ state rates. With increasing sizeof the produced GHZ state, the advantage from using a QIBover parallel sources increases significantly. For a 12-photonGHZ state, the QIB can deliver up to 100 detected states persecond, a six orders of magnitude increase over current stateof the art.

    generating N pairs is

    PN = pN−1η2N

    (1− (1− p)M+1ηM+1

    1− (1− p)η

    )N−1, (S35)

    which is again modified from Eq. (S25) to put the firstphoton pair into the waiting time.

    The P1 and waiting time are however unmodified, theydepend only on the (assumed lossless) heralding signal,not the (un-measurable) loss of photons within the loop.Then the generation rate with losses included is still givenby Eq. (S34), but with PN updated to the lossy version.

    For which losses does time-multiplexing and feed-forward provide an advantage over spatial multiplexing?In general this depends on the number of desired pairs N ,the pair production probability p, and the chosen max-imum waiting time M . In fact the waiting time can beoptimised for each parameter set, and we show in Fig. S5the advantage of using multiplexing with optimised Mover non-multiplexed cases. We show the multiplicativeincrease in rate for various pumping strengths and loopefficiencies. Of course multiplexing is more effective forless lossy loops, but the advantage depends only weaklyon pump power.

    C. Expected absolute rates

    We have demonstrated almost an order of magnitude in-crease in the generation rates for four-photon GHZ states.The true power of the QIB, however, becomes apparentwhen going to larger states; something we couldn’t doin the current experiment due to technical limitations.

    In Fig. S6, we calculate the expected detection rates forlarge GHZ states for both the standard approach of par-allel sources, and the QIB. The current state of the artis the generation of 12-photon GHZ states [6]. Usingthe efficiency values from this publication, we find a sixorders of magnitude increase in the detection rate of 12-photon GHZ states when using the QIB, totalling about100 detected states per second.

    D. Entanglement visibility

    Instead of improving the rate for a constant p, it isalso possible to improve the entanglement visibility byreducing p, while keeping the 2N -photon rate constant.We neglect the waiting time here to keep the formulasreadable, but it would be only a small correction loweringthe visibility of the feed-forward source. For equal ratesof multi-photon production (in the large M limit for theQIB), we set

    pNS = pNTMη

    2N = pNQIBη2N

    (1

    1− (1− p)η

    )N−1, (S36)

    for pair production probabilities for spatial multiplexingpS , time multiplexing pTM and for the QIB pQIB .

    Thus the time-multiplexed single pair generation prob-ability must be scaled up to pTM = pS/η

    2, decreasing theentanglement visibility due to multi-pair emissions. How-ever, the feed-forward fusion pair generation probabilitydecreases to

    pQIB =pSη2

    (1− (1− p)η)N−1N (S37)

    ≈ pSη2

    (1− (1− p)η)

    for large N , which is smaller than pS again for η > 0.62.As an example a visibility increase from ∼25 % to ∼75 %is possible with the QIB and 2N = 10 entangled photonsfor the same 10-fold production rate.

    S5. DETAILS OF SIMULATIONS

    In Fig. 2, simulations are performed with QuTiP [37,38]. For the average fidelity we assume single qubits enterthe loop and are subject to loss, a small rotation dueto an imperfect quarter-wave plate (off by 0.27◦). Thenthe process fidelity is directly found from the average

    fidelity as Fproc =3Favg−1

    2 [39–42]. For the entangledpairs simulation we additionally take into account the fullstatistics of the down-conversion source, the roundtrip lossof the QIB, and also the imperfect extinction ratio of thePockels cell, allowing uncorrelated photons to be coupledinto the QIB during storage of the desired photon. Thiscauses the entanglement fidelity to decrease faster than theunentangled qubit case. Finally, for the HOM visibilitywe include accidental coincidences and the asymmetric

  • 9

    losses due to one photon of the two being stored in theQIB.

    S6. EXPERIMENTAL DETAILS:ELECTRONICS, TIMING, EOM, LOSS BUDGET

    Electronics — The herald (Alice) detection events aresent to a comparator (PRL-350TTL, Pulse Research Lab),which produces a rising and falling edge on separate out-puts for each detection. The falling edges are sent directlyto the timetagger (Time Tagger 20, Swabian Instruments).The rising edges are sent to an FPGA (Spartan6 Evalu-ation Board, Xilinx) which decides the EOM switchingsequence based on the heralding events. For example forthe four-photon GHZ state production wth 11 multiplexedsources, if the FPGA gets two herald clicks 6 roundtripsapart, it will cause the EOM to turn on after the firstphoton enters the loop, remain on for 6 roundtrips, thenturn off at the appropriate moment to enact a PBS oper-ation between the two photons. The FPGA gets its clockfrom a frequency-doubled (by a Si5344, Silicon Labs) ver-sion of the photodiode output of the pump Ti:Sapphirelaser which is repetition-rate stabilized to a master clock.The signals to turn on and off the EOM are again sentto a comparator, one output of which are connected tothe timetagger to provide gating of the photon detectiontimetags. The other outputs from the comparator drivethe EOM. Finally the photon detections after the QIBare also sent to the timetagger, and fourfold coincidencesare found between the two herald and two QIB photons,gated by the FPGA switching signals.

    Electro-optic modulator — The high-voltage driver forthe EOM is from Bergmann Meßgeräte Entwicklung KG,and the RTP Pockels cell is from Leysop Ltd. The driverhas a rise and fall time aroud 5 ns, sufficiently less than thehalf-roundtrip time of the QIB of 6.6 ns to allow switchingbetween all three modes. The maximum duty cycle ofthe cell is around 5 %, and the maximum switching rateis 100 kHz, which limits our maximum count rates here.Drivers with faster rates of around 2 MHz are available,and it should be possible to reach 5 ns rise times with thesetoo, increasing our maximum rate 20 fold. Of course as wescale to larger N , the probability of N -fold coincidencesdecreases, meaning the maximum switching rate is nolonger a limiting factor. The extinction ratio of the EOMis around 100 : 1.Timing considerations — The experiment runs off a

    common clock from the pump Ti:Sapphire laser, meaningoptical and electronic timings are stable relative to one

    another. To allow sufficient time for the heralding signalsto reach the FPGA, be processed, and set the EOM, theQIB photons are stored for 1.7 µs in single-mode fiber.This was chosen to allow very long storage times; forthe GHZ states with 11 multiplexed sources, only 600 nsis required. Having both herald detections available tothe FPGA before any photons arrive at the QIB is keyto reducing the switching load: the QIB stores the firstphoton only when it is already known that the secondhas been heralded.

    We set the maximum storage time M for each effectivesource. If the second photon is detected before the maxi-mum storage time, they are interfered directly, and thesource is made ready for the next heralding event, as inthe idea of relative multiplexing [43]. The average firstphoton will thus be stored under half of the maximumtime, and the maximum average repetition rate of thesource will be the inverse of half the maximum storagetime. For now the repetition period is limited by themaximum switching speed of the EOM.

    Loss budget — The roundtrip loss of the QIB is ac-counted for with the following efficiencies: PBS (98.7 %)2;EOM 98 %; 9 dielectric mirrors (Laseroptik GmbH)(99.6 %)9; self-coated spherical end mirror 99.3 %. Thesegive a total roundtrip transmission of 91.7 %, which agreeswith that extracted from the fits in Figs. 2 and 3. Theroundtrip efficiency of (90.57± 0.06) % from Fig. 2 isslightly lower than expected since for long storage timesthe mode is no longer perfectly refocused by our curvedend mirrors. For only up to 5 roundtrips, where thelargest contribution to the four-photon GHZ state ratecomes from, we extract a roundtrip efficiency from Fig. 3of (93.7± 0.7) %.

    S7. ADDITIONAL EXPERIMENTAL DATA

    We present raw HOM dip count data in Fig. S7.

    We evaluate the fidelity of our GHZ states follow-ing [44], and show the fidelity, population, and coherencein Fig. S8a. The fidelity is the average of the populationand coherence, F = (P + C)/2. The population is eval-uated from Fig. S8b as the counts in the first and lastbins divided by the total counts. The coherence is evalu-ated from four such datasets (example in Fig. S8c) in the

    measurement basis (|H〉 ± eiθ |V 〉)/√

    2, where θk = kπ/4

    for k = [0, 1, 2, 3]. Then C = 14∑3k=0(−1)k 〈Mk〉 for the

    expectation value of Mk = cos (kπ/4)σx + sin (kπ/4)σy.

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  • 10

    0 2 4 6Time (ps)

    0

    200

    400FWHM = 1238fst = 13nsV = (81.2 ±1.6)%

    b

    0.0 0.1 0.2Time (ps)

    0

    50

    Four

    fold

    s per

    seco

    nd

    FWHM = 36fst = 408nsV = (53.6 ±1.7)%

    c

    0.00 0.05 0.10Time (ps)

    0

    20 FWHM = 30fst = 671nsV = (24.1 ±2.7)%

    d

    0 1 2 3 4Time (ps)

    0.0

    0.2

    0.4

    0.6

    0.8

    1.0

    Four

    fold

    s per

    seco

    nd

    FWHM = 1231fst = 13 nsV = (94.5 ±1.8)%

    a

    FIG. S7. Further data for Hong-Ou-Mandel interference. Each plot lists the full-width half-maximum of the HOM dip, thestorage time of the first photon t and the dip visibility, V = (max−min)/max. a, Best measured visibility at low pump power,showing the indistinguishability of the photon pair source. b-d, Example HOM dips at higher power for faster data collection,showing degradation as storage time is increased from 13 ns to 671 ns. The FWHM of the dip also decreases proportionally tothe storage time, as the mirror that is scanned to measure the dip is the end mirror of the QIB, meaning the translation iseffectively multiplied by the number of storage roundtrips.

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  • 11

    5 10 15 20Number of sources

    0.5

    0.6

    0.7

    0.8

    0.9

    1.0a

    PopulationFidelityCoherence

    Detector combination0

    200

    400

    600

    800

    1000

    1200

    Four

    fold

    s (40

    s) HHHH

    HHHV

    HHVH . . .

    VVVH

    VVVV

    Population

    b

    Detector combination0

    20

    40

    60

    80

    Four

    fold

    s (40

    s)

    HHHH

    VVVV

    Coherence ( 3 term)c

    0 /4 /2 3 /4k

    1.000.750.500.250.000.250.500.751.00

    Mk

    d

    FIG. S8. Further data for four-photon GHZ states. a, The fidelity as in Fig. 3, made up of the population and coherence terms.The coherence is lower than the population due to imperfect HOM interference and a small phase in the loop. b, Raw fourfoldcount data for the first data point of the population (two sources). c, Raw fourfold count data for the first data point of the

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    Exponential enhancement of multi-photon entanglement rate via quantum interference buffering MethodsS1 Action of QIBA Comparison to quantum memories

    S2 Generation of GHZ statesS3 Generation of linear cluster statesA Cluster state generation with additional EOMB Replacement of EOM with a static wave plateC CPHASE gate with QIB

    S4 Exponential increase in probabilitiesA Scaling improvement, probabilityB Rate improvementC Expected absolute ratesD Entanglement visibility

    S5 Details of simulationsS6 Experimental details: electronics, timing, EOM, loss budgetS7 Additional experimental data References