Tag: Quantum simulation

  • Combining quantum processors with real-time classical communication

    Combining quantum processors with real-time classical communication

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    Circuit cutting

    The gates in a quantum circuit are quantum channels acting on density matrices ρ. A single quantum channel \({\mathcal{E}}(\rho )\) is cut by expressing it as a sum over I quantum channels \({{\mathcal{E}}}_{i}(\rho )\) resulting in the QPD

    $${\mathcal{E}}(\rho )=\mathop{\sum }\limits_{i=0}^{I-1}{a}_{i}{{\mathcal{E}}}_{i}(\rho ).$$

    (1)

    The channels \({{\mathcal{E}}}_{i}(\rho )\) are easier to implement than \({\mathcal{E}}(\rho )\) and are built from LO16 or LOCC17 (Fig. 1). As some of the coefficients ai are negative, we introduce γ = ∑iai and Pi = ai/γ to recover a valid probability distribution with probabilities Pi over the channels \({{\mathcal{E}}}_{i}\). Here, γ can be seen as the amount by which the QPD deviates from a true probability distribution and is thus a cost to pay to implement the QPD. Without a QPD an observable is estimated by \(\langle O\rangle ={\rm{Tr}}\,\{O{\mathcal{E}}(\rho )\}\). However, when using this QPD, we build an unbiased Monte Carlo estimator of O as

    $${\langle O\rangle }_{{\rm{QPD}}}=\gamma \mathop{\sum }\limits_{i=0}^{I-1}{P}_{i}{\rm{sign}}({a}_{i})\,\text{Tr}\,\{O{{\mathcal{E}}}_{i}(\rho )\}.$$

    (2)

    The variance of the QPD estimator OQPD is a factor of γ2 larger than the variance of the non-cut estimator O (ref. 44). When cutting n > 1 identical channels, we can build an estimator by taking the product of the QPDs for each individual channel, resulting in a γ2n rescaling factor22,45. This exponential increase in variance is compensated by a corresponding increase in the number of measured shots. Therefore, γ2n is called the sampling overhead and indicates that circuit cutting must be used sparingly. Details of the LO and LOCC quantum channels \({{\mathcal{E}}}_{i}\) and their coefficients ai are provided in sections ‘Virtual gates implemented with LO’ and ‘Virtual gates implemented with LOCC’, respectively.

    Virtual gates implemented with LO

    Here, we discuss how to implement virtual CZ gates with LO16,18. We follow ref. 16 and, therefore, decompose each cut CZ gate into local operations and a sum over six different circuits defined by

    $$\begin{array}{l}2{\rm{CZ}}\,=\sum _{\alpha \in \{\pm 1\}}{R}_{z}\left(\alpha \frac{\pi }{2}\right)\otimes {R}_{z}\left(\alpha \frac{\pi }{2}\right)\\ \,\,\,-\sum _{{\alpha }_{1},{\alpha }_{2}\in \{\pm 1\}}{\alpha }_{1}{\alpha }_{2}{R}_{z}\left(-\frac{{\alpha }_{1}+1}{2}\pi \right)\otimes \left(\frac{I+{\alpha }_{2}Z}{2}\right)\\ \,\,\,-\sum _{{\alpha }_{1},{\alpha }_{2}\in \{\pm 1\}}{\alpha }_{1}{\alpha }_{2}\left(\frac{I+{\alpha }_{1}Z}{2}\right)\otimes {R}_{z}\left(-\frac{{\alpha }_{2}+1}{2}\pi \right),\end{array}$$

    (3)

    where \({R}_{z}(\theta )=\exp \left(-{\rm{i}}\frac{\theta }{2}Z\right)\) are virtual Z rotations46. The factor 2 in front of CZ is for readability. Each of the possible six circuits is thus weighted by a 1/6 probability (Extended Data Fig. 1). The operations (I + Z)/2 and (I − Z)/2 correspond to the projectors |0 0| and |1 1|, respectively. They are implemented by MCMs and classical post-processing. More specifically, when computing the expectation value of an observable O = ∑iaiOi with the LO QPD, we multiply the expectation values Oi by 1 and −1 when the outcome of an MCM is 0 and 1, respectively.

    In the experiments that implement graph states with LO in the main text, we implement the CZ gate with six circuits built from Rz gates and MCMs16. Cutting four CZ gates with LO thus requires I = 64 = 1,296 circuits. However, as the node and edge stabilizers of the graph states are at most in the light cone47 of one virtual gate, we instead implement two QPDs in parallel, which requires I = 62 = 36 LO circuits per expectation value. In general, sampling from a QPD results in an overhead of \({({\sum }_{i=0}^{I-1}| {a}_{i}| )}^{2}\), where I is the number of circuits in the QPD and the ai are the QPD coefficients44. However, as the LO QPDs in our experiments have only 36 circuits, we fully enumerate the QPDs by executing all 36 circuits. The sampling cost of full enumeration is \(I({\sum }_{i=0}^{I-1}| {a}_{i}{| }^{2})\). Furthermore, as ai = 1/2 i = 0, …, I − 1, sampling from the QPD and fully enumerating it both have the same shot overhead.

    The decomposition in equation (3) with γ2 = 9 is optimal with respect to the sampling overhead for a single gate17. Recently, refs. 30,31 found a new protocol that achieves the same γ overhead as LOCC when cutting multiple gates in parallel. The proofs in refs. 30,31 are theoretical demonstrating the existence of a decomposition.

    Virtual gates implemented with LOCC

    We now discuss the implementation of the dynamic circuits that enable the virtual gates with LOCC. We first present an error suppression and mitigation of dynamic circuits with dynamical decoupling (DD) and zero-noise extrapolation (ZNE). Second, we discuss the methodology to create the cut Bell pairs and present the circuits to implement one, two and three cut Bell pairs. Finally, we propose a simple benchmark experiment to assess the quality of a virtual gate.

    Error-mitigated quantum circuit switch instructions

    All quantum circuits presented in this work are written in Qiskit. The feed-forward operations of the LOCC circuits are executed with a quantum circuit switch instruction, hereafter referred to as a switch. A switch defines a set of cases in which the quantum circuit can branch depending on the outcome of a corresponding set of measurements. This branching occurs in real time for each experimental shot, with the measurement outcomes being collected by a central processor, which in turn broadcasts the selected case (here corresponding to a combination of X and Z gates) to all control instruments.

    As quantum computing scales, the control electronics become tailored to its QPU and are no longer built from off-the-shelf components. Recent IBM devices have a single QPU with a rack of dedicated and tailored control electronics, as shown in refs. 29,48. The realization of the feed-forward we present builds upon the work in ref. 29 and advances its scalability in two main ways. First, our development enables the synchronization and inter-communication between separate experimental setups. Not only are the control instruments for the two sub-QPUs located in different racks, but they are also configurable in software to operate on them independently for the LO experiments and recombined for LOCC. This architecture is extensible to multiple racks and QPUs. It overcomes several of the challenges in operating a distributed control system as pointed out in ref. 23. Second, the duration of the conditional operation is independent of the measurement results, of which qubits are measured, and which qubits are subject to the conditional operations (apart from minor differences due to cable lengths). This enables the scheduling and execution of programs equally across the combined QPU as if it were a single one.

    The feed-forward process results in a latency of the order of 0.5 μs (independent of the selected case) during which no gates can be applied (Extended Data Fig. 2a, red area). Free evolution during this period (τ), often dominated by static ZZ cross-talk in the Hamiltonian, typically with a strength ranging from about 103 Hz to 104 Hz, substantially deteriorates results. To cancel this unwanted interaction and any other constant or slowly fluctuating IZ or ZI terms, we precede the conditional gates with a staggered DD XX sequence, adding 3τ to the switch duration (Extended Data Fig. 2a). The value of τ is determined by the longest latency path from one QPU to the other and is fine-tuned by maximizing the signal on such a DD sequence. Furthermore, we mitigate the effect of the overall delay on the observables of interest with ZNE22. To do this, we first stretch the switch duration by a factor c = (τ + δ)/τ, where δ is a variable delay added before each X gate in the DD sequence (Extended Data Fig. 2a). Second, we extrapolate the stabilizer values to the zero-delay limit c = 0 with a linear fit. In many cases, an exponential fit can be justified1; however, we observe in our benchmark experiments that a linear fit is appropriate (Extended Data Fig. 2). Without DD, we observe strong oscillations in the measured stabilizers that prevent an accurate ZNE (see the XZ stabilizer in Extended Data Fig. 2c). As seen in the main text, this error suppression and mitigation reduce the error on the stabilizers affected by virtual gates.

    The error suppression and mitigation that we implement for the switch also apply to other control flow statements. The switch is not the only instruction capable of representing control flow. For instance, OpenQASM349 supports if/else statements. Our scheme is done by (1) adding DD sequences to the latency (possibly by adding delays if the control electronics cannot emit pulses during the latency); (2) stretching the delay; and (3) extrapolating to the zero-delay limit.

    Cut Bell pair factories

    Here, we discuss the quantum circuits to prepare the cut Bell pairs needed to realize virtual gates with LOCC. To create a factory for k cut Bell pairs, we must find a linear combination of circuits with two disjoint partitions with k qubits each to reproduce the statistics of Bell pairs. We create the state ρk of the Bell pairs following ref. 50 such that \({\rho }_{k}=(1+{t}_{k}){\rho }_{k}^{+}-{t}_{k}{\rho }_{k}^{-}\), where tk = 2k − 1. Here, \({\rho }_{k}^{\pm }\) are mixed states separable with respect to the partitions A and B. Note that ρk entangles the qubit partitions A and B, shown in Fig. 1c, but \({\rho }_{k}^{\pm }\) do not. The total cost of this QPD with two states is determined by γk = 2tk + 1. Next, we realize \({\rho }_{k}^{\pm }\) from a probabilistic mixture of pure states \({\rho }_{k,i}^{\pm }\), that is, valid probability distributions. The state \({\rho }_{k}^{-}\) is easily implemented by a uniform mixture of all basis states that correspond to a 0 entry on the diagonal of the density matrix ρk. The basis states themselves do not appear in ρk. We thus implement \({\rho }_{k}^{-}\) as a diagonal density matrix of \({n}_{k}^{-}={4}^{k}-{2}^{k}\) basis states. The state \({\rho }_{k}^{+}\) is harder to engineer. It requires a probabilistic mixture of intricate states with entanglement within each partition A and B but not between them. To engineer \({\rho }_{k}^{+}\), we thus build a parametric quantum circuit Ck(θi) with parameters θi in which no two-qubit gate connects qubits between A and B. Following ref. 50, we need \({n}_{k}^{+}={2}^{{2}^{k}}-1\) pure states to realize \({\rho }_{k}^{+}\). The exact form of \({\rho }_{k}^{+}\), omitted here for brevity, is given in Appendix B of ref. 50. Therefore, the total number of parameter sets \(I={n}_{k}^{+}+{n}_{k}^{-}\) required to implement one, two and three cut Bell pairs is 5, 27 and 311, respectively. Finally, the coefficients ai,k of all the circuits in the QPD in equation (1) that implement \({\rho }_{k}^{\pm }\) are

    $${a}_{i,k}=\frac{1+{t}_{k}}{{n}_{k}^{+}},\,\,{\rm{for}}\,\,i\in \{0,…,{n}_{k}^{+}-1\},\,{\rm{and}}$$

    (4)

    $${a}_{i,k}=-\frac{{t}_{k}}{{n}_{k}^{-}},\,\,{\rm{for}}\,\,i\in \{{n}_{k}^{+},…,{n}_{k}^{+}+{n}_{k}^{-}-1\}.$$

    (5)

    For k = 2, the resulting weights, ai,k/γk are approximately all equal. There is thus no practical difference between sampling and enumerating the k = 2 QPD when executing it on hardware. More precisely, for the factories with two cut Bell pairs that we run on hardware, the cost of sampling the QPD is \({({\sum }_{i=0}^{I-1}| {a}_{i,2}| )}^{2}={\gamma }_{2}^{2}(1+1.6\times 1{0}^{-7})\) and the cost of fully enumerating the QPD is \(I({\sum }_{i=0}^{I-1}| {a}_{i,2}{| }^{2})={\gamma }_{2}^{2}(1+1.0\times 1{0}^{-3})\), where γ2 = 7.

    We construct all pure states \({\rho }_{k,i}^{\pm }\) from the same template variational quantum circuit Ck(θi) with parameters θi, where the index i = 0, …, I − 1 runs over the I elements of the probabilistic mixtures defining \({\rho }_{k}^{\pm }\). The parameters θi in the template circuits Ck(θi) are optimized by the SLSQP classical optimizer51 by minimizing the L2-norm with respect to the I pure target states needed to represent \({\rho }_{k}^{+}\), where the norm is evaluated with a classical state vector simulation. After testing various approaches, we find that those provided in Fig. 1c and Extended Data Fig. 3 enable us to achieve an error, based on the L2 norm, of less than 10−8 for each state while having minimal hardware requirements. To enable rapid execution of the QPD with parametric updates, all the parameters are the angles of virtual Z rotations46 (Fig. 1c). As \({\rho }_{k}^{-}\) is built from basis states, we analytically derive the parameters. Therefore, we could also significantly simplify the ansatz Ck(θi), for example, by cancelling CNOT gates. However, we keep the same template for compilation and execution efficiency. On first inspection, the parameters entering \({\rho }_{k}^{+}\) do not have any usable structure. We thus leave it up to future research to further investigate whether these parameters have any structure that could be leveraged to simplify the cut Bell pair factories.

    A single-cut Bell pair is engineered by applying the gates U(θ0, θ1) and U(θ2, θ3) on qubits 0 and 1. Here, and in the figures, the gate U(θ, ϕ) corresponds to \(\sqrt{X}{R}_{z}(\theta )\sqrt{X}{R}_{z}(\phi )\). The QPD of a single-cut Bell pair requires five sets of parameters given by {[π/2, 0, π/2, 0], [π/2, −2π/3, π/2, 2π/3], [π/2, 2π/3, π/2, −2π/3], [π, 0, 0, 0], [0, 0, π, 0]} which could also be derived analytically. The circuits to simultaneously create two and three cut Bell pairs are shown in Fig. 1c and Extended Data Fig. 3, respectively. The circuits and the values of the parameters as obtained by the optimizer are available on GitHub (www.github.com/eggerdj/cut_graph_state_data).

    In the experiments that implement graph states with LOCC in the main text, we construct two QPDs in parallel with I = 27 circuits, each QPD implementing two long-range CZ gates. This execution is similar to the LO execution in which we also execute two QPDs in parallel.

    Benchmarking qubits for LOCC

    The quality of a CNOT gate implemented with dynamic circuits depends on hardware properties. For example, qubit relaxation, dephasing and static ZZ cross-talk all negatively affect the qubits during the idle time of the switch. Furthermore, measurement quality also affects virtual gates implemented with LOCC. Errors on MCMs are harder to correct than errors on final measurements as they propagate to the rest of the circuit through the conditional gates52. For instance, assignment errors during readout result in an incorrect application of a single-qubit X or Z gate. Given the variability in these qubit properties, care must be taken in selecting those to act as cut Bell pairs. To determine which qubits will perform well as cut Bell pairs, we develop a fast characterization experiment on four qubits that does not require a QPD or error mitigation. This experiment creates a graph state between qubits 0 and 3 by consuming an uncut Bell pair created on qubits 1 and 2 with a Hadamard and a CNOT gate. We measure the stabilizers ZX and XZ which require two different measurement bases. The resulting circuit, shown in Extended Data Fig. 4a, is structurally equivalent to half of the circuit that consumes two cut Bell pairs, for example, Fig. 1c. We execute this experiment on all qubit chains of length four on the devices that we use and report the mean squared error (MSE), that is, [(ZX − 1)2 + (XZ − 1)2]/2 as a quality metric. The lower the MSE is the better the set of qubits act as cut Bell pairs. With this experiment we benchmark, ibm_kyiv (the device used to create the graph state with 103 nodes), and ibm_pinguino-1a and ibm_pinguino-1b (the two Eagle QPUs combined into a single device, named ibm_pinguino-2a, used to create the graph state with 134 nodes). We observe more than an order of magnitude variation in MSE across each device (Extended Data Fig. 4b).

    The qubits we chose to act as cut Bell pairs are a tradeoff between the graph we want to engineer and the quality of the MSE benchmark. For example, the graphs with periodic boundary conditions presented in the main text were designed first based on the desired shape of |G and second based on the MSE of the Bell pair quality test.

    Graph states

    A graph state |G is created from a graph G = (V, E) with nodes V and edges E by applying an initial Hadamard gate to each qubit, corresponding to a node in V, and then CZ gates to each pair of qubits (i, j) E (refs. 53,54). The resulting state |G has V first-order stabilizers, one for each node iV, defined by Si = XikN(i)Zk. Here, N(i) is the neighbourhood of node i defined by E. These stabilizers satisfy Si|G = |G. By construction, any product of stabilizers is also a stabilizer. If an edge (i, j) E is not implemented by a CZ gate, the corresponding stabilizers drop to zero, that is, Si = Sj = 0. This effect can be seen in the dropped edge benchmark, see, for example, Fig. 2b.

    Entanglement witness

    We now define a success criterion for the implementation of a graph state with entanglement witnesses55. A witness \({\mathcal{W}}\) is designed to detect a certain form of entanglement. As we cut edges in the graph state, we focus on witnesses \({{\mathcal{W}}}_{i,j}\) over two nodes i and j connected by an edge in E. An edge (i, j) of our graph state |G presents entanglement if the expectation value \(\langle {{\mathcal{W}}}_{i,j}\rangle < 0\). The witness does not detect entanglement if \(\langle {{\mathcal{W}}}_{i,j}\rangle \ge 0\). The first-order stabilizers of nodes i and j with (i, j) E are

    $${S}_{i}={Z}_{j}{X}_{i}\prod _{k\in N(i)\backslash j}{Z}_{k}\,\text{and}\,{S}_{j}={X}_{j}{Z}_{i}\prod _{k\in N(j)\backslash i}{Z}_{k}.$$

    (6)

    Here, N(i) is the neighbourhood of node i, which includes j because (i, j) E. Thus, N(i)\j is the neighbourhood of node i excluding j. Following refs. 55,56, we build an entanglement witness for edge (i, j) E as

    $${{\mathcal{W}}}_{i,j}=\frac{1}{4}{\mathbb{I}}-\frac{1}{4}(\langle {S}_{i}\rangle +\langle {S}_{j}\rangle +\langle {S}_{i}{S}_{j}\rangle ).$$

    (7)

    This witness is zero or positive if the states are separable. Alternatively, as in ref. 27, a witness for bi-separability is also given by

    $${{\mathcal{W}}}_{i,j}^{{\prime} }={\mathbb{I}}-\langle {S}_{i}\rangle -\langle {S}_{j}\rangle .$$

    (8)

    Here, we consider both witnesses. The data in the main text are presented for \({{\mathcal{W}}}_{i,j}\). As discussed in ref. 56, \({{\mathcal{W}}}_{i,j}\) is more robust to noise than \({{\mathcal{W}}}_{i,\,j}^{{\prime} }\). However, \({{\mathcal{W}}}_{i,j}\) requires more experimental effort to measure than \({{\mathcal{W}}}_{i,\,j}^{{\prime} }\) because of the stabilizer SiSj.

    For completeness, we now show how a witness can detect entanglement by focusing on \({{\mathcal{W}}}_{i,j}\). A separable state satisfies \(\langle {P}_{1}…{P}_{n}\rangle ={\prod }_{i}\langle {P}_{i}\rangle \), where Pi are single-qubit Pauli operators. Therefore, we can show, using the Cauchy–Schwarz inequality, that \(\langle {S}_{i}\rangle +\langle {S}_{j}\rangle +\langle {S}_{i}{S}_{j}\rangle \le 1\) and that \({{\mathcal{W}}}_{i,j}\ge 0\) for separable states.

    $$\langle {S}_{i}\rangle +\langle {S}_{j}\rangle +\langle {S}_{i}{S}_{j}\rangle =\langle {Z}_{j}\rangle \langle {X}_{i}\rangle \prod _{k\in N(i)\backslash j}\langle {Z}_{k}\rangle $$

    (9)

    $$+\langle {X}_{j}\rangle \langle {Z}_{i}\rangle \prod _{k\in N(j)\backslash i}\langle {Z}_{k}\rangle +\langle {Y}_{i}\rangle \langle {Y}_{j}\rangle \prod _{k\in M(i,j)}\langle {Z}_{k}\rangle $$

    (10)

    $$\le | \langle {Z}_{j}\rangle | | \langle {X}_{i}\rangle | +| \langle {X}_{j}\rangle | | \langle {Z}_{i}\rangle | +| \langle {Y}_{j}\rangle | | \langle {Y}_{i}\rangle | $$

    (11)

    $$\le \sqrt{{\langle {X}_{i}\rangle }^{2}+{\langle {Y}_{i}\rangle }^{2}+{\langle {Z}_{i}\rangle }^{2}}\sqrt{{\langle {X}_{j}\rangle }^{2}+{\langle {Y}_{j}\rangle }^{2}+{\langle {Z}_{j}\rangle }^{2}}$$

    (12)

    The step from equation (10) to equation (11) relies on ∏iai ≤ ∏i ai and that \({\prod }_{k}| \langle {Z}_{k}\rangle | \le 1\), where the product runs over nodes that do not contain i or j. The step from equation (11) to equation (12) is based on the Cauchy–Schwarz inequality. The final step relies on the fact that \({\langle {X}_{i}\rangle }^{2}+{\langle {Y}_{i}\rangle }^{2}+{\langle {Z}_{i}\rangle }^{2}\le 1\) with pure states equal to one. Therefore, the witness \({{\mathcal{W}}}_{i,j}\) will be negative if the state is not separable.

    In the graph states presented in the main text, we execute a statistical test at a 99% confidence level to detect entanglement. As discussed in the Supplementary Information and shown in Fig. 2b, some witnesses may go below −1/2 because of readout error mitigation, the QPD and Switch ZNE. We, therefore, consider an edge to have the statistics of entanglement if the deviation from −1/2 is not statistically greater than ±1/2. Based on a one-tailed test, we consider that edge (i, j) is bi-partite entangled if

    $$-\frac{1}{2}+\left|\langle {{\mathcal{W}}}_{i,j}\rangle +\frac{1}{2}\right|+{z}_{99 \% }{\sigma }_{{\mathcal{W}},i,j} < 0.$$

    (14)

    Similarly, we form a success criterion based on \({{\mathcal{W}}}_{i,j}^{{\prime} }\) as

    $$-1+| \langle {{\mathcal{W}}}_{i,j}^{{\prime} }\rangle +1| +{z}_{99 \% }{\sigma }_{{{\mathcal{W}}}^{{\prime} },i,j} < 0.$$

    (15)

    This criterion penalizes any deviation from −1, that is, the most negative value that \({{\mathcal{W}}}_{i,\,j}^{{\prime} }\) can have. Here, z99% = 2.326 is the z-score of a Gaussian distribution at a 99% confidence level and \({\sigma }_{{\mathcal{W}},i,j}\) is the standard deviation of edge witness \({{\mathcal{W}}}_{i,j}\). These tests are conservative as they penalize any deviation from the ideal values. Moreover, these tests are most suitable for circuit cutting because the QPD may increase the variance \({\sigma }_{{{\mathcal{W}}}_{i,j}}\) of the measured witnesses. Therefore, the statistics of entanglement are detected only if the mean of a witness is sufficiently negative and its standard deviation is sufficiently small. An edge (i, j) E fails the criteria if equation (14) or equation (15) is not satisfied. All edges in E, including the cut edges, pass the test based on \({{\mathcal{W}}}_{i,j}\) when implemented with LO and LOCC (Extended Data Table 2). However, some edges fail the test based on \({{\mathcal{W}}}_{i,\,j}^{{\prime} }\) because of the lower noise robustness of \({{\mathcal{W}}}_{i,\,j}^{{\prime} }\) compared with \({{\mathcal{W}}}_{i,j}\).

    Circuit count for stabilizer measurements

    Obtaining the bipartite entanglement witnesses requires measuring the expectation values of Si, Sj and SiSj of each edge (i, j) E. For the 103- and 134-node graphs presented in the main text, all 219- and 278-node and edge stabilizers, respectively, can be measured in NS = 7 groups of commuting observables. To mitigate final measurement readout errors, we use twirled readout error extinction (TREX) with NTREX samples57. When virtual gates are used with LO and LOCC, we require ILO and ILOCC more circuits, respectively. In this work, we fully enumerate the QPD. Furthermore, for LOCC, we mitigate the delay of the switch instruction with ZNE based on NZNE stretch factors. Therefore, the four types of experiments are executed with the following number of circuits.

    • Swaps: NSNTREX

    • Dropped edge: NSNTREX

    • LO: NSNTREXILO

    • LOCC: NSNTREXILOCCNZNE

    In the experiments for the 103- and 134-node graph states, we use NTREX = 5 and 3 TREX samples, respectively. Therefore, measuring the stabilizers without a QPD requires NS × NTREX = 35 circuits for the 103-node graph. For LO and LOCC, measuring the stabilizers for the graphs in the main text requires 64 and 272 circuits, respectively. However, owing to the graph structure, each edge witness is only ever in the light cone of two cut gates at most. We may thus execute a total of ILO = 62 and ILOCC = 27 circuits for LO and LOCC, respectively, based on the light cone of the gates. For higher-weight observables, this corresponds to sampling the diagonal terms of a joint QPD. Therefore, measuring the stabilizers with LO requires NS × NTREX × ILO = 1,260 circuits. For LOCC, we further perform error mitigation of the switch with NZNE = 5 stretch factors. We, therefore, execute NS × NTREX × ILOCC × NZNE = 4,725 circuits to measure the error-mitigated stabilizers needed to compute \({{\mathcal{W}}}_{i,j}\). Each circuit is executed with a total of 1,024 shots.

    To reconstruct the value of the measured observables, we first merge the shots from the TREX samples. To do this, we flip the classical bits in the measured bit strings corresponding to measurements for which TREX prepended an X gate. These processed bit strings are then aggregated in a count dictionary with 1,024 × NTREX counts. Next, to obtain the value of a stabilizer, we identify which of the NS measurement bases we need to use. The value of a stabilizer and its corresponding standard deviation are then obtained by resampling the corresponding 1,024 × NTREX counts. Here, we randomly select 10% of the shots to compute an expectation value. Ten such expectation values are averaged and reported as the measured stabilizer value. The standard deviation of these 10 measurements is reported as the standard deviation of the stabilizer, shown as error bars in Fig. 2b. Finally, if the stabilizer is in the light cone of a virtual gate implemented with LOCC, we linearly fit the value of the stabilizer obtained at the NZNE = 5 switch stretch factors. This fit, shown in Extended Data Fig. 2d, enables us to report the stabilizer at the extrapolated zero-delay switch.

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  • Observation of Hilbert space fragmentation and fractonic excitations in 2D

    Observation of Hilbert space fragmentation and fractonic excitations in 2D

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    Experimental details

    Here we briefly describe the initial-state preparation common to all measurements. Experiments were performed in a single plane of a vertical one-dimensional optical lattice. For the in-plane lattice, we used the folded lattice described in ref. 39. As the in-plane lattice is subject to disorder and harmonic confinement, we used a digital micromirror device to shape the horizontal on-site potential, allowing us to achieve approximately homogeneous trapping depths and tunnelling energies throughout the system. Using a second digital micromirror device, we additionally projected a tapered, rectangular box in the centre of this corrected system, to achieve reliable loading and high filling in a central area of about 15 × 15 lattice sites.

    Starting from these Mott insulators, to prepare the initial states of interest, we then performed local addressing over the entire area41,42, whereas the data analysis was performed in a smaller region of interest (ROI) of either 8 × 8 or 10 × 10 lattice sites at the centre of the system. In addition, working with larger systems than the size of the ROI minimizes the influence of finite-size and boundary effects. With this preparation sequence, we achieved a filling of 0.88(2) per site on the addressed sites and a filling of 0.04(2) on the non-addressed sites in the ROI. These values were averaged over all datasets and initial configurations.

    Magnetic-field gradient calibration

    The potential tilt in our experiments was realized by global magnetic fields, which allowed us to induce the most homogeneous gradients. We calibrated the magnitude and the orientation of the magnetic gradient using spatially resolved microwave spectroscopy on the magnetic-field-sensitive transition between the \(| F=1,{m}_{F}=-\,1\rangle \) and the \(| F=2,{m}_{F}=-\,2\rangle \) hyperfine ground states.

    To this end, we prepared a large Mott insulator with all atoms in the \(| F=1,{m}_{F}=-\,1| \rangle \) state. We then adiabatically ramped up the magnetic field to its target configuration and performed narrow microwave sweeps at variable centre frequencies. As a consequence, atoms were addressed resonantly within a narrow stripe subjected to the same magnetic-field strength and flipped into the \(| F=2,{m}_{F}=-\,2\rangle \) state, which were then removed before imaging. We fitted a two-dimensional Gaussian to these stripes of missing atoms, which allowed us to map the field strength and gradient orientation versus their position (Extended Data Fig. 1a).

    To be able to continuously vary the applied gradient strength, we used a combination of coils: a single vertical gradient coil and a pair of vertical offset coils in Helmholtz configuration with reversed field polarity to realize a quadrupole field near the plane of the atoms. For the initial calibration, we worked with a fixed gradient coil setpoint and tuned the vertical offset and additional in-plane offset fields such that the magnetic zero point was at the location of the atoms; subsequently, we shifted the zero point by a fixed amount using the in-plane offset fields, resulting in an in-plane gradient at the correct angle. We then proceeded to calibrate the gradient strength for various gradient coil setpoints as described above; for technical reasons, we tuned the gradient coil instead of the offset coils. We interpolated between the calibrated values by fitting them with the function

    $$g(\Delta B)=\frac{{g}_{0}^{2}r}{\sqrt{{g}_{0}^{2}{r}^{2}+{(\Delta B+{B}_{0})}^{2}}},$$

    (3)

    where r is the displacement of the magnetic field zero to the atoms, g0 is the maximal gradient strength, B0 describes background fields and ΔB is the change of the setpoint of the gradient coil. As we changed ΔB by only a few per cent, we can assume g0(B) = constant, which is also supported by the fact that the fit function describes the data well, as shown in Extended Data Fig. 1b.

    On the basis of this curve, we can then rescale the x axis in Extended Data Fig. 2 and obtain an absolute value for the gradient strength.

    Hubbard parameters

    To extract the Hubbard parameters of our folded optical lattice39, we made use of two methods. First, we performed amplitude modulation spectroscopy to calibrate the lattice depth. The results were then compared with a band-structure calculation to obtain the values for the on-site interaction U and the tunnelling energy J. Here we found U/J = 21(2) with U = h × 275(5) Hz and J = h × 13(1) Hz. The error bars arise from the uncertainty of the lattice-depth calibration itself as well as the slightly anisotropic hopping along the two lattice axes39. Second, we can independently calibrate the Hubbard parameters using the quench dynamics of isolated dimers (see Extended Data Fig. 3 and below). As a result, we extracted τ = ħ/J = 10.0(3) ms, equivalent to J = h × 16.0(5) Hz. Comparing again with our band-structure calculation, this corresponds to U/J = 17(1) with U = h × 260(5) Hz. We attribute the deviations between these two calibrations to day-to-day drifts of the lattice beam alignment over the entire data-taking period.

    For data evaluation, we used τ = 11 ms for all datasets, motivated by the long data-taking period of several days for a given dataset. Theory calculations (see below) were performed for U/J = 18, which was chosen as an intermediate value between the two calibrations.

    Tuning the gradient to resonance

    For the presented studies, it is important that the applied gradient matches the on-site interaction, that is, Δ = U. We benchmarked the resonance location by measuring the dimer imbalance as a function of the gradient strength for various tunnelling times, as illustrated in Extended Data Fig. 2. Here we expected the strongest decay of the dimer imbalance, as defined in the main text, when the resonance condition is fulfilled. For smaller gradients, we expected a slower drop in imbalance, whereas for much stronger gradients, we expected all processes to be off-resonant and no dynamics to occur at all, leading to high imbalance even at later times.

    Our experimental results match the described expectation qualitatively. To confirm that we were not accidentally probing at a time where the imbalance shows any Δ-dependent oscillations, we probed for multiple fixed evolution times (up to t/τ = 40), observing consistent behaviour for all of the chosen evolution times. The resonance width is inherently limited by the finite tunnelling bandwidth and residual potential disorder. Our chosen operation point was located at the centre of the resonance and showed the strongest decay, as marked by the vertical dashed line in Extended Data Fig. 2. On the basis of our gradient calibration presented above and in Extended Data Fig. 1b, this point corresponds to a value of Δ = h × 238(3) Hz.

    Comparing with our independent band-structure calculation, we found a qualitative agreement within 15% to the value of U for both calibration methods of the Hubbard parameters described above. In particular, U changes only very slowly with the lattice depth and varies by less than J for our calibrations. As such, this gradient setpoint remains valid throughout all measurements.

    Data analysis

    All data, unless specified differently, were analysed as explained in the following: we calculated the quantity of interest (imbalance, Fourier components, diagonal sums) on the individual experimental shots, then averaged over these results to obtain the data shown in the figures. For the reference-subtracted defect occupations (Fig. 4b, middle, and Extended Data Fig. 4b), we subtracted the densities averaged over all shots. To calculate the imbalances in Fig. 5c,d, we chose the boundary of the respective ROIs such that atoms close to the interface boundary that could be part of either the chequerboard or the dimer were counted as belonging to the dimer part of the system. As such, we obtained the same number of atoms for both halves of the system and the imbalance can, in principle, reach its typical limits of ±1; this explains the perhaps unintuitive shape of the ROIs shown in Fig. 5b.

    Fourier analysis

    To analyse the Fourier components of the average densities, we calculated the discrete Fourier transform according to

    $$\begin{array}{l}F({\bf{k}})\,=\,\mathop{\sum }\limits_{n=0}^{N-1}\mathop{\sum }\limits_{m=0}^{M-1}{a}_{n,m}\exp \,\left(-2{\rm{\pi }}i(\frac{nj}{N}+\frac{ml}{M})\right)\\ \,\,=\mathop{\sum }\limits_{n=0}^{N-1}\mathop{\sum }\limits_{m=0}^{M-1}{a}_{n,m}\exp (\,-\,{\rm{i}}{k}_{x}n-{\rm{i}}{k}_{y}m)\end{array}$$

    (4)

    with an,m the average densities at site n, m for an ROI of size N × M and \({k}_{x}=\frac{2{\rm{\pi }}j}{N},{k}_{y}=\frac{2{\rm{\pi }}l}{M}\). Here the index j runs from \(-\left(\frac{N-1}{2}\right),\ldots ,0,\ldots ,\frac{N-1}{2}\) for odd N and \(\lceil \frac{N-1}{2}\rceil ,\ldots ,0,\ldots ,\frac{N}{2}\) for even N and analogously for l. The value at (kx, ky) = (0, 0) is just the sum of the signal; it contains no additional relevant information and is thus neglected (white rectangles in the insets of Fig. 3).

    It is noted that the discrete Fourier transform obeys point reflection symmetry, that is, F(k) = F(−k). Therefore, in the main text, we plot only the parts of the momentum space (kx, ky) that contain non-redundant information.

    Isolated dimer dynamics

    To further understand and investigate the decay of the dimer pattern on a microscopic level, we prepared isolated dimers and tracked their evolution after a sudden quench. We isolated the dimers by adding empty columns between the atom pairs, as illustrated in the inset of Extended Data Fig. 3. For this configuration, the dimers were, including only first-order processes, completely decoupled from one another, allowing us to study the formation of the horizontally oriented dimers described in Fig. 3a. The change in orientation can be understood intuitively. Starting from a dimer, the upper atom can tunnel onto the neighbouring site by forming a doublon, as illustrated in the middle inset of Extended Data Fig. 3. From there, the atoms can either rearrange into the original dimer or into the flipped dimer, which is energetically degenerate to the original dimer configuration.

    Extended Data Fig. 3 shows the time evolution of the isolated dimers. Here we plot the populations of the three possible states: the vertical dimer, the doublon and the horizontal dimer. Although the dimer states can be detected unambiguously, we assigned the doublon if all three sites were empty. To correct, on average, for cases where no atoms were initially prepared, we subtracted the value obtained analogously from a reference measurement tracking the initial-state preparation. We observed a clear oscillation between the two cases of vertically and horizontally oriented dimers, which quickly dephases owing to residual potential disorder. We compared the measured data with a numerical simulation of a three-state model given by

    $$\widehat{H}=\left(\begin{array}{ccc}{\delta }_{i} & \sqrt{2}J & 0\\ \sqrt{2}J & U-\varDelta +{\delta }_{j} & \sqrt{2}J\\ 0 & \sqrt{2}J & {\delta }_{k}\end{array}\right)$$

    (5)

    where δi, δj, δk describe the disorder strength between adjacent sites. For the calculation, we sampled δi, δj, δk from a normal distribution around zero and averaged over N = 100 such realizations. The additional factor of \(\sqrt{2}\) for the hopping has to be taken into account owing to the bosonic enhancement characteristic for indistinguishable bosons. We then fitted the calculations to the measured occupation of the vertical and horizontal dimers to generate the solid lines in Fig. 3b. Here we allowed for the disorder strength, the difference U − Δ, an overall amplitude (which respects normalization) as well as the timescale as free fit parameters. The initial time offset was kept fixed at zero. It is noted that the doublon occupation was not included in the fits, instead the solid line in Extended Data Fig. 3 is given by the model expectation using the fit values obtained from fitting the two other curves. We observed good agreement between the doublon occupation as obtained from our measured data and the numerical model using the fit parameters for the two other curves, validating our method of extracting the doublon occupation.

    From the fit, we extracted the standard deviation of the disorder distribution σ = 1.2(1) × J, a deviation from resonance of U − Δ = 0.0(3) × J and a timescale of τ = 10.0(3) ms. The latter can serve as a secondary way to calibrate the Hubbard parameters of our system (see above).

    Negative defect and additional analysis

    Here we present our measurements on the negative defect and describe the data presented in Fig. 4 and Extended Data Fig. 4 in more detail. We also present an alternative way of evaluating the data for the positive defect and directly compare the spreading of the defect holes for both the negative and the positive defects.

    The spreading of the defects can be observed directly in the average occupations (Fig. 4b and Extended Data Fig. 4b, leftmost column), through a reduced contrast of the (background) chequerboard on sites accessible to the defect atoms. This is owing to the following processes. First, the defect atoms can move to initially empty sites of the chequerboard, thereby increasing the average density on these sites. The defect atoms can also move onto initially occupied sites of the chequerboard, where we then observe a reduced average density owing to parity projection. Finally, nearby atoms from the background chequerboard can become mobile owing to the presence of the defect and move onto the site occupied by the defect atom, thus reducing the average density on their original sites as well as on the site of the defect atom owing to parity projection. For the negative defect in particular, the motion of the hole can be observed by an increase of the average occupation on its initial site (see also Extended Data Fig. 5b in the following), and a simultaneous decrease of the average occupation on the neighbouring sites on its equipotential line. By contrast, the hole site for the positive defect remains unoccupied. These effects are highlighted by subtracting the occupation of a chequerboard state without deterministically created defects. Initially empty sites accessible to the defect atoms will feature a positive, reference-subtracted value, whereas initially occupied sites accessible to the defect atoms will show negative values. The latter, as explained above, is due to either parity projection, atoms becoming mobile owing to the defect or, for the case of the negative defect, also the spreading of the defect hole. When comparing with theory, we observed good agreement, especially for the negative defect (Extended Data Fig. 4b,c). For the simulations, we did not include any experimental imperfections such as disorder and initial-state preparation fidelities. We further quantified the directional spreading of the defects by summing along the diagonals of the reference-subtracted occupations. When summing parallel to the equipotential lines, the occupation is only different from zero on the diagonals on which the defect atom and hole were initially placed. The growth by one additional diagonal for times t/τ > 0 can be explained by the above-mentioned processes, that is, the defect’s influence on the neighbouring atoms. As an additional characterization of the positive defect, we also studied the spreading on the zigzag-shaped equipotential line (Extended Data Fig. 5a, inset) instead of summing the reference-subtracted signal along the ROI diagonals. The result of this analysis is shown in Extended Data Fig. 5a. Here we again observe that the spread occurs along only one direction, as the immobile hole prevents the spread in the opposite direction. The latter is expected, as the hole can only move by second-order processes8. This is also evidenced by the density on the site of the hole remaining nearly unchanged.

    Looking at this further, by comparing the increase of the densities on the sites initially occupied by the defect holes, we can also clearly observe the difference between the positive and the negative defects (Extended Data Fig. 5b). For the positive defect, the density increased only slightly, whereas for the negative defect we observed an immediate, fast increase, as here the hole is mobile in first order. Specifically, the hole of the negative defect can move in processes where neighbouring particles located on the equipotential line above the defect atom hop onto the defect atom and then to the site of the hole (Extended Data Fig. 4a, bottom right). The hole’s motion is restricted to its initial equipotential line. As for all other measurements on the spreading of defects on top of the chequerboard background, we attribute deviations from the theoretical expectations to disorder in the system and imperfect initial-state preparation, that is, the presence of additional, non-deterministic defects.

    Numerical methods for defects

    The underlying physics in the Bose–Hubbard model is described by an effective Hamiltonian derived in ref. 8, which features HSF. In Extended Data Fig. 6, we compare the time evolution of the positive defect under this effective Hamiltonian with the time evolution of the original Bose–Hubbard model. We show the parity-projected on-site occupation and have subtracted a perfect chequerboard state (at t/τ = 0, that is, without time evolution) to better highlight the differences. It is noted that in Fig. 4 and Extended Data Figs. 4 and 5a, we instead subtract the theory calculations with a time-evolved version of the chequerboard for better comparison with the experimental data. In contrast to the effective model, the background chequerboard state is not completely frozen under time evolution with the Bose–Hubbard model. Nevertheless, this additional dynamics of the background does not strongly influence the dynamics of the mobile defect compared with the effective model. Therefore, we conclude that the underlying physics of the Bose–Hubbard model in the chosen limits are well captured by the effective model featuring HSF.

    Numerical methods for convergence

    The data were obtained using tensor-network methods and exact diagonalization. All data were calculated by matrix-product-operator time evolution using the TeNPy package46,47, except for the time evolution with the effective model in Extended Data Fig. 6, which was performed with exact diagonalization. In Extended Data Fig. 7, convergence in the bond dimension and in the Trotter step is studied. In Extended Data Fig. 7a, the evolution of the imbalance for the chequerboard and dimer states shows perfect overlap for bond dimensions χ = 256 and χ = 300. For both curves, a Trotter step size of dt = 0.001 was used. In Extended Data Fig. 7b, the imbalance is compared for Trotter step sizes of dt = 0.001 and dt = 0.0005 at a fixed bond dimension of χ = 256.

    Numerical methods for imbalance

    In Extended Data Fig. 7c, we compare the imbalance of the perfect case to the time evolution under imperfect conditions, similar to those of the experiment. For the latter, we have included deviations of all relevant quantities away from optimum, fidelities for state preparation and an additional random on-site potential (see the caption of Extended Data Fig. 7 for details). Each time step is averaged over Nav,dimer [29, 100], Nav,squares [17, 100], Nav,CHB [10, 100] different preparations. We find that the effect of state-dependent dynamics is still clearly visible also for experimental conditions. For the dimer state, the impact of experimental conditions is the strongest, which we attribute to the highest sensitivity to imperfect state preparation. In the case of the dimer state, all atoms have only one nearest neighbour. Removing this neighbour directly leads to a decrease in mobility and can induce frozen particles. By contrast, the squares state does not suffer from this effect on the same level. Each atom has three nearest neighbours, and therefore one missing neighbour does not lead to frozen sites.

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