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Characterize arbitrary quantum networks in the noisy intermediate-scale quantum era

Zhen-Peng Xu [email protected] School of Physics and Optoelectronics Engineering, Anhui University, 230601 Hefei, China Naturwissenschaftlich-Technische Fakultät, Universität Siegen, Walter-Flex-Straße 3, 57068 Siegen, Germany
Abstract

Quantum networks are of high interest nowadays. In short, it describes the distribution of quantum sources represented by edges to different parties represented by nodes in the network. Bundles of tools have been developed recently to characterize quantum states from the network in the ideal case. However, features of quantum networks in the noisy intermediate-scale quantum (NISQ) era invalidate most of them and call for feasible tools. By utilizing purity, covariance and topology of quantum networks, we provide a systematic approach to tackle with arbitrary quantum networks in the NISQ era, which can be noisy, intermediate-scale, random and sparse. One application of our method is to witness the progress of essential elements in quantum networks, like the quality of multipartite entangled sources and quantum memory.

pacs:
03.65.Ta, 03.65.Ud

Numerous works have advertised from different scales the advent of quantum network technology, as small as the storage of a single entangled pair [1], and as broad as quantum internet [2, 3, 4]. Apart from the theoretical importance, quantum networks appear naturally in practice, especially in quantum key distribution [5, 6], quantum network metrology [7, 8, 9] and quantum distributed computation [10]. A recent move is into the characterization of different quantum correlations arising from quantum networks [11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23].

A quantum network can be abstracted as a hypergraph, where each node stands for a local lab and each hyperedge represents a quantum source that distributes particles only to labs associated with the corresponding nodes, see Fig. 1 for examples. A correlated quantum network (CQN) allows the pre-shared classical protocol, i.e., global classical correlation [12], an independent quantum network (IQN) allows not. Despite recent progress [11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23], the study of quantum network states is still in its cradle. Past research has focused mainly on IQN, bundles of tools [17, 24, 18, 19, 25] have been added into the current toolbox. However, they become incapable to detect the underlying structure of CQN even when only a small amount of global classical correlation appears. In comparison, few methods [11, 12, 11, 13, 14, 15] exist for CQN, which either work only for special kinds of states like symmetric states [13, 15, 14], limited quantum networks like the triangle network [11, 12] or complete nn-partite network with (n1)(n-1)-partite sources [26, 27, 28]. However, an undeniable fact is that we progress toward the noisy intermediate-scale quantum (NISQ) era, as pointed out sagaciously by Preskill [29]. The global classical correlation exists then frequently in real applications, which can even elicit from the flap of a butterfly’s wings in Brazil [30].

Refer to caption
Figure 1: Three quantum networks, where each node stands for one local lab, one edge in real line represents a genuine bipartite entangled quantum source shared by different labs in the corresponding nodes, and one edge in dashed line represents a separable quantum source. In practice, the quantum network in (a) can degenerate to the one in (b), even to the one in (c).

Apart from the unavoidable global noise, quantum networks in the NISQ era share at least other three features: intermediate-scale, random, and sparse. Though the size of quantum networks in the NISQ era is limited, it can be not small, considering that IBM has unveiled a quantum chip with 433433 qubits [31] already. The randomness in the network [32] can originate from the random establishment of quantum links with quantum repeaters [33, 34], and also the decoherence of established links as considered in waiting time [35]. Degeneration of a triangle quantum network until a classical network is illustrated in Fig. 1. Since genuine multipartite entanglement is hard to prepare and to maintain [36, 37], the realistic quantum networks will be sparse. Tools for quantum networks in the NISQ era regarding those features are still missing.

In this work, we characterize correlated quantum networks in the NISQ era by employing the purity of the state and covariance of the measured data. Those methods are operational in the sense that only the available experiment data is employed, without knowing the exact underlying quantum state. Purity of the network state plays an essential role here, as the classical correlation in a state can be captured by its purity. Pretty recent research shows that the purity of a multipartite state can be evaluated efficiently with only local operations [38, 39], which fits the network scenario. The methods developed here are feasible for noisy intermediate-scale or big quantum networks. Interestingly, they work even for a collection of networks with different kinds of topology, which can cover the random network models, especially the ones with probabilistic genuine bipartite sources as in the consideration of quantum repeaters [33]. Thus, they answer one corresponding open question in the review paper on nonlocality in quantum networks [22]. We can also apply our methods to a part of the network instead of the whole, which fits the sparse structure of the network in the NISQ era and reduces the difficulty of computation.

GHZ state under decoherence.— As a warming-up exercise we discuss the Greenberger-Horne-Zeilinger (GHZ) state of nn qubits under decoherence,

ρ(α)=(1α)|GHZ+GHZ+|+α|GHZGHZ|,\rho(\alpha)=(1-\alpha)|{\rm GHZ}_{+}\rangle\langle{\rm GHZ}_{+}|+\alpha|{\rm GHZ}_{-}\rangle\langle{\rm GHZ}_{-}|, (1)

where |GHZ±=(|00±|11)/2|{\rm GHZ}_{\pm}\rangle=(|0\cdots 0\rangle\pm|1\cdots 1\rangle)/\sqrt{2}, and α[0,1/2]\alpha\in[0,1/2] describes the degree of decoherence. Despite its simplicity, this example allows us to introduce our main ideas.

If all the nn parties implement the same measurement Z=|00||11|Z=|0\rangle\langle 0|-|1\rangle\langle 1|, then two possible combinations of outcomes happen equally with probability 1/21/2, i.e., either all of the outcomes are 0, or all of them are 11. To simulate this statistical behaviour without genuine nn-partite entanglement, the state for simulation can only be ρc=[|0000|+|1111|]/2\rho_{c}=[|0\cdots 0\rangle\langle 0\cdots 0|+|1\cdots 1\rangle\langle 1\cdots 1|]/2, since no other 010-1 string appear as a combination of outcomes. Such a simulation invalidates known methods with only statistical data [19, 26, 27, 28]. It costs at least one classical bit of randomness, as the Shannon entropy or the Von Neumann entropy of ρc\rho_{c} is 11. However, the Von Neumann entropy of the state ρ(α)\rho(\alpha) is [αlogα+(1α)log(1α)]-[\alpha\log\alpha+(1-\alpha)\log(1-\alpha)], which is strictly less than 11 for α[0,1/2)\alpha\in[0,1/2). This means that we cannot simulate the statistical behaviour and the Von Neumann entropy of ρ(α)\rho(\alpha) simultaneously by a quantum network with at most (n1)(n-1)-partite sources.

The Von Neumann entropy is one way to measure the purity of the state, capturing partially the classical correlations in the state. To continue, we examine firstly different measures of purity and choose a suitable one for our following methods. For a given state ρ\rho in the dd-dimensional space, the common measures of its purity [40, 41, 42] are Rényi α\alpha-purity log2dlog2(Tr(ρα))/(1α)\log_{2}d-\log_{2}(\operatorname{Tr}(\rho^{\alpha}))/(1-\alpha), which converges to the Von Neumann entropy as α\alpha tends to 11, and linear entropy purity Tr(ρ2)1/d\operatorname{Tr}(\rho^{2})-1/d. Through the whole text, we take τ=Tr(ρ2)\tau=\operatorname{Tr}(\rho^{2}) to quantify the purity, which determines Rényi 2-purity and linear entropy purity. The advantage of τ\tau over other quantifiers, like the Von Neumann entropy, is that it fits the covariance of experimental data well in our approach, as both of them contain the information of ρ2\rho^{2}. As for the estimation of purity of a multipartite state with different measures, it can be done efficiently with only local operations [38, 39], which are feasible in the network scenario.

Noisy quantum networks.— Noise is unavoidable for the quantum network states in the NISQ era, either the local noise or the global one. Quantum networks with different noise models can all be classified as CQNs. Firstly, we develop the covariance matrix decomposition method for CQN, where a key step is to separate the part related to global classical correlation out in the whole covariance matrix. For a given hypergraph G(V,E)G(V,E) and a state ρ\rho from CQN of GG, the state ρ\rho can be decomposed as

ρ=kpkρk,ρk=(iV𝒞i(k))(eEηe(k)),\displaystyle\rho=\sum\nolimits_{k}p_{k}\rho_{k},\ \rho_{k}=\Big{(}\bigotimes\nolimits_{i\in V}\mathcal{C}_{i}^{(k)}\Big{)}\Big{(}\bigotimes\nolimits_{e\in E}\eta_{e}^{(k)}\Big{)}, (2)

where {pk}k\{p_{k}\}_{k} with kpk=1\sum_{k}p_{k}=1 and pk>0p_{k}>0 is the global classical correlation, 𝒞i(k)\mathcal{C}_{i}^{(k)} is a local channel for the ii-th party, ηe(k)\eta_{e}^{(k)} is an entangled state distributed from the source labeled by the hyperedge ee.

For simplicity, we assume each party has only one measurement, and denote MiM_{i} the measurement for the ii-th party. Then we introduce three kinds of covariance matrices, Γ\Gamma, Γ(k)\Gamma^{(k)} and Γ(c)\Gamma^{(c)}, whose elements in the ii-th row and jj-th column are Γij\Gamma_{ij}, Γij(k)\Gamma_{ij}^{(k)} and Γij(c)\Gamma^{(c)}_{ij}, respectively, where

Γij\displaystyle\Gamma_{ij} =MiMjMiMj,Mi=Tr(ρMi),\displaystyle=\braket{M_{i}M_{j}}-\braket{M_{i}}\braket{M_{j}},\ \braket{M_{i}}=\operatorname{Tr}(\rho M_{i}),
Γij(k)\displaystyle\Gamma^{(k)}_{ij} =MiMjkMikMjk,Mik=Tr(ρkMi),\displaystyle=\braket{M_{i}M_{j}}_{k}-\braket{M_{i}}_{k}\braket{M_{j}}_{k},\ \braket{M_{i}}_{k}=\operatorname{Tr}(\rho_{k}M_{i}),
Γij(c)\displaystyle\Gamma^{(c)}_{ij} =kpkMikMjkMiMj.\displaystyle=\sum\nolimits_{k}p_{k}\braket{M_{i}}_{k}\braket{M_{j}}_{k}-\braket{M_{i}}\braket{M_{j}}. (3)

The covariance matrix Γ\Gamma is the one that can be observed directly in experiments. The covariance matrices {Γ(k)}k\{\Gamma^{(k)}\}_{k} are hidden in the experimental data when we assume that the randomness of the sampling {pk,ρk}k\{p_{k},\rho_{k}\}_{k} is inaccessible. The covariance matrix Γ(c)\Gamma^{(c)} can be viewed as a classical covariance matrix, since it is only about the distribution of classical data {M1k,,Mnk}k\{\braket{M_{1}}_{k},\ldots,\braket{M_{n}}_{k}\}_{k}. Throughout the whole paper, we only consider the dichotomic measurements with outcomes ±1\pm 1. A pivotal observation is that the classical covariance matrix Γ(c)\Gamma^{(c)} can be separated out from the observed one Γ\Gamma perfectly, i.e.,

Γ=kpkΓ(k)+Γ(c),\displaystyle\Gamma=\sum\nolimits_{k}p_{k}\Gamma^{(k)}+\Gamma^{(c)}, (4)

whose proof can be found in Sec. A in Supplemental Material (SM) [43]. Since {Γ(k)}k\{\Gamma^{(k)}\}_{k} are about network states from IQN, the existing method in Ref. [19] can be employed to impose constraints on them. However, if there is no limitation of Γ(c)\Gamma^{(c)}, the observed covariance matrix Γ\Gamma can still have arbitrary relation with the network topology GG. As it turns out, the purity of the state implies a nontrivial condition on Γ(c)\Gamma^{(c)}, leading to a semi-definite programming (SDP) to determine whether a state can arise from CQN with a given topology.

Observation 1.

For a given state ρ\rho from the CQN with the network topology G(V,E)G(V,E), measurements {Mi}iV\{M_{i}\}_{i\in V}, which result in the covariance matrix Γ\Gamma, it holds that

Γ=eEΥe+T,ΠeΥeΠe=Υe0,\displaystyle\Gamma=\sum\nolimits_{e\in E}\Upsilon_{e}+T,\ \Pi_{e}\Upsilon_{e}\Pi_{e}=\Upsilon_{e}\succeq 0,
T0,maxiVTiiβ,Tr(T)l1β,\displaystyle T\succeq 0,\ \max\nolimits_{i\in V}T_{ii}\leq\beta,\ \operatorname{Tr}(T)\leq l_{1}\beta, (5)

where l1l_{1} is the maximal eigenvalue of iVMiMi\sum_{i\in V}M_{i}\otimes M_{i}, β=21τ2\beta=2\sqrt{1-\tau^{2}}, TiiT_{ii} is the ii-th diagonal term of TT, Πe=iePi\Pi_{e}=\sum_{i\in e}P_{i} with PiP_{i} to be the projection onto ii-th row.

To apply the criterion in this observation, we need firstly estimate the purity of the state ρ\rho, and then implement the measurements {Mi}i\{M_{i}\}_{i} and obtain the covariance matrix from the experimental data. It should work for arbitrary network topology with around 5050 nodes in practice. This observation can be understood as follows. The term eEΥe\sum_{e\in E}\Upsilon_{e} corresponds to kpkΓ(k)\sum_{k}p_{k}\Gamma^{(k)}, as each Γ(k)\Gamma^{(k)} has a similar decomposition [19]. The variable TT plays the role of Γ(c)\Gamma^{(c)} and inherits all its constraints. A detailed proof is provided in Sec. B in SM [43]. The application of Observation 1 to the triangle quantum network is illustrated in Fig. 2. We remark that the rank of the state determines the Rényi-0 purity which reads log2(d/r)\log_{2}(d/r). By considering the rank rr also, we can set β=min{r(1τ),21τ2}\beta=\min\{r(1-\tau),2\sqrt{1-\tau^{2}}\} as a tighter bound.

Refer to caption
Figure 2: The decomposition of the covariance matrix Γ\Gamma of a noisy state from the triangle network, where each matrix contains 99 elements, the elements in the blank area are 0. The block structure of each Υe\Upsilon_{e} imposes a constraint on itself. The critical step is to obtain constraints of Γ(c)\Gamma^{(c)} from available information of the quantum network, like purity.

Revisit GHZ state under decoherence.— We take the state ρ(α)\rho(\alpha) in Eq. (1) and measurements ZZ for all parties as an example to illustrate Observation 1. The covariance matrix Γ\Gamma of ρ(α)\rho(\alpha) contains always only 11 as its elements.

If Γ\Gamma is from the statistics of a state in a network without nn-partite sources, then Γ\Gamma should satisfy the decomposition in Eq. (1), where GG is the hypergraph with nn nodes and includes all subsets with (n1)(n-1) elements as hyperedges. Notice that, the rank of Γ\Gamma is 11, and ΓΥe0\Gamma\succeq\Upsilon_{e}\succeq 0, which implies that each Υe\Upsilon_{e} should be proportional to Γ\Gamma.

Since Υe\Upsilon_{e} always contains element 0 as exemplified in Fig. 2, we have Υe=0\Upsilon_{e}=0, for all eEe\in E. Consequently, T=ΓT=\Gamma and maxiTii=1\max_{i}T_{ii}=1. The rank of the state ρ(α)\rho(\alpha) is however 22 and the purity is τ=12α+2α2\tau=1-2\alpha+2\alpha^{2}. Thus, β=1\beta=1 happens only for α=1/2\alpha=1/2, in which case ρ(α)\rho(\alpha) is fully separable. This leads to the conclusion that ρ(α)\rho(\alpha) can arise from a network without nn-partite sources if and only if α=1/2\alpha=1/2. Our criterion is therefore tight.

Intermediate-scale networks.— The advantage of covariance matrix decomposition is that it requires only experimental data of few measurements and information of purity. However, the computation becomes heavy for intermediate-scale networks with around 500500 nodes, due to the complexity of SDP in the method.

Here we propose another approach to solve this issue, which can even take care of the randomness feature in the NISQ era. Firstly, we introduce the fact that ij|Mij|rTr(M)\sum_{ij}|M_{ij}|\leq r\operatorname{Tr}(M) for a semidefinite matrix MM whose rank is rr, and take the triangle network as an example. According to the decomposition of Γ\Gamma in Observation 1, ij|Γij|ije[|Υe,ij|+|Γij(c)|]e2Tr(Υe)+3Tr(Γ(c))\sum_{ij}|\Gamma_{ij}|\leq\sum_{ij}\sum_{e}[|\Upsilon_{e,ij}|+|\Gamma^{(c)}_{ij}|]\leq\sum_{e}2\operatorname{Tr}(\Upsilon_{e})+3\operatorname{Tr}(\Gamma^{(c)}), where the last inequality is from the block structures of Υe\Upsilon_{e}’s and Γ(c)\Gamma^{(c)} as in Fig. 2. Consequently, ij|Γij|2Tr(Γ)+Tr(Γ(c))\sum_{ij}|\Gamma_{ij}|\leq 2\operatorname{Tr}(\Gamma)+\operatorname{Tr}(\Gamma^{(c)}) by applying the first equality in Eq. (1) again. For the general network topology G(V,E)G(V,E) with V={1,,n}V=\{1,\ldots,n\} and kk to be the maximal size of hyperedges in EE, we have

i,j|Γij|kTr(Γ)+(nk)Tr(Γ(c)).\sum\nolimits_{i,j}|\Gamma_{ij}|\leq k\operatorname{Tr}(\Gamma)+(n-k)\operatorname{Tr}(\Gamma^{(c)}). (6)

In practice, we can replace Tr(Γc)\operatorname{Tr}(\Gamma^{c}) in Eq. (6) by any estimation of it, like the analytical upper bound in Eq. (1) results from series of relaxations [43]. A good estimation plays a vital role in the efficiency of the inequality here, same as in the criterion in Observation 1. Nowadays, it is still hard to prepare genuine multiparite entangled states for a large system [36]. Thus, kk is usually much smaller than nn in Eq. (6), i.e., small sources in a big network.

Random networks.— The establishment of genuine multipartite entanglement among remote labs is usually random as in the scenario of quantum repeaters [33]. The established one can still degenerate to less-partite ones randomly due to decoherence. This urges us to introduce the concept of random network, where the genuine multipartite entanglement in each source exists probabilistically. As an example, we consider a genuine tripartite entangled source, whose degeneration is captured by the triangle network in Fig. 2, assumed to be with probability pp. The network state ρ\rho has then the decomposition ρ=pi=13qiρi+(1p)ρ0\rho=p\sum_{i=1}^{3}q_{i}\rho_{i}+(1-p)\rho_{0}, where ρ0\rho_{0} is the original tripartite state and other ρi\rho_{i}’s are independent triangle network states, iqi=1\sum_{i}q_{i}=1 and qi0q_{i}\geq 0. This leads to the covariance matrix Γ=pi=13qiΓ(i)+(1p)Γ(0)+Γ(c)\Gamma=p\sum_{i=1}^{3}q_{i}\Gamma^{(i)}+(1-p)\Gamma^{(0)}+\Gamma^{(c)}, where Γ(i)\Gamma^{(i)}’s are the covariance matrices for ρi\rho_{i}’s, and Γ(c)\Gamma^{(c)} is the classical one. As argued before, Γ~:=i=13qiΓ(i)\tilde{\Gamma}:=\sum_{i=1}^{3}q_{i}\Gamma^{(i)} has the decomposition eEΥe\sum_{e\in E}\Upsilon_{e} as in Fig. 2, which implies that i,j=13|Γ~ij|2Tr(Γ~)\sum_{i,j=1}^{3}|\tilde{\Gamma}_{ij}|\leq 2\operatorname{Tr}(\tilde{\Gamma}). Consequently,

i,j|Γij|\displaystyle\sum\nolimits_{i,j}|\Gamma_{ij}| 2pTr(Γ~)+3[(1p)Tr(Γ(0))+Tr(Γ(c))]\displaystyle\leq 2p\operatorname{Tr}(\tilde{\Gamma})+3[(1-p)\operatorname{Tr}(\Gamma^{(0)})+\operatorname{Tr}(\Gamma^{(c)})]
=2Tr(Γ)+[(1p)Tr(Γ(0))+Tr(Γ(c))]\displaystyle=2\operatorname{Tr}(\Gamma)+[(1-p)\operatorname{Tr}(\Gamma^{(0)})+\operatorname{Tr}(\Gamma^{(c)})]
2Tr(Γ)+3(1p)+Tr(Γ(c)),\displaystyle\leq 2\operatorname{Tr}(\Gamma)+3(1-p)+\operatorname{Tr}(\Gamma^{(c)}), (7)

where the last inequality is from the fact that any variance should be no more than 11 as the outcomes of the measurements are ±1\pm 1.

This result is the very first characterization of random quantum network states, which can be generalized to arbitrary random quantum networks as follows.

Observation 2.

Assume ρ\rho is a state from the random quantum network with nn parties and ckc_{k} genuine kk-partite sources on average for each kk. If Γ\Gamma is a covariance matrix of measurements whose outcomes are ±1\pm 1, then

i,j|Γij|\displaystyle\sum\nolimits_{i,j}|\Gamma_{ij}|\leq maxkkxk+y\displaystyle\max\sum\nolimits_{k}kx_{k}+y
such that kxk+y=Tr(Γ),\displaystyle\sum\nolimits_{k}x_{k}+y=\operatorname{Tr}(\Gamma),
0xkkck,\displaystyle 0\leq x_{k}\leq kc_{k},
0y=Tr(Γ(c)).\displaystyle 0\leq y=\operatorname{Tr}(\Gamma^{(c)}). (8)

The proof is in Sec. C in SM [43]. Equation (2) is one inequality including a linear programming, which can be verified efficiently even for large random networks.

The criterion in Observation 2 is device-independent, in the sense that it works without any assumption of the underlying quantum system and measurements. Besides, it does not depend on the exact underlying network topology, but the parameters {ck}\{c_{k}\}. Such results can also be used to benchmark the quality of genuine multipartite entanglement, which degenerates randomly due to decoherence. In such a case, parameters {ck}\{c_{k}\} should be functions of time. Observation 2 answers an open question in Ref. [22] also, i.e., how to characterize the mixture of quantum networks with different kinds of topology.

Sparse networks.— In a reasonable prospect, the quantum network should be sparse in the near future. Even though we have a relatively large quantum network, the size and the amount of quantum sources would be relatively small as illustrated in Fig. 3. The exact numbers depend on the progress of quantum technologies.

Refer to caption
Figure 3: A sparse network GsG_{s} with 1313 nodes, which contains an angle (in region AA) as a sub-network. The centeral node in region BB is the filled one.

For a given state ρ\rho from a large network G(V,E)G(V,E), a necessary condition is that ρS:=TrS¯ρ\rho_{S}:=\operatorname{Tr}_{\bar{S}}\rho can arise from the network with the induced subgraph H(S,ES)H(S,E_{S}) on SS, where SS is an arbitrary subset of VV and ES={eS|eE}E_{S}=\{e\cap S|e\in E\}. Then we could apply Observations 1 and 2 for each reduced state ρS\rho_{S}. The sparsity of the network can reduce the complexity of this approach, as we do not need too many relatively small sub-networks to cover the original one. Correspondingly, we have to estimate the classical covariance matrix ΓS(c)\Gamma^{(c)}_{S} for each ρS\rho_{S}. Since ρS\rho_{S} as a reduced state could be much mixed than the original state ρ\rho, the purity of ρS\rho_{S} could lead to too loose constraints in Observation 1. A key observation here is that ΓS,ij(c)=Γij(c)\Gamma^{(c)}_{S,ij}=\Gamma^{(c)}_{ij} for any i,jSi,j\in S, with Γ(c)\Gamma^{(c)} to be the classical covariance matrix corresponding to the original network state ρ\rho. More explanations are provided in Sec. D in SM [43].

For instance, we consider the state ρ(α)\rho(\alpha) as in Eq. (1) for 1313 qubits and network GsG_{s} with only bipartite sources as shown in Fig. 3. Then the reduced state ρA(α)=(|000000|+|111111|)/2\rho_{A}(\alpha)=(|000\rangle\langle 000|+|111\rangle\langle 111|)/2 for the three qubits in region AA as in Fig. 3. The rank of ρA(α)\rho_{A}(\alpha) is two, and the covariance matrix of ρA(α)\rho_{A}(\alpha) contains only 11. Notice that, the sub-network in the region AA is a special case of the triangle network as illustrated in Fig. 1. The same argument as before implies that ΓA(c)\Gamma^{(c)}_{A} contains 11 only, which does not contradict with the purity of ρA(α)\rho_{A}(\alpha), but with the one of the original state ρ(α)\rho(\alpha) for α[0,1/2)\alpha\in[0,1/2). Thus, with the global purity and the statistical data of the qubits in the small region AA, we obtain the same tight result. This strategy saves much effort, since we only need to measure few qubits in a large network.

There is another approach to employ sub-networks to determine whether a state can arise from the original network or not, i.e., we measure out one party associated with one node vv and broadcast the outcomes. Then we can treat the party associated with node vv and all the related sources together as a new multipartite source, which distributes particles to all the parties in 𝒩(v):={u|(u,v)E}{\cal N}(v):=\{u|(u,v)\in E\}. If the original network is sparse, then the size of 𝒩(v){\cal N}(v), i.e., the size of the new introduced entangled source is usually not big. For example, if vv is the central node in region BB as in Fig. 3, then the new source distributes particles to parties associated with all the other three nodes in the region BB. We can do this procedure for a subset SS of nodes sequentially. By applying Observations 1 and 2 for the resulting sub-network, we can obtain new criteria for the original network state.

Discussion.— Quantum networks work as a playground for various quantum technologies, like quantum repeaters and quantum memory. Concerning the real-life implementation of quantum networks, we examine them in the background of the noisy intermediate-scale quantum (NISQ) era. In this paper, we have focused on four aspects of such quantum networks, that is, they should be noisy, intermediate-scale, random, and sparse. We developed operational methods based on purity and covariance to address all those four features.

There exist already methods to tackle with the noisy quantum network states, e.g., the witness based on fidelity [11, 12, 14, 15] and nonlocality inequalities [28, 27, 26]. However, the witness based on fidelity works mostly either for small networks or special states like graph states in practice. The nonlocality inequalities are designed specially for the nn-partite network with all (n1)(n-1)-partite sources. In comparison, our methods work for any kind of network topology, by employing experiment data only, without knowing the exact underlying quantum state and measurements. Nevertheless, quantum theory is assumed here, which is another difference between our consideration and network nonlocality.

‘Quantum technologists should continue to strive for more accurate quantum gates and, eventually, fully fault-tolerant quantum computing’ [29] and networks, for which our methods can provide the witness.

Acknowledgements.— I thank David Gross, H Chau Nguyen, Julio I. de Vicente, Kiara Hansenne, Mariami Gachechiladze, Nikolai Wyderka, Otfried Gühne, Shu-Heng Liu, Sixia Yu, Tristan Kraft, especially Laurens Ligthart and Thomas Cope for discussions and suggestions. Moreover, I would like to thank Tristan Kraft for careful reading of the manuscript. This work was supported by National Natural Science Foundation of China (Grant No. 12305007) and Anhui Provincial Natural Science Foundation (Grant No. 2308085QA29), the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation, project numbers 447948357 and 440958198), the Sino-German Center for Research Promotion (Project M-0294), the ERC (Consolidator Grant 683107/TempoQ), the Alexander Humboldt foundation.

Supplemental Material of
“Characterize arbitrary quantum networks in the noisy intermediate-scale quantum era”
Zhen-Peng Xu

School of Physics and Optoelectronics Engineering, Anhui University, 230601 Hefei, China and
Naturwissenschaftlich-Technische Fakultät, Universität Siegen, Walter-Flex-Straße 3, 57068 Siegen, Germany

I A. Covariance Matrix of mixed state

For a given state ρ=kpkρk\rho=\sum_{k}p_{k}\rho_{k} and a set of observables {Mi}\{M_{i}\}, denote

Γij=Tr(MiMjρ)Tr(Miρ)Tr(Mjρ),\displaystyle\Gamma_{ij}=\operatorname{Tr}(M_{i}M_{j}\rho)-\operatorname{Tr}(M_{i}\rho)\operatorname{Tr}(M_{j}\rho), (9)
Γij(k)=Tr(MiMjρk)Tr(Miρk)Tr(Mjρk),\displaystyle\Gamma_{ij}^{(k)}=\operatorname{Tr}(M_{i}M_{j}\rho_{k})-\operatorname{Tr}(M_{i}\rho_{k})\operatorname{Tr}(M_{j}\rho_{k}), (10)
Γijc=kpkTr(Miρk)Tr(Mjρk)Tr(Miρ)Tr(Mjρ).\displaystyle\Gamma_{ij}^{c}=\sum_{k}p_{k}\operatorname{Tr}(M_{i}\rho_{k})\operatorname{Tr}(M_{j}\rho_{k})-\operatorname{Tr}(M_{i}\rho)\operatorname{Tr}(M_{j}\rho). (11)

Then we have

Γij=kpkΓij(k)+Γijc.\Gamma_{ij}=\sum_{k}p_{k}\Gamma_{ij}^{(k)}+\Gamma_{ij}^{c}. (12)

Besides, the matrices Γ=(Γij)\Gamma=(\Gamma_{ij}), Γ(k)=(Γij(k))\Gamma^{(k)}=(\Gamma_{ij}^{(k)}), Γc=(Γijc)\Gamma^{c}=(\Gamma_{ij}^{c}) are positive semi-definite.

II B. Estimation of mean value and variance

Lemma 5.

If the mixed state ρ\rho has the decomposition

ρ=kpkρk,pk>0,\rho=\sum_{k}p_{k}\rho_{k},p_{k}>0, (13)

then

rank(ρρk)rank(ρ).\operatorname{rank}(\rho-\rho_{k})\leq\operatorname{rank}(\rho). (14)
Proof.

Denote Π\Pi the projection onto the subspace SρS_{\rho} spanned by the eigenstates of ρ\rho. By definition,

ΠρΠ=ρ,\Pi\rho\Pi=\rho, (15)

which implies that

kpk(ρkΠρkΠ)=0.\sum_{k}p_{k}(\rho_{k}-\Pi\rho_{k}\Pi)=0. (16)

Since ρkΠρkΠ0\rho_{k}-\Pi\rho_{k}\Pi\succeq 0, we have ΠρkΠ=ρk\Pi\rho_{k}\Pi=\rho_{k}, k\forall k. Hence, rank(ρρk)\operatorname{rank}(\rho-\rho_{k}) is no more than the dimension of SρS_{\rho}, which, by definition, is rank(ρ)\operatorname{rank}(\rho). ∎

Lemma 6.

For any projector PP, and two states ρ,σ\rho,\sigma where σ\sigma is in the range of ρ\rho, denote M=2P𝟙M=2P-\mathds{1}, we have

Tr(M(ρσ))RρσF,\operatorname{Tr}(M(\rho-\sigma))\leq\sqrt{R}\left\lVert\rho-\sigma\right\rVert_{\rm F}, (17)

where R=maxnrank(σ)4n(rn)rR=\max_{n\leq\operatorname{rank}(\sigma)}\frac{4n(r-n)}{r}, r=rank(ρ)r=\operatorname{rank}(\rho) and F\left\lVert\cdot\right\rVert_{\rm F} is the Frobenius norm.

Proof.
Tr(P(ρσ))=Tr(P(ρσ)+)Tr(P(ρσ))Tr(P(ρσ)+)Tr((ρσ)+)=λi>0λi,\displaystyle\operatorname{Tr}(P(\rho-\sigma))=\operatorname{Tr}(P(\rho-\sigma)^{+})-\operatorname{Tr}(P(\rho-\sigma)^{-})\leq\operatorname{Tr}(P(\rho-\sigma)^{+})\leq\operatorname{Tr}((\rho-\sigma)^{+})=\sum_{\lambda_{i}>0}\lambda_{i}, (18)

where (ρσ)±(\rho-\sigma)^{\pm} are the non-negative and negative part of ρσ\rho-\sigma, that is,

ρσ=(ρσ)+(ρσ).\rho-\sigma=(\rho-\sigma)^{+}-(\rho-\sigma)^{-}. (19)

Tr(ρσ)=0\operatorname{Tr}(\rho-\sigma)=0 implies that

λi>0λi+λi<0λi=0.\sum_{\lambda_{i}>0}\lambda_{i}+\sum_{\lambda_{i}<0}\lambda_{i}=0. (20)

Denote p,np,n the number of positive eigenvalues and the number of negative eigenvalues of ρσ\rho-\sigma, respectively.

Tr((ρσ)2)\displaystyle\operatorname{Tr}((\rho-\sigma)^{2}) =λi>0λi2+λi<0λi21p(λi>0λi)2+1n(λi<0λi)2=n+pnp(λi>0λi)2.\displaystyle=\sum_{\lambda_{i}>0}\lambda_{i}^{2}+\sum_{\lambda_{i}<0}\lambda_{i}^{2}\geq\frac{1}{p}\left(\sum_{\lambda_{i}>0}\lambda_{i}\right)^{2}+\frac{1}{n}\left(\sum_{\lambda_{i}<0}\lambda_{i}\right)^{2}=\frac{n+p}{np}\left(\sum_{\lambda_{i}>0}\lambda_{i}\right)^{2}. (21)

Combining Eq. (18) and Eq. (21), we have

Tr(P(ρσ))npn+pρσFn(rn)rρσF,\displaystyle\operatorname{Tr}(P(\rho-\sigma))\leq\sqrt{\frac{np}{n+p}}||\rho-\sigma||_{\rm F}\leq\sqrt{\frac{n(r-n)}{r}}||\rho-\sigma||_{\rm F}, (22)

since n+prn+p\leq r. Notice that Tr(M(ρσ))=2Tr(P(ρσ))\operatorname{Tr}(M(\rho-\sigma))=2\operatorname{Tr}(P(\rho-\sigma)) and nrank(σ)n\leq\operatorname{rank}(\sigma) as observed in Ref. [44], we finish the proof. ∎

Observation 7.

For a given set of dichotomic observables {Mi}\{M_{i}\} with outcome ±1\pm 1 and a mixed state ρ=kpkρk\rho=\sum_{k}p_{k}\rho_{k}, we have

|kpkMikMjkMiMj|R(τ0τ),\left|\sum_{k}p_{k}\braket{M_{i}}_{k}\braket{M_{j}}_{k}-\braket{M_{i}}\braket{M_{j}}\right|\leq R(\tau_{0}-\tau), (23)

where R=maxnn04n(rn)rR=\max_{n\leq n_{0}}\frac{4n(r-n)}{r}, r=rank(ρ)r=\operatorname{rank}(\rho), n0=maxkrank(ρk)rn_{0}=\max_{k}\operatorname{rank}(\rho_{k})\leq r, τ0\tau_{0} is the average purity, i.e, τ0=kpkTr(ρk2)\tau_{0}=\sum_{k}p_{k}\operatorname{Tr}(\rho_{k}^{2}).

Proof.
|kpkMikMjkMiMj|\displaystyle\left|\sum_{k}p_{k}\braket{M_{i}}_{k}\braket{M_{j}}_{k}-\braket{M_{i}}\braket{M_{j}}\right| =|kpk(MikMi)(MjkMj)|\displaystyle=\left|\sum_{k}p_{k}(\braket{M_{i}}_{k}-\braket{M_{i}})(\braket{M_{j}}_{k}-\braket{M_{j}})\right|
kpk|MikMi||MjkMj|\displaystyle\leq\sum_{k}p_{k}|{\braket{M_{i}}_{k}-\braket{M_{i}}}||{\braket{M_{j}}_{k}-\braket{M_{j}}}|
kpk(RρρkF)2\displaystyle\leq\sum_{k}p_{k}\left(\sqrt{R}\left\lVert\rho-\rho_{k}\right\rVert_{\rm F}\right)^{2}
=RkpkTr((ρρk)2)\displaystyle=R\sum_{k}p_{k}\operatorname{Tr}((\rho-\rho_{k})^{2})
=Rkpk(Tr(ρk2)+Tr(ρ2)2Tr(ρρk))\displaystyle=R\sum_{k}p_{k}(\operatorname{Tr}(\rho_{k}^{2})+\operatorname{Tr}(\rho^{2})-2\operatorname{Tr}(\rho\rho_{k}))
=R(τ0τ).\displaystyle=R(\tau_{0}-\tau).

Note that RrR\leq r and τ01\tau_{0}\leq 1. In the case that ρk\rho_{k}’s are all pure states, τ0=1\tau_{0}=1 and Rmin{4(11/r),r}R\leq\min\{4(1-1/r),r\}.

We have two remarks. Firstly, here we have made use of the rank rr and the quantifier of purity τ=Tr(ρ2)\tau=\operatorname{Tr}(\rho^{2}) to provide an upper bound. In principle, there could be other quantifiers of purity which can be employed in a tighter bound. The crucial point is how to get rid of the exact decomposition in the procedure of relaxation, since only the final state ρ\rho is assumed to be available. Secondly, another measure of purity is the single-shot distillable purity 𝒫d1(ρ)\mathcal{P}_{d}^{1}(\rho), which equals to log2(d/r)\lfloor\log_{2}(d/r)\rfloor [42]. Since the rank rr determines 𝒫d1(ρ)\mathcal{P}_{d}^{1}(\rho), but not the other way around. If we employ 𝒫d1(ρ)\mathcal{P}_{d}^{1}(\rho) instead of the rank rr, the results might be less accurate in principle. Hence, it is also a key point that how to chose and combine different measures of purity to extract more information.

Observation 8.

For a set of hermitian operators {Mi}\{M_{i}\}, a mixed state ρ=kpkρk\rho=\sum_{k}p_{k}\rho_{k},

Tr(Γp)l1r(τ0τ),\operatorname{Tr}(\Gamma_{p})\leq l_{1}r(\tau_{0}-\tau), (24)

where l1l_{1} is the maximal singular value of iMiMi\sum_{i}M_{i}\otimes M_{i}, r,τ,τ0r,\tau,\tau_{0} are the rank and purity of ρ\rho and the average purity of the decomposition, respectively.

Proof.
Tr(Γp)\displaystyle\operatorname{Tr}(\Gamma_{p}) =i(kpkMikMikMiMi)\displaystyle=\sum_{i}\left(\sum_{k}p_{k}\braket{M_{i}}_{k}\braket{M_{i}}_{k}-\braket{M_{i}}\braket{M_{i}}\right) (25)
=i(kpk(MikMi)2)\displaystyle=\sum_{i}\left(\sum_{k}p_{k}\left(\braket{M_{i}}_{k}-\braket{M_{i}}\right)^{2}\right) (26)
=Tr((iMiMi)(kpk(ρkρ)(ρkρ)))\displaystyle=\operatorname{Tr}\left(\left(\sum_{i}M_{i}\otimes M_{i}\right)\left(\sum_{k}p_{k}(\rho_{k}-\rho)\otimes(\rho_{k}-\rho)\right)\right) (27)
l1kpk(ρkρ)(ρkρ)1\displaystyle\leq l_{1}\left\lVert\sum_{k}p_{k}(\rho_{k}-\rho)\otimes(\rho_{k}-\rho)\right\rVert_{1} (28)
=2l1λi>0λi,\displaystyle=2l_{1}\sum_{\lambda_{i}>0}\lambda_{i}, (29)

where {λi}\{\lambda_{i}\} are eigenvalues of kpk(ρkρ)(ρkρ)\sum_{k}p_{k}(\rho_{k}-\rho)\otimes(\rho_{k}-\rho).

Note that,

rank(kpk(ρkρ)(ρkρ))r2.\operatorname{rank}\left(\sum_{k}p_{k}(\rho_{k}-\rho)\otimes(\rho_{k}-\rho)\right)\leq r^{2}. (30)

Following the similar procedure in Lemma 6, we know that

λi>0λir22kpk(ρkρ)(ρkρ)F,\sum_{\lambda_{i}>0}\lambda_{i}\leq\frac{\sqrt{r^{2}}}{2}\left\lVert\sum_{k}p_{k}(\rho_{k}-\rho)\otimes(\rho_{k}-\rho)\right\rVert_{F}, (31)

which leads to

Tr(Γp)\displaystyle\operatorname{Tr}(\Gamma_{p}) l1rkpk(ρkρ)(ρkρ)F\displaystyle\leq l_{1}r\left\lVert\sum_{k}p_{k}(\rho_{k}-\rho)\otimes(\rho_{k}-\rho)\right\rVert_{F} (32)
=l1r(k,tpkpt[Tr((ρkρ)(ρtρ))]2)1/2\displaystyle=l_{1}r\left(\sum_{k,t}p_{k}p_{t}[\operatorname{Tr}((\rho_{k}-\rho)(\rho_{t}-\rho))]^{2}\right)^{1/2} (33)
l1r(k,tpkptTr((ρkρ)2)Tr((ρtρ)2))1/2\displaystyle\leq l_{1}r\left(\sum_{k,t}p_{k}p_{t}\operatorname{Tr}((\rho_{k}-\rho)^{2})\operatorname{Tr}((\rho_{t}-\rho)^{2})\right)^{1/2} (34)
=l1rkpkTr((ρkρ)2)\displaystyle=l_{1}r\sum_{k}p_{k}\operatorname{Tr}((\rho_{k}-\rho)^{2}) (35)
=l1r(τ0τ).\displaystyle=l_{1}r(\tau_{0}-\tau). (36)

In the case that {Mi}\{M_{i}\} are all dichotomic measurements, l1l_{1} is no more than the size of {Mi}\{M_{i}\}. Hence, the bound in Eq. (24) is tighter than the one by trivially summing up the upper bound r(τ0τ)r(\tau_{0}-\tau) for each term in the diagonal.

In summary, we have proved the following observation. Notice that τ01\tau_{0}\leq 1.

Observation 9.

For a given set of dichotomic measurements {\cal M}, a state ρ\rho with rank rr and purity τ\tau,

maxΓcr(1τ),Tr(Γc)l1r(1τ),\max\Gamma^{c}\leq r(1-\tau),\ \operatorname{Tr}(\Gamma^{c})\leq l_{1}r(1-\tau), (37)

where l1l_{1} is the maximal singular value of MMM\sum_{M\in{\cal M}}M\otimes M.

Observation 10.
maxΓc21τ2,Tr(Γc)2l11τ2,\displaystyle\max\Gamma^{c}\leq 2\sqrt{1-\tau^{2}},\ \operatorname{Tr}(\Gamma^{c})\leq 2l_{1}\sqrt{1-\tau^{2}},

where l1l_{1} is the maximal singular value of iMiMi\sum_{i}M_{i}\otimes M_{i}.

Proof.

As we have observed,

Γijc=MiMjkpkMikMjk=Tr([MiMj][ρρkpkρkρk]),\displaystyle\Gamma^{c}_{ij}=\braket{M_{i}}\braket{M_{j}}-\sum_{k}p_{k}\braket{M_{i}}_{k}\braket{M_{j}}_{k}=\operatorname{Tr}\left([M_{i}\otimes M_{j}]\left[\rho\otimes\rho-\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}\right]\right), (38)
Tr(Γc)=Tr([iMiMi][ρρkpkρkρk]).\displaystyle\operatorname{Tr}(\Gamma^{c})=\operatorname{Tr}\left(\left[\sum_{i}M_{i}\otimes M_{i}\right]\left[\rho\otimes\rho-\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}\right]\right). (39)

Since the maximal singular values of MiMjM_{i}\otimes M_{j} is 11, Von Neumann’s trace inequality, and the relation between trace norm and fidelity imply that, ϵ[0,1)\forall\epsilon\in[0,1),

|Γijc|\displaystyle\left|\Gamma^{c}_{ij}\right| ρρkpkρkρkTr21f(ρρ,kpkρkρk)21τ2,\displaystyle\leq\left\lVert\rho\otimes\rho-\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}\right\rVert_{\operatorname{Tr}}\leq 2\sqrt{1-f\left(\rho\otimes\rho,\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}\right)}\leq 2\sqrt{1-\tau^{2}}, (40)

where ϵ[1/3,τ)\epsilon\in[1/3,\tau) and the last inequality is from the fact that

f(ρρ,kpkρkρk)\displaystyle f(\rho\otimes\rho,\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}) =[Trρρ(kpkρkρk)ρρ]2\displaystyle=\left[\operatorname{Tr}\sqrt{\sqrt{\rho\otimes\rho}\left(\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}\right)\sqrt{\rho\otimes\rho}}\right]^{2} (41)
Tr(ρρ(kpkρkρk)ρρ)\displaystyle\geq\operatorname{Tr}\left(\sqrt{\rho\otimes\rho}\left(\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}\right)\sqrt{\rho\otimes\rho}\right) (42)
Tr((ρρ)(kpkρkρk))\displaystyle\geq\operatorname{Tr}\left(\left(\rho\otimes\rho\right)\left(\sum_{k}p_{k}\rho_{k}\otimes\rho_{k}\right)\right) (43)
(kpkTr(ρρk))2=τ2.\displaystyle\geq\left(\sum_{k}p_{k}\operatorname{Tr}(\rho\rho_{k})\right)^{2}=\tau^{2}. (44)

Similarly, we can proof the result for Tr(Γc)\operatorname{Tr}(\Gamma^{c}). ∎

We have two extra remarks. Firstly, for a given mixed state ρ=kpkρk\rho=\sum_{k}p_{k}\rho_{k} whose purity is τ\tau, we have

1τ=1Tr(ρ2)kpkρρkF2.\displaystyle 1-\tau=1-\operatorname{Tr}(\rho^{2})\geq\sum_{k}p_{k}\left\lVert\rho-\rho_{k}\right\rVert_{\rm F}^{2}. (45)

Hence, there is a kk such that ρρkF1τ\left\lVert\rho-\rho_{k}\right\rVert_{\rm F}\leq\sqrt{1-\tau}.

Secondly, Von Neumann’s trace inequality and the relation between trace distance and fidelity imply that

Tr(M(ρσ))ρσTr21f(ρ,σ).\operatorname{Tr}(M(\rho-\sigma))\leq\left\lVert\rho-\sigma\right\rVert_{\operatorname{Tr}}\leq 2\sqrt{1-f(\rho,\sigma)}. (46)

Besides, τ=Tr(ρ2)kpkf(ρ,ρk)\tau=\operatorname{Tr}(\rho^{2})\leq\sum_{k}p_{k}f(\rho,\rho_{k}) implies that there exist a kk^{\prime} such that f(ρ,ρk)τf(\rho,\rho_{k^{\prime}})\geq\tau. Consequently, |Tr(M(ρρk))|2(1τ)|\operatorname{Tr}(M(\rho-\rho_{k^{\prime}}))|\leq 2\sqrt{(1-\tau)}.

III C. Covariance inequalities

For a given covariance matrix Υ\Upsilon whose rows and columns are divided into kk blocks, we have

i,j=1k|Υij|\displaystyle\sum_{i,j=1}^{k}|{\Upsilon_{ij}}| i,j=1k|Υii||Υjj|=(i=1k|Υii|)2ki=1k|Υii|=kTr(Υ).\displaystyle\leq\sum_{i,j=1}^{k}\sqrt{|{\Upsilon_{ii}}||{\Upsilon_{jj}}|}=\left(\sum_{i=1}^{k}\sqrt{|{\Upsilon_{ii}}|}\right)^{2}\leq k\sum_{i=1}^{k}|{\Upsilon_{ii}}|=k\operatorname{Tr}(\Upsilon). (47)

For a network G(V,E)G(V,E), where VV is the set of nodes or receivers, E={e}E=\{e\} is the set of sources, denote Cij={ee(i,j)}C_{ij}=\{e\mid e\supseteq(i,j)\}, cijc_{ij} the size of CijC_{ij}. For a given state ρ𝒮C\rho\in\mathcal{S}_{\rm C}, from the covariance matrix decomposition, we know that eCijΥe,ij=ΓijΓijc\sum_{e\in C_{ij}}\Upsilon_{e,ij}=\Gamma_{ij}-\Gamma^{c}_{ij}.

i,j|Γij|\displaystyle\sum_{i,j}|{\Gamma_{ij}}| i,j(e|Υe,ij|+|Γijc|)ekeTr(Υe)+nTr(Γc),\displaystyle\leq\sum_{i,j}\left(\sum_{e}|{\Upsilon_{e,ij}}|+|{\Gamma^{c}_{ij}}|\right)\leq\sum_{e}k_{e}\operatorname{Tr}(\Upsilon_{e})+n\operatorname{Tr}(\Gamma^{c}), (48)

where kek_{e} is the size of the source ee. In the last inequality, we have applied the inequality in Eq. (47) for both of Υe,ij\Upsilon_{e,ij} and Γijc\Gamma^{c}_{ij}.

Denote k=maxekek=\max_{e}k_{e}, we have

i,j|Γij|\displaystyle\sum_{i,j}|{\Gamma_{ij}}| keTr(Υe)+nTr(Γc)=kTr(Γ)+(nk)Tr(Γc).\displaystyle\leq k\sum_{e}\operatorname{Tr}(\Upsilon_{e})+n\operatorname{Tr}(\Gamma^{c})=k\operatorname{Tr}(\Gamma)+(n-k)\operatorname{Tr}(\Gamma^{c}). (49)

This leads to Corollary 1 in the main text.

In the case of an IQN with only bipartite sources and at most c3c_{3} tripartite sources, Γc=0\Gamma^{c}=0. Similarly, we have

i,j|Γij|2Tr(Γ)+e,ke=3Tr(Υe)2Tr(Γ)+3mc3,\sum_{i,j}|{\Gamma_{ij}}|\leq 2\operatorname{Tr}(\Gamma)+\sum_{e,k_{e}=3}\operatorname{Tr}(\Upsilon_{e})\leq 2\operatorname{Tr}(\Gamma)+3mc_{3}, (50)

where mm is the maximal number of measurements per party. Here we have made use of the inequality Tr(Υe)kem\operatorname{Tr}(\Upsilon_{e})\leq k_{e}m, since the covariance of the random variable in [1,1][-1,1] is no more than 11.

For any state ρ=kpkρk\rho=\sum_{k}p_{k}\rho_{k}, where ρk\rho_{k} is from an IQN with only bipartite sources and at most c3c_{3} tripartite sources, we have

i,j|Γij|\displaystyle\sum_{i,j}|{\Gamma_{ij}}| =i,j|kpkΓij(k)+Γijc|\displaystyle=\sum_{i,j}\Big{|}{\sum_{k}p_{k}\Gamma^{(k)}_{ij}+\Gamma^{c}_{ij}}\Big{|} (51)
kpki,j|Γij(k)|+i,j|Γijc|\displaystyle\leq\sum_{k}p_{k}\sum_{i,j}|{\Gamma^{(k)}_{ij}}|+\sum_{i,j}|{\Gamma^{c}_{ij}}| (52)
kpk(2Tr(Γ(k))+3mc3)+nTr(Γc)\displaystyle\leq\sum_{k}p_{k}(2\operatorname{Tr}(\Gamma^{(k)})+3mc_{3})+n\operatorname{Tr}(\Gamma^{c}) (53)
=2Tr(Γ)+(n2)Tr(Γc)+3mc3.\displaystyle=2\operatorname{Tr}(\Gamma)+(n-2)\operatorname{Tr}(\Gamma^{c})+3mc_{3}. (54)

Note that, ρk\rho_{k}’s might be from different networks with different topologies, the only constraint is that there are only bipartite sources and at most c3c_{3} tripartite sources.

In the general case,

i,j|Γij(k)|ekeTr(Υe(k)),\sum_{i,j}|{\Gamma^{(k)}_{ij}}|\leq\sum_{e}k_{e}\operatorname{Tr}(\Upsilon_{e}^{(k)}), (55)

which leads to

i,j|Γij|\displaystyle\sum_{i,j}|{\Gamma_{ij}}| kpkekeTr(Υe(k))+nTr(Γijc)\displaystyle\leq\sum_{k}p_{k}\sum_{e}k_{e}\operatorname{Tr}(\Upsilon_{e}^{(k)})+n\operatorname{Tr}(\Gamma^{c}_{ij})
=ttkpkeEt(k)Tr(Υe(k))+nTr(Γijc)\displaystyle=\sum_{t}t\sum_{k}p_{k}\sum_{e\in E_{t}^{(k)}}\operatorname{Tr}(\Upsilon_{e}^{(k)})+n\operatorname{Tr}(\Gamma^{c}_{ij})
=ttxt+ny,\displaystyle=\sum_{t}tx_{t}+ny, (56)

where xt:=kpkeEt(k)Tr(Υe(k))x_{t}:=\sum_{k}p_{k}\sum_{e\in E_{t}^{(k)}}\operatorname{Tr}(\Upsilon_{e}^{(k)}), and y:=Tr(Γijc)y:=\operatorname{Tr}(\Gamma^{c}_{ij}).

By definition, we have txt+y=Tr(Γ)\sum_{t}x_{t}+y=\operatorname{Tr}(\Gamma). Notice that

0xt\displaystyle 0\leq x_{t} kpkeEt(k)mt=kpkct(k)mt=ctmt,\displaystyle\leq\sum_{k}p_{k}\sum_{e\in E_{t}^{(k)}}mt=\sum_{k}p_{k}c_{t}^{(k)}mt=c_{t}mt, (57)

with ct=kpkct(k)c_{t}=\sum_{k}p_{k}c_{t}^{(k)} to be the average number of genuine kk-partite sources.

IV D. Sub-networks

For a given network G(V,E)G(V,E), a network state ρ\rho, and a subset SS of VV, denote ρS\rho_{S} the reduced state of ρ\rho on SS. By definition, the state ρ\rho can be decomposed as

ρ=kpkρk,ρk=(iV𝒞i(k))(eEηe(k)),\displaystyle\rho=\sum\nolimits_{k}p_{k}\rho_{k},\ \rho_{k}=\Big{(}\bigotimes\nolimits_{i\in V}\mathcal{C}_{i}^{(k)}\Big{)}\Big{(}\bigotimes\nolimits_{e\in E}\eta_{e}^{(k)}\Big{)}, (58)

where {pk}k\{p_{k}\}_{k} with kpk=1\sum_{k}p_{k}=1 and pk>0p_{k}>0 is the global classical correlation, 𝒞i(k)\mathcal{C}_{i}^{(k)} is a local channel for the ii-th party, ηe(k)\eta_{e}^{(k)} is an entangled state distributed from the source labeled by the hyperedge ee.

Firstly, the decomposition ρ=kpkρk\rho=\sum_{k}p_{k}\rho_{k} leads to the decomposition ρS=kpkρS,k\rho_{S}=\sum_{k}p_{k}\rho_{S,k} with ρS,k\rho_{S,k} to be the corresponding reduced state of ρk\rho_{k}, and ρk\rho_{k} is an independent network state of the original network implies that ρS,k\rho_{S,k} is also an independent network state of the sub-network, by definition of the state from correlated quantum networks. Secondly, Tr(MρS,k)=Tr(Mρk)\operatorname{Tr}(M\rho_{S,k})=\operatorname{Tr}(M\rho_{k}) if MM acts only nontrivially on the subset SS. Then the definition of the classical covariance matrices implies that ΓS,ij(c)=Γij(c)\Gamma^{(c)}_{S,ij}=\Gamma^{(c)}_{ij}, and ΓS(c)\Gamma^{(c)}_{S} inherits all the constraints for Γ(c)\Gamma^{(c)}. To be more explicitly,

ΓS,ij(c)\displaystyle\Gamma^{(c)}_{S,ij} =kpkMiS,kMjS,kMiSMiS=kpkMikMjkMiMi=Γij(c).\displaystyle=\sum_{k}p_{k}\langle M_{i}\rangle_{S,k}\langle M_{j}\rangle_{S,k}-\langle M_{i}\rangle_{S}\langle M_{i}\rangle_{S}=\sum_{k}p_{k}\langle M_{i}\rangle_{k}\langle M_{j}\rangle_{k}-\langle M_{i}\rangle\langle M_{i}\rangle=\Gamma^{(c)}_{ij}. (59)

References