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The European Physical Journal Plus

Zero-correlation entanglement vs. Schmidt rank

Andrei Tănăsescu, Adriana Balan, Pantelimon George Popescu

Published May 1, 2021• 0 citations
Publisher
DOI
10.1140/epjp/s13360-021-01468-y

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Tail-Resolved Schmidt-Rank Width of Weighted Phase Networks: Noncommuting Activation Limits, Gauge-Stable Perturbations, and Approximate Tree Complexity

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This work develops a finite-resolution counterpart of Schmidt-rank width for weighted phase networks and uses it to distinguish algebraic Schmidt-rank activation from spectrally resolved entanglement complexity. For a bipartition $A|A^c$ with Schmidt coefficients $s_1 \ge s_2 \ge \cdots$, define the discarded Schmidt-tail mass $$\tau_r^A(\psi)=\left(\sum_{j>r}s_j^2\right)^{1/2},$$ and the corresponding $\epsilon$-resolved Schmidt rank $$R_\epsilon^A(\psi)=\min\left\{r:\tau_r^A(\psi)\le\epsilon\right\}.$$ The global tail-resolved Schmidt-rank width is then $$\chi_{\mathrm{res}}^{(\epsilon)}(\psi)=\min_T\max_{e\in E(T)}\log_2R_\epsilon^{A_e}(\psi),$$ where $T$ ranges over subcubic decomposition trees and $A_e|A_e^c$ is the bipartition induced by deleting the tree edge $e$. At zero resolution, $\epsilon=0$, this quantity reduces to ordinary Schmidt-rank width. For graph states, the flat cut Schmidt spectrum gives an exact calibration: $$\chi_{\mathrm{res}}^{(\epsilon)}(|G\rangle)=\log_2\left\lceil(1-\epsilon^2)\,2^{\operatorname{rw}(G)}\right\rceil,\qquad0\le\epsilon<1,$$ where $\operatorname{rw}(G)$ is the graph rank-width. Consequently, graph families with linear rank-width retain linear tail-resolved Schmidt-rank width at every fixed finite resolution $\epsilon<1$. The paper next establishes a gauge-stable perturbation theory. After optimization over cut-local diagonal phases, Schmidt truncation tails satisfy the Lipschitz estimate $$\left|\tau_r^A(\psi)-\tau_r^A(\phi)\right|\led_{\mathrm{diag}}^A(\psi,\phi),$$ which yields a global resolution-shift sandwich for $\chi_{\mathrm{res}}^{(\epsilon)}$. For balanced pairwise weighted phase networks with crossing phase errors $\eta_e$, $$d_{\mathrm{diag}}^A\le\frac14\left\|\eta_{E(A,A^c)}\right\|_2.$$ If a fixed coupling template $W$ is implemented with coupling error $\Delta W$ and timing error $\Delta t$, then $$\eta=t\,\Delta W+\Delta t\,W+\Delta t\,\Delta W,$$ giving an explicit certificate that converts finite calibration and timing uncertainty into a guaranteed resolved-width bound. The tail-resolved width also controls approximate subcubic tree-tensor-network complexity. If $D_{\mathrm{TTN}}^{(\epsilon)}$ denotes the minimum possible maximal bond dimension of a subcubic TTN approximating the state within Hilbert-space norm error $\epsilon$, then $$2^{\chi_{\mathrm{res}}^{(\epsilon)}}\leD_{\mathrm{TTN}}^{(\epsilon)}\le2^{\chi_{\mathrm{res}}^{\left(\epsilon/\sqrt{2n-3}\right)}}.$$ The central application concerns the Clifford point of the complete weighted phase network. Consider $$|\Psi_V(\lambda)\rangle=\exp\left[i\sum_e\left(\pi+\lambda V_e\right)n_u n_v\right]|+\rangle^{\otimes n}.$$ For every fixed resolution $$0<\epsilon<\frac{1}{\sqrt{2}},$$ the tail-resolved width remains equal to $1$ for all sufficiently small $|\lambda|$, independently of the perturbation direction $V$. In contrast, at exact zero resolution an arbitrarily small generic nonuniform perturbation activates the maximal complete-support Schmidt-rank width $$\left\lceil\frac{n}{3}\right\rceil,$$ whereas a uniform perturbation activates only $$\log_2\left(\left\lceil\frac{n}{3}\right\rceil+1\right).$$ Thus the zero-resolution and zero-perturbation limits do not commute. For an open, dense, full-measure class of nonuniform perturbation directions, $$\lim_{\epsilon\downarrow0}\lim_{\lambda\to0}\chi_{\mathrm{res}}^{(\epsilon)}=1,$$ while $$\lim_{\lambda\to0,\ \lambda\neq0}\lim_{\epsilon\downarrow0}\chi_{\mathrm{res}}^{(\epsilon)}=\left\lceil\frac{n}{3}\right\rceil.$$ This establishes a sharp distinction between algebraic Schmidt activation and finite-resolution activation: infinitesimal symmetry breaking can create maximal exact Schmidt-rank width while remaining invisible at any fixed finite spectral resolution sufficiently close to the Clifford point. The results connect weighted phase and fixed $ZZ$/Ising networks, graph width parameters, Schmidt-spectrum stability, and approximate tensor-network complexity. The global phase-error certificate is intentionally conservative: it does not by itself establish thermodynamic robustness against a size-independent coherent error on every edge.

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Mutually unbiased bases containing a complex Hadamard matrix of Schmidt rank three

Mengyao Hu, Lin Chen, Yize Sun

Constructing four six-dimensional mutually unbiased bases (MUBs) is an open problem in quantum physics and measurement. We investigate the existence of four MUBs including the identity, and a complex Hadamard matrix (CHM) of Schmidt rank three. The CHM is equivalent to a controlled unitary operation on the qubit-qutrit system via local unitary transformation I 2 ⊗ V and I 2 ⊗ W . We show that V and W have no zero entry, and apply it to exclude constructed examples as members of MUBs. We further show that the maximum of entangling power of controlled unitary operation is log 2 3 ebits. We derive the condition under which the maximum is achieved, and construct concrete examples. Our results describe the phenomenon that if a CHM of Schmidt rank three belongs to an MUB then its entangling power may not reach the maximum.

arXiv:1910.05515•Proceedings of the Royal Society A Mathematical Physical and Engineering Sciences•Mar 1, 2020•0 citations
This work develops a finite-resolution counterpart of Schmidt-rank width for weighted phase networks and uses it to distinguish algebraic Schmidt-rank activation from spectrally resolved entanglement complexity. For a bipartition A∣AcA|A^cA∣Ac with Schmidt coefficients s1≥s2≥⋯s_1 \ge s_2 \ge \cdotss1​≥s2​≥⋯, define the discarded Schmidt-tail mass τrA(ψ)=(∑j>rsj2)1/2,\tau_r^A(\psi)=\left(\sum_{j>r}s_j^2\right)^{1/2},τrA​(ψ)=(∑j>r​sj2​)1/2, and the corresponding ϵ\epsilonϵ-resolved Schmidt rank RϵA(ψ)=min⁡{r:τrA(ψ)≤ϵ}.R_\epsilon^A(\psi)=\min\left\{r:\tau_r^A(\psi)\le\epsilon\right\}.RϵA​(ψ)=min{r:τrA​(ψ)≤ϵ}. The global tail-resolved Schmidt-rank width is then χres(ϵ)(ψ)=min⁡Tmax⁡e∈E(T)log⁡2RϵAe(ψ),\chi_{\mathrm{res}}^{(\epsilon)}(\psi)=\min_T\max_{e\in E(T)}\log_2R_\epsilon^{A_e}(\psi),χres(ϵ)​(ψ)=minT​maxe∈E(T)​log2​RϵAe​​(ψ), where TTT ranges over subcubic decomposition trees and Ae∣AecA_e|A_e^cAe​∣Aec​ is the bipartition induced by deleting the tree edge eee. At zero resolution, ϵ=0\epsilon=0ϵ=0, this quantity reduces to ordinary Schmidt-rank width. For graph states, the flat cut Schmidt spectrum gives an exact calibration: χres(ϵ)(∣G⟩)=log⁡2⌈(1−ϵ2) 2rw⁡(G)⌉,0≤ϵ<1,\chi_{\mathrm{res}}^{(\epsilon)}(|G\rangle)=\log_2\left\lceil(1-\epsilon^2)\,2^{\operatorname{rw}(G)}\right\rceil,\qquad0\le\epsilon<1,χres(ϵ)​(∣G⟩)=log2​⌈(1−ϵ2)2rw(G)⌉,0≤ϵ<1, where rw⁡(G)\operatorname{rw}(G)rw(G) is the graph rank-width. Consequently, graph families with linear rank-width retain linear tail-resolved Schmidt-rank width at every fixed finite resolution ϵ<1\epsilon<1ϵ<1. The paper next establishes a gauge-stable perturbation theory. After optimization over cut-local diagonal phases, Schmidt truncation tails satisfy the Lipschitz estimate $$\left|\tau_r^A(\psi)-\tau_r^A(\phi)\right|\led_{\mathrm{diag}}^A(\psi,\phi),$$ which yields a global resolution-shift sandwich for χres(ϵ)\chi_{\mathrm{res}}^{(\epsilon)}χres(ϵ)​. For balanced pairwise weighted phase networks with crossing phase errors ηe\eta_eηe​, ddiagA≤14∥ηE(A,Ac)∥2.d_{\mathrm{diag}}^A\le\frac14\left\|\eta_{E(A,A^c)}\right\|_2.ddiagA​≤41​​ηE(A,Ac)​​2​. If a fixed coupling template WWW is implemented with coupling error ΔW\Delta WΔW and timing error Δt\Delta tΔt, then η=t ΔW+Δt W+Δt ΔW,\eta=t\,\Delta W+\Delta t\,W+\Delta t\,\Delta W,η=tΔW+ΔtW+ΔtΔW, giving an explicit certificate that converts finite calibration and timing uncertainty into a guaranteed resolved-width bound. The tail-resolved width also controls approximate subcubic tree-tensor-network complexity. If DTTN(ϵ)D_{\mathrm{TTN}}^{(\epsilon)}DTTN(ϵ)​ denotes the minimum possible maximal bond dimension of a subcubic TTN approximating the state within Hilbert-space norm error ϵ\epsilonϵ, then $$2^{\chi_{\mathrm{res}}^{(\epsilon)}}\leD_{\mathrm{TTN}}^{(\epsilon)}\le2^{\chi_{\mathrm{res}}^{\left(\epsilon/\sqrt{2n-3}\right)}}.$$ The central application concerns the Clifford point of the complete weighted phase network. Consider ∣ΨV(λ)⟩=exp⁡[i∑e(π+λVe)nunv]∣+⟩⊗n.|\Psi_V(\lambda)\rangle=\exp\left[i\sum_e\left(\pi+\lambda V_e\right)n_u n_v\right]|+\rangle^{\otimes n}.∣ΨV​(λ)⟩=exp[i∑e​(π+λVe​)nu​nv​]∣+⟩⊗n. For every fixed resolution 0<ϵ<12,0<\epsilon<\frac{1}{\sqrt{2}},0<ϵ<2​1​, the tail-resolved width remains equal to 111 for all sufficiently small ∣λ∣|\lambda|∣λ∣, independently of the perturbation direction VVV. In contrast, at exact zero resolution an arbitrarily small generic nonuniform perturbation activates the maximal complete-support Schmidt-rank width ⌈n3⌉,\left\lceil\frac{n}{3}\right\rceil,⌈3n​⌉, whereas a uniform perturbation activates only log⁡2(⌈n3⌉+1).\log_2\left(\left\lceil\frac{n}{3}\right\rceil+1\right).log2​(⌈3n​⌉+1). Thus the zero-resolution and zero-perturbation limits do not commute. For an open, dense, full-measure class of nonuniform perturbation directions, lim⁡ϵ↓0lim⁡λ→0χres(ϵ)=1,\lim_{\epsilon\downarrow0}\lim_{\lambda\to0}\chi_{\mathrm{res}}^{(\epsilon)}=1,limϵ↓0​limλ→0​χres(ϵ)​=1, while lim⁡λ→0, λ≠0lim⁡ϵ↓0χres(ϵ)=⌈n3⌉.\lim_{\lambda\to0,\ \lambda\neq0}\lim_{\epsilon\downarrow0}\chi_{\mathrm{res}}^{(\epsilon)}=\left\lceil\frac{n}{3}\right\rceil.limλ→0, λ=0​limϵ↓0​χres(ϵ)​=⌈3n​⌉. This establishes a sharp distinction between algebraic Schmidt activation and finite-resolution activation: infinitesimal symmetry breaking can create maximal exact Schmidt-rank width while remaining invisible at any fixed finite spectral resolution sufficiently close to the Clifford point. The results connect weighted phase and fixed ZZZZZZ/Ising networks, graph width parameters, Schmidt-spectrum stability, and approximate tensor-network complexity. The global phase-error certificate is intentionally conservative: it does not by itself establish thermodynamic robustness against a size-independent coherent error on every edge.
Constructing four six-dimensional mutually unbiased bases (MUBs) is an open problem in quantum physics and measurement. We investigate the existence of four MUBs including the identity, and a complex Hadamard matrix (CHM) of Schmidt rank three. The CHM is equivalent to a controlled unitary operation on the qubit-qutrit system via local unitary transformation I 2 ⊗ V and I 2 ⊗ W . We show that V and W have no zero entry, and apply it to exclude constructed examples as members of MUBs. We further show that the maximum of entangling power of controlled unitary operation is log 2 3 ebits. We derive the condition under which the maximum is achieved, and construct concrete examples. Our results describe the phenomenon that if a CHM of Schmidt rank three belongs to an MUB then its entangling power may not reach the maximum.