Logarithmic growth of peripheral entanglement concentrated via noisy measurements in a star network of spins
Pith reviewed 2026-05-24 07:31 UTC · model grok-4.3
The pith
In a star network of spins with XYZ Heisenberg interactions, localizable bipartite peripheral entanglement grows logarithmically with periphery size when xy-anisotropy vanishes.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
In the large-periphery limit of an XYZ Heisenberg star network, the localizable bipartite peripheral entanglement obtained by projective or unsharp measurements on the central qubit grows as the logarithm of the number of peripheral qubits when the xy-anisotropy parameter is zero; this logarithmic growth persists for arbitrary noise strength in the unsharp-measurement description.
What carries the argument
Localizable bipartite peripheral entanglement (LBPE) concentrated by measurements performed solely on the central qubit of the star network.
If this is right
- In the large-periphery limit the logarithmic growth remains for any strength of unsharp measurement noise.
- Nonzero xy-anisotropy suppresses the logarithmic scaling unless a local magnetic field is applied to the central qubit.
- In the large-center and competing-center limits the peripheral entanglement no longer exhibits logarithmic growth with periphery size.
- Partial-trace entanglement between periphery qubits behaves like LBPE only in the large-periphery limit.
Where Pith is reading between the lines
- If the logarithmic scaling survives in real devices, star networks could serve as scalable entanglement concentrators without requiring direct control over every peripheral qubit.
- The anisotropy dependence suggests that small symmetry-breaking terms could be used as a diagnostic for whether a fabricated network has reached the large-periphery regime.
- The persistence under unsharp measurements indicates that the effect may be observable even when the central qubit suffers significant decoherence during readout.
Load-bearing premise
The interactions must be exactly of XYZ Heisenberg form between center and periphery, and entanglement must be localized exclusively by measurements on the central qubit.
What would settle it
Calculate the localizable entanglement for a star network with twenty or more peripheral qubits at zero xy-anisotropy; the value should increase by roughly ln(2) each time the periphery size doubles.
Figures
read the original abstract
In a star-network of qubits interacting via Heisenberg interaction of XYZ-type, we demonstrate a logarithmic growth of the localizable bipartite peripheral entanglement with increasing periphery-size and vanishing xy-anisotropy. This feature disappears when xy-anisotropy becomes non-zero, exhibiting an anisotropy effect, which can be negated by taking the system out of equilibrium by a qubit-local magnetic field. In the large-center and the competing-center limits of the model, the behaviour of LBPE is qualitatively different from that of the large-periphery limit. Also, the bipartite peripheral entanglement computed via a partial trace-based approach behaves qualitatively similarly to the LBPE in the large periphery limit, while in the other two limits, it behaves differently. We further consider the generalized description of localizable entanglement using unsharp measurements, and demonstrate that the logarithmic growth of LBPE is present for all noise strengths in the large-periphery limit, while in the competing-center limit, it does not.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper studies localizable bipartite peripheral entanglement (LBPE) in a star network of qubits coupled by XYZ Heisenberg interactions. It reports that LBPE grows logarithmically with periphery size N in the large-periphery limit when the xy-anisotropy vanishes; this scaling persists for all noise strengths when localizable entanglement is defined via unsharp measurements. The scaling is absent for nonzero anisotropy (unless a local magnetic field is applied) and the behavior differs qualitatively in the large-center and competing-center limits. Partial-trace entanglement is compared to LBPE across these regimes.
Significance. A robust logarithmic scaling of LBPE under arbitrary noise would be of interest for entanglement concentration protocols in noisy quantum networks. The generalization from projective to unsharp measurements and the contrast across the three scaling limits are the main technical contributions. The result is currently limited by its reliance on finite-N numerics without an analytical large-N derivation.
major comments (2)
- [Large-periphery limit (results and discussion of LBPE scaling)] Large-periphery limit: the central claim that LBPE(N) ~ log(N) as N→∞ (for vanishing xy-anisotropy and all noise strengths) rests on numerical observations for finite N. No analytical derivation, exact diagonalization in the thermodynamic limit, or closed-form expression for the optimized measurement is provided to confirm that the growth does not saturate or cross over due to sub-leading corrections.
- [Unsharp measurements and noise analysis] Unsharp-measurement generalization: the statement that logarithmic growth survives for all noise strengths in the large-periphery limit inherits the same finite-size extrapolation issue; the manuscript does not supply an analytic argument showing that the unsharp-measurement optimization preserves the scaling when N→∞.
minor comments (2)
- [Model definition] Notation for the three limits (large-periphery, large-center, competing-center) should be defined once with explicit parameter regimes rather than introduced piecemeal.
- [Numerical results figures] Figure captions for the LBPE vs. N plots should explicitly state the range of N used and whether error bars or fitting uncertainties are shown.
Simulated Author's Rebuttal
We thank the referee for their careful reading and constructive comments. We appreciate the recognition of the potential interest in robust logarithmic scaling of LBPE. We address the major comments below, noting that our results rely on finite-N numerics.
read point-by-point responses
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Referee: Large-periphery limit: the central claim that LBPE(N) ~ log(N) as N→∞ (for vanishing xy-anisotropy and all noise strengths) rests on numerical observations for finite N. No analytical derivation, exact diagonalization in the thermodynamic limit, or closed-form expression for the optimized measurement is provided to confirm that the growth does not saturate or cross over due to sub-leading corrections.
Authors: We agree that the logarithmic scaling claim is based on numerical observations for finite N and that no analytical derivation, exact diagonalization in the thermodynamic limit, or closed-form expression is provided. The manuscript shows consistent log(N) growth across accessible system sizes with no saturation observed. We will revise the discussion to include more details on the finite-size scaling fits, the maximum N reached, and an explicit statement on the absence of an analytic large-N proof. revision: partial
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Referee: Unsharp-measurement generalization: the statement that logarithmic growth survives for all noise strengths in the large-periphery limit inherits the same finite-size extrapolation issue; the manuscript does not supply an analytic argument showing that the unsharp-measurement optimization preserves the scaling when N→∞.
Authors: The unsharp-measurement results are likewise obtained from finite-N numerical optimization over measurement strength for each noise level. No analytic argument for preservation of the scaling at infinite N is supplied. We will revise the relevant section to emphasize the numerical character of the observation and to note the extrapolation limitation explicitly. revision: partial
- Analytical derivation confirming logarithmic growth of LBPE (projective or unsharp) in the thermodynamic limit
Circularity Check
No circularity: logarithmic scaling is a numerical observation from the model, not a tautological reduction
full rationale
The paper defines the star-network Hamiltonian with XYZ Heisenberg interactions and localizable bipartite peripheral entanglement (LBPE) via projective/unsharp measurements on the central spin. The claimed log(N) growth in the large-periphery limit (vanishing xy-anisotropy, any noise) is presented as an observed feature from finite-N computations, not derived by fitting a parameter that is then renamed as a prediction or by self-referential definition. No load-bearing step reduces to a self-citation chain, ansatz smuggled via prior work, or uniqueness theorem from the same authors. The distinction between large-periphery, large-center, and competing-center regimes is model-dependent but does not create circularity. The result is self-contained against external benchmarks (exact diagonalization or measurement optimization on the given Hamiltonian) and does not equate the output to its inputs by construction.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption The system is governed by the XYZ Heisenberg interaction on a star geometry.
- domain assumption Localizable bipartite peripheral entanglement is defined via measurements on the central qubit.
Reference graph
Works this paper leans on
-
[1]
We group the basis states according to Eq
np = 2 We first consider the case of Jp = 1 (mp = −1, 0, 1) among the allowed values Jp = 0, 1 for np = 2. We group the basis states according to Eq. (24) as {|−1/2⟩ |−1⟩ , |1/2⟩ |0⟩ , |−1/2⟩ |1⟩} and {|1/2⟩ |−1⟩ , |−1/2⟩ |0⟩ , |1/2⟩ |1⟩} 10 respectively, leading to the H1 block having the form (23), with A1 and A2 being two 3 × 3 matrices given by A1 = 1...
-
[2]
∆ 2 γα+ − 1 2 γα− 1 2 ∆ 2 # , A2 = 1 2
np = 3 In this case, Jp = 3 /2, 1/2, 1/2, and we start with the block Hs(Jp = 3/2), where grouping the basis as {|−1/2⟩ |3/2⟩ , |1/2⟩ |1/2⟩ , |−1/2⟩ |−1/2⟩ , |1/2⟩ |−3/2⟩} and {|1/2⟩ |3/2⟩ , |−1/2⟩ |1/2⟩ , |1/2⟩ |−1/2⟩ , |−1/2⟩ |−3/2⟩} makes H3/2 of the form (23) with the 4 × 4 matrices A1 and A2 given by A1 = 1 2 3∆ 2 0 γα+ 1 2 0 0 − ∆ 2 α− 1 2 γ...
-
[3]
R. Horodecki, P. Horodecki, M. Horodecki, and K. Horodecki, Rev. Mod. Phys.81, 865 (2009); O. G¨uhne and G. T´oth, Phys. Rep. 474, 1 (2009)
work page 2009
-
[4]
C. H. Bennett and S. J. Wiesner, Phys. Rev. Lett. 69, 2881 (1992); C. H. Bennett, G. Brassard, C. Cr ´epeau, R. Jozsa, A. Peres, and W. K. Wootters, Phys. Rev. Lett. 70, 1895 (1993); K. Mattle, H. Weinfurter, P. G. Kwiat, and A. Zeilinger, Phys. Rev. Lett. 76, 4656 (1996); D. Bouwmeester, J.-W. Pan, K. Mattle, M. Eibl, H. Weinfurter, and A. Zeilinger, Nat...
work page 1992
-
[5]
A. K. Ekert, Phys. Rev. Lett. 67, 661 (1991); T. Jennewein, C. Simon, G. Weihs, H. Weinfurter, and A. Zeilinger, Phys. Rev. Lett. 84, 4729 (2000); J. Yin, Y .-H. Li, S.-K. Liao, M. Yang, Y . Cao, L. Zhang, J.-G. Ren, W.-Q. Cai, W.-Y . Liu, S.-L. Li, R. Shu, Y .-M. Huang, L. Deng, L. Li, Q. Zhang, N.-L. Liu, Y .-A. Chen, C.-Y . Lu, X.-B. Wang, F. Xu, J.-Y ...
work page 1991
-
[6]
M. Dalmonte, B. Vermersch, and P. Zoller, Nature Physics14, 827 (2018); C. Kokail, R. van Bijnen, A. Elben, B. Vermersch, and P. Zoller, Nature Physics17, 936 (2021)
work page 2018
-
[7]
M. F. Riedel, P. B ¨ohi, Y . Li, T. W. H ¨ansch, A. Sinatra, and P. Treutlein, Nature 464, 1170 (2010); J. Joo, W. J. Munro, and T. P. Spiller, Phys. Rev. Lett.107, 083601 (2011); R. Demkowicz-Dobrza´nski and L. Maccone, Phys. Rev. Lett. 113, 250801 (2014)
work page 2010
-
[8]
R. Raussendorf and H. J. Briegel, Phys. Rev. Lett. 86, 5188 (2001); H. J. Briegel, D. E. Browne, W. D ¨ur, R. Raussendorf, and M. Van den Nest, Nat. Phys. 5, 19 (2009)
work page 2001
- [9]
- [10]
-
[11]
D. Leibfried, R. Blatt, C. Monroe, and D. Wineland, Rev. Mod. Phys. 75, 281 (2003); D. Porras and J. I. Cirac, Phys. Rev. Lett.92, 207901 (2004); X.-L. Deng, D. Porras, and J. I. Cirac, Phys. Rev. A 72, 063407 (2005)
work page 2003
-
[12]
L. M. K. Vandersypen and I. L. Chuang, Rev. Mod. Phys. 76, 1037 (2005); K. R. K. Rao, H. Katiyar, T. S. Mahesh, A. Sen (De), U. Sen, and A. Kumar, Phys. Rev. A 88, 022312 (2013)
work page 2005
-
[13]
L.-M. Duan, E. Demler, and M. D. Lukin, Phys. Rev. Lett. 91, 090402 (2003); O. Mandel, M. Greiner, A. Widera, T. Rom, T. W. Hansch, and I. Bloch, Nature425, 937 (2003); I. Bloch, J. Phys. B: At. Mol. Opt. Phys. 38, S629 (2005); P. Treutlein, T. Steinmetz, Y . Colombe, B. Lev, P. Hommelhoff, J. Reichel, M. Greiner, O. Mandel, A. Widera, T. Rom, I. Bloch, a...
work page 2003
- [14]
-
[15]
Spin chains as data buses, logic buses and entanglers,
S. Bose, Phys. Rev. Lett. 91, 207901 (2003); S. Bose, A. Bayat, P. Sodano, L. Banchi, and P. Verrucchi, “Spin chains as data buses, logic buses and entanglers,” in Quan- tum State Transfer and Network Engineering , edited by G. M. Nikolopoulos and I. Jex (Springer Berlin, Heidelberg, 2013) Chap. 1, pp. 1–38
work page 2003
-
[16]
M. Hein, W. D ¨ur, J. Eisert, R. Raussendorf, M. Van den Nest, and H. J. Briegel, arXiv:quant-ph/0602096 (2006)
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[17]
U. Schollw ¨ock, Rev. Mod. Phys.77, 259 (2005); F. Verstraete, V . Murg, and J. Cirac, Advances in Physics 57, 143 (2008); U. Schollw ¨ock, Annals of Physics 326, 96 (2011), january 2011 Special Issue; R. Or ´us, Annals of Physics 349, 117 (2014); J. C. Bridgeman and C. T. Chubb, Journal of Physics A: Mathematical and Theoretical 50, 223001 (2017)
work page 2005
-
[18]
Renormalization algorithms for Quantum-Many Body Systems in two and higher dimensions
F. Verstraete and J. I. Cirac, arXiv:cond-mat/0407066 (2004); G. Vidal, Phys. Rev. Lett.99, 220405 (2007); Phys. Rev. Lett. 101, 110501 (2008); M. Rizzi, S. Montangero, and G. Vi- dal, Phys. Rev. A 77, 052328 (2008); M. Aguado and G. Vi- dal, Phys. Rev. Lett. 100, 070404 (2008); L. Cincio, J. Dziar- maga, and M. M. Rams, Phys. Rev. Lett. 100, 240603 (2008...
work page internal anchor Pith review Pith/arXiv arXiv 2004
-
[19]
B. E. Kane, Nature 393, 133 (1998); Y . Makhlin, G. Sc ¨ohn, and A. Shnirman, Nature 398, 305 (1999); A. Imamog ¯lu, D. D. Awschalom, G. Burkard, D. P. DiVincenzo, D. Loss, M. Sherwin, and A. Small, Phys. Rev. Lett. 83, 4204 (1999); S.-B. Zheng and G.-C. Guo, Phys. Rev. Lett.85, 2392 (2000); J. I. Cirac and P. Zoller, Nature404, 579 (2000)
work page 1998
- [20]
-
[21]
N. Y . Yao, L. Jiang, A. V . Gorshkov, Z.-X. Gong, A. Zhai, L.-M. Duan, and M. D. Lukin, Phys. Rev. Lett. 106, 040505 (2011); Y . Ping, B. W. Lovett, S. C. Benjamin, and E. M. Gauger, Phys. Rev. Lett. 110, 100503 (2013); Y .-M. Zhu and L. Ma, Physics Letters A 382, 1651 (2018); R. Grimaudo, A. S. Magalh ˜aes de Castro, A. Messina, and D. Valenti, Fortschr...
work page 2011
-
[22]
Yung, Journal of Physics B: Atomic, Molecular and Op- tical Physics 44, 135504 (2011)
M.-H. Yung, Journal of Physics B: Atomic, Molecular and Op- tical Physics 44, 135504 (2011)
work page 2011
-
[23]
H.-L. Deng and X.-M. Fang, Journal of Physics B: Atomic, Molecular and Optical Physics 41, 025503 (2008)
work page 2008
-
[24]
A. O. Sushkov, I. Lovchinsky, N. Chisholm, R. L. Walsworth, H. Park, and M. D. Lukin, Phys. Rev. Lett. 113, 197601 (2014)
work page 2014
-
[25]
S. Haddadi, M. Ghominejad, A. Akhound, and M. R. Pourkarimi, Scientific Reports 11, 22691 (2021)
work page 2021
-
[26]
D. T urkpence, F. Altintas, M. Paternostro, and Ozg ur E. M ustecaplio˘glu, Europhysics Letters 117, 50002 (2017)
work page 2017
-
[27]
O. Arisoy and ¨O. E. M ¨ustecaplıo˘glu, Scientific Reports 11, 12981 (2021)
work page 2021
- [28]
-
[29]
F. Anz `a, B. Militello, and A. Messina, Journal of Physics B: Atomic, Molecular and Optical Physics 43, 205501 (2010); B. Militello and A. Messina, Phys. Rev. A83, 042305 (2011); X. S. Ma, G. X. Zhao, J. Y . Zhang, and A. M. Wang, 13 Quantum Information Processing 12, 321 (2013); W.-B. He, S. Chesi, H.-Q. Lin, and X.-W. Guan, Phys. Rev. B 99, 174308 (201...
-
[30]
S. Haddadi, M. R. Pourkarimi, A. Akhound, and M. Ghominejad, Modern Physics Letters A 34, 1950175 (2019)
work page 2019
-
[31]
C. Radhakrishnan, Z. L ¨u, J. Jing, and T. Byrnes, Phys. Rev. A 100, 042333 (2019)
work page 2019
-
[32]
K. Modi, A. Brodutch, H. Cable, T. Paterek, and V . Vedral, Rev. Mod. Phys. 84, 1655 (2012); A. Bera, T. Das, D. Sad- hukhan, S. S. Roy, A. Sen(De), and U. Sen, Reports on Progress in Physics 81, 024001 (2017)
work page 2012
-
[33]
V . E. Korepin, N. M. Bogoliubov, and A. G. Izergin,Quantum Inverse Scattering Method and Correlation Functions , Cam- bridge Monographs on Mathematical Physics (Cambridge University Press, 1993); F. Mila, European Journal of Physics 21, 499 (2000); T. Giamarchi, Quantum physics in one dimen- sion, International series of monographs on physics (Claren- do...
work page 1993
-
[34]
D. P. DiVincenzo, C. A. Fuchs, H. Mabuchi, J. A. Smolin, A. Thapliyal, and A. Uhlmann, arXiv:quant-ph/9803033 (1998)
work page internal anchor Pith review Pith/arXiv arXiv 1998
-
[35]
F. Verstraete, M. Popp, and J. I. Cirac, Phys. Rev. Lett. 92, 027901 (2004); M. Popp, F. Verstraete, M. A. Mart ´ın- Delgado, and J. I. Cirac, Phys. Rev. A 71, 042306 (2005)
work page 2004
-
[36]
D. Sadhukhan, S. S. Roy, A. K. Pal, D. Rakshit, A. Sen(De), and U. Sen, Phys. Rev. A 95, 022301 (2017); J. G. Krishnan, H. K. J., and A. K. Pal, Phys. Rev. A 107, 042411 (2023)
work page 2017
-
[37]
R. Banerjee, A. K. Pal, and A. Sen(De), Phys. Rev. A 101, 042339 (2020); Phys. Rev. Res. 4, 023035 (2022)
work page 2020
-
[38]
J. I. Latorre, R. Or ´us, E. Rico, and J. Vidal, Phys. Rev. A 71, 064101 (2005); R. G. Unanyan, C. Ionescu, and M. Fleis- chhauer, Phys. Rev. A72, 022326 (2005)
work page 2005
-
[39]
M. B. Plenio, Phys. Rev. Lett. 95, 090503 (2005)
work page 2005
-
[40]
A. Peres, Phys. Rev. Lett. 77, 1413 (1996); M. Horodecki, P. Horodecki, and R. Horodecki, Phys. Lett. A 223, 1 (1996); K. ˙Zyczkowski, P. Horodecki, A. Sanpera, and M. Lewen- stein, Phys. Rev. A58, 883 (1998); G. Vidal and R. F. Werner, Phys. Rev. A65, 032314 (2002); J. Lee, M. S. Kim, Y . J. Park, and S. Lee, Journal of Modern Optics 47, 2151 (2000)
work page 1996
-
[41]
R. H. Dicke, Phys. Rev. 93, 99 (1954); M. Bergmann and O. G ¨uhne, Journal of Physics A: Mathematical and Theoret- ical 46, 385304 (2013); B. L ¨ucke, J. Peise, G. Vitagliano, J. Arlt, L. Santos, G. T ´oth, and C. Klempt, Phys. Rev. Lett. 112, 155304 (2014); A. Kumar, H. S. Dhar, R. Prabhu, A. Sen(De), and U. Sen, Physics Letters A 381, 1701 (2017)
work page 1954
-
[42]
T. J. Osborne and M. A. Nielsen, Phys. Rev. A 66, 032110 (2002)
work page 2002
-
[43]
J. K. Stockton, J. M. Geremia, A. C. Doherty, and H. Mabuchi, Phys. Rev. A 67, 022112 (2003)
work page 2003
-
[44]
E. Barouch, B. M. McCoy, and M. Dresden, Phys. Rev. A 2, 1075 (1970); E. Barouch and B. M. McCoy, Phys. Rev. A 3, 786 (1971); Phys. Rev. A 3, 2137 (1971)
work page 1970
- [45]
-
[46]
C. De Dominicis and I. Giardina, Random Fields and Spin Glasses: A Field Theory Approach (Cambridge University Press, 2006)
work page 2006
-
[47]
Y . Wang, Z. Hu, B. C. Sanders, and S. Kais, Frontiers in Physics 8 (2020), 10.3389/fphy.2020.589504
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