pith. sign in

arxiv: 2606.00163 · v1 · pith:6TAZOWJOnew · submitted 2026-05-29 · ✦ hep-th · cond-mat.stat-mech· gr-qc· quant-ph

Phase separation seeded by Z2 and U(1) topological defects from holography

Pith reviewed 2026-06-28 21:39 UTC · model grok-4.3

classification ✦ hep-th cond-mat.stat-mechgr-qcquant-ph
keywords phase separationtopological defectsholographyspinodal decompositionsymmetry breakingZ2 defectsU(1) defectsdouble quench
0
0 comments X

The pith

Topological defects from symmetry breaking seed phase separation in holographic models.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper uses a double-quench protocol in holography to link spontaneous symmetry breaking with phase separation. An initial quench rapidly crosses the critical point and creates topological defects, after which a second quench drives the system into the unstable spinodal regime. The cores of these defects, whether from Z2 or U(1) symmetry, expand into macroscopic phase-separated domains. Both types of defects produce identical dynamical patterns, supporting the claim that defects act as universal nucleation seeds. This connects two common processes in systems with multiple instabilities through the positions of pre-existing defects.

Core claim

In holographic models with a double-quench protocol, topological defects generated during the initial symmetry-breaking quench serve as nucleation sites for phase separation triggered by the subsequent quench into the spinodal regime. The defect cores expand into macroscopic domains, and this behavior is universal across Z2 and U(1) systems despite their different topological properties.

What carries the argument

Topological defects (domain walls or vortices) created by the first quench, which expand during spinodal decomposition to form phase-separated domains.

If this is right

  • Nucleation sites of phase separation are fixed by the locations of defects formed in the first quench.
  • Macroscopic domains grow directly by expansion of the defect cores rather than by random fluctuations.
  • The same dynamical sequence occurs for both Z2 and U(1) defects.
  • Topological defects serve as universal seeds for phase separation across different symmetry classes.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The result suggests that engineering initial defect density could control the pattern of phase separation in analogous non-holographic models.
  • Similar seeding by defects may occur in real condensed-matter systems such as binary fluids or magnetic materials undergoing multiple quenches.
  • The universality across symmetries implies the mechanism could be tested in effective field theories without gravity duals.

Load-bearing premise

The double-quench protocol in the holographic model accurately isolates the role of topological defects as the dominant nucleation seeds without other dynamical factors dominating the phase separation process.

What would settle it

A holographic simulation in which phase separation nucleates at locations unrelated to the initial defect positions, or in which defect cores do not expand into the domains, would falsify the seeding claim.

Figures

Figures reproduced from arXiv: 2606.00163 by Jing-Fei Zhang, Xin Zhang, Zhang-Yu Nie, Zi-Qiang Zhao.

Figure 1
Figure 1. Figure 1: FIG. 1. The time evolution of the scalar condensate in [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. Nonequilibrium evolution of the system with [PITH_FULL_IMAGE:figures/full_fig_p003_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. Nonequilibrium evolution of the system with [PITH_FULL_IMAGE:figures/full_fig_p004_3.png] view at source ↗
read the original abstract

We study the interaction between spontaneous symmetry breaking and phase separation dynamics in holography. Using a double-quench protocol, the system first rapidly crosses the critical point and generates topological defects, while a second quench drives the system into a nonlinear unstable regime with spinodal decomposition. We investigate both $\mathbb{Z}_2$ and $U(1)$ symmetric systems, where different types of topological defects emerge during symmetry breaking. We show that topological defects dynamically determine the nucleation sites of phase separation. As the instability grows, the defect cores expand into macroscopic phase-separated domains. Despite the distinct symmetries and topological properties of these defects, both systems exhibit the same universal dynamical behavior, indicating that topological defects can universally serve as dynamical seeds for subsequent phase separation.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

1 major / 0 minor

Summary. The paper studies the interaction of spontaneous symmetry breaking and phase separation in holographic models via a double-quench protocol. The first quench generates Z2 or U(1) topological defects; the second drives the system into a spinodal regime. The central claim is that defect cores expand into macroscopic phase-separated domains and that both symmetries exhibit the same universal dynamical behavior, implying topological defects universally seed phase separation.

Significance. If the numerical results are robust, the work supplies concrete holographic evidence that topological defects can act as dominant nucleation sites for spinodal decomposition, independent of the underlying symmetry. This offers a dynamical mechanism that may apply to strongly coupled non-equilibrium systems and is supported by direct time evolution rather than fitted parameters.

major comments (1)
  1. [Protocol and numerical setup (likely §3)] The double-quench protocol description leaves open whether control runs (defect-free states after the first quench, or varied second-quench amplitudes) were performed to show that phase separation is suppressed or relocated in the absence of pre-existing defects. Without such controls, it is unclear whether the second quench itself triggers widespread spinodal nucleation from homogeneous regions or numerical fluctuations, which directly affects the claim that defects are the dominant seeds.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for the careful reading of our manuscript and the constructive comment on the double-quench protocol. We address the point below and will revise the manuscript accordingly to strengthen the presentation of our numerical evidence.

read point-by-point responses
  1. Referee: [Protocol and numerical setup (likely §3)] The double-quench protocol description leaves open whether control runs (defect-free states after the first quench, or varied second-quench amplitudes) were performed to show that phase separation is suppressed or relocated in the absence of pre-existing defects. Without such controls, it is unclear whether the second quench itself triggers widespread spinodal nucleation from homogeneous regions or numerical fluctuations, which directly affects the claim that defects are the dominant seeds.

    Authors: We agree that explicit control simulations would provide stronger confirmation that defects are the dominant nucleation sites. In the present work the first quench is spatially uniform and crosses the critical point, generating topological defects via the Kibble-Zurek mechanism as the only source of inhomogeneity; the second quench is likewise uniform. Our simulations across multiple realizations consistently show that spinodal domains nucleate and expand from the defect cores rather than appearing randomly. Nevertheless, we acknowledge that the manuscript does not report dedicated runs with a modified first quench (e.g., adiabatic or symmetry-preserving) that would leave the system defect-free after the first stage. We will therefore add a new subsection in §3 describing (i) the evolution under a slower first quench that suppresses defect formation and (ii) the effect of varying the amplitude of the second quench. These additional results will be included in the revised manuscript to demonstrate that phase separation is indeed relocated or suppressed when pre-existing defects are absent. revision: yes

Circularity Check

0 steps flagged

No circularity: claims rest on numerical holographic evolution

full rationale

The paper's central claim—that topological defects from a first quench seed phase separation after a second quench—is advanced via direct numerical solution of the holographic equations of motion under the described double-quench protocol. No equations, ansatze, or uniqueness theorems are quoted that reduce the reported dynamical behavior to fitted parameters, self-citations, or definitional identities. The derivation chain is therefore self-contained and independent of the enumerated circularity patterns.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 0 invented entities

Based solely on the abstract, no explicit free parameters, axioms, or invented entities are identifiable; the holographic model and quench protocol are treated as standard background.

pith-pipeline@v0.9.1-grok · 5670 in / 1168 out tokens · 23227 ms · 2026-06-28T21:39:51.516104+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

43 extracted references · 2 canonical work pages

  1. [1]

    W. H. Zurek, Nature317, 505 (1985)

  2. [2]

    A. J. Bray, Adv. Phys.43, 357 (1994), arXiv:cond- mat/9501089

  3. [3]

    L. E. Sadler, J. M. Higbie, S. R. Leslie, M. Vengalattore, and D. M. Stamper-Kurn, Nature443, 312 (2006)

  4. [4]

    T. W. B. Kibble, J. Phys. A9, 1387 (1976)

  5. [5]

    Polkovnikov, K

    A. Polkovnikov, K. Sengupta, A. Silva, and M. Vengalat- tore, Rev. Mod. Phys.83, 863 (2011), arXiv:1007.5331 [cond-mat.stat-mech]

  6. [6]

    W. H. Zurek, Phys. Rept.276, 177 (1996), arXiv:cond- mat/9607135

  7. [7]

    Digal, R

    S. Digal, R. Ray, and A. M. Srivastava, Phys. Rev. Lett. 83, 5030 (1999), arXiv:hep-ph/9805502

  8. [8]

    M. E. Dodd, P. C. Hendry, N. S. Lawson, P. V. E. Mc- Clintock, and C. D. H. Williams, Phys. Rev. Lett.81, 3703 (1998), arXiv:cond-mat/9808117

  9. [9]

    Carmi, E

    R. Carmi, E. Polturak, and G. Koren, Phys. Rev. Lett. 84, 4966 (2000)

  10. [10]

    del Campo and W

    A. del Campo and W. H. Zurek, Int. J. Mod. Phys. A29, 1430018 (2014), arXiv:1310.1600 [cond-mat.stat-mech]

  11. [11]

    Sonner, A

    J. Sonner, A. del Campo, and W. H. Zurek, Nature Commun.6, 7406 (2015), arXiv:1406.2329 [hep-th]

  12. [12]

    Li, H.-Q

    Z.-H. Li, H.-Q. Shi, and H.-Q. Zhang, JHEP05, 056 (2022), arXiv:2111.15230 [hep-th]

  13. [13]

    Zeng, C.-Y

    H.-B. Zeng, C.-Y. Xia, and A. del Campo, Phys. Rev. Lett.130, 060402 (2023), arXiv:2204.13529 [cond- mat.stat-mech]

  14. [14]

    del Campo, F

    A. del Campo, F. J. G´ omez-Ruiz, and H.-Q. Zhang, Phys. Rev. B106, L140101 (2022), arXiv:2202.11731 [cond-mat.stat-mech]

  15. [15]

    Xia, H.-B

    C.-Y. Xia, H.-B. Zeng, A. Grabarits, and A. del Campo, Nature Commun.17, 3668 (2026), arXiv:2406.09433 [cond-mat.stat-mech]

  16. [16]

    Ma, H.-Q

    T.-C. Ma, H.-Q. Shi, H.-Q. Zhang, and A. del Campo, Phys. Rev. Res.7, 013096 (2025), arXiv:2406.05167 [cond-mat.stat-mech]

  17. [17]

    Yang, C.-Y

    P. Yang, C.-Y. Xia, S. Grieninger, H.-B. Zeng, and M. Baggioli, Phys. Rev. Lett.136, 051602 (2026), arXiv:2508.05964 [cond-mat.stat-mech]

  18. [18]

    C.-X. Wang, A. Grabarits, J.-M. Cui, H.-B. Zeng, Y.- F. Huang, C.-F. Li, and A. del Campo, (2025), arXiv:2507.01087 [quant-ph]

  19. [19]

    B. Ko, J. W. Park, and Y. Shin, Nature Physics15, 1227–1231 (2019)

  20. [20]

    Monaco, J

    R. Monaco, J. Mygind, and R. J. Rivers, Physical Review Letters89(2002), 10.1103/physrevlett.89.080603

  21. [21]

    C. N. Weiler, T. W. Neely, D. R. Scherer, A. S. Bradley, M. J. Davis, and B. P. Anderson, Nature455, 948–951 (2008)

  22. [22]

    J. W. Cahn and J. E. Hilliard, The Journal of Chemical Physics28, 258 (1958)

  23. [23]

    J. W. Cahn, Acta Metallurgica9, 795 (1961)

  24. [24]

    P. C. Hohenberg and B. I. Halperin, Rev. Mod. Phys.49, 435 (1977)

  25. [25]

    Barra and P

    E. Nicklas, H. Strobel, T. Zibold, C. Gross, B. A. Malomed, P. G. Kevrekidis, and M. K. Oberthaler, Physical Review Letters107(2011), 10.1103/phys- revlett.107.193001

  26. [26]

    Franco, A

    S. Franco, A. Garcia-Garcia, and D. Rodriguez-Gomez, JHEP04, 092 (2010), arXiv:0906.1214 [hep-th]

  27. [27]

    Gregory, S

    R. Gregory, S. Kanno, and J. Soda, JHEP10, 010 (2009), arXiv:0907.3203 [hep-th]

  28. [28]

    Zhang, C.-Y

    X.-K. Zhang, C.-Y. Xia, Z.-Y. Nie, and H. Zeng, Phys. Rev. D105, 046016 (2022), arXiv:2105.14294 [hep-th]

  29. [29]

    Zhao, X.-K

    Z.-Q. Zhao, X.-K. Zhang, and Z.-Y. Nie, JHEP02, 023 (2023), arXiv:2211.14762 [hep-th]

  30. [30]

    Zhao, Z.-Y

    X. Zhao, Z.-Y. Nie, Z.-Q. Zhao, H.-B. Zeng, Y. Tian, and M. Baggioli, JHEP02, 184 (2024), arXiv:2311.08277 [hep-th]

  31. [31]

    Jin, Y.-p

    Z.-h. Jin, Y.-p. An, and L. Li, (2026), arXiv:2604.17216 [hep-th]

  32. [32]

    R. A. Janik, J. Jankowski, and H. Soltanpanahi, Phys. Rev. Lett.117, 091603 (2016), arXiv:1512.06871 [hep- th]

  33. [33]

    R. A. Janik, J. Jankowski, and H. Soltanpanahi, Phys. Rev. Lett.119, 261601 (2017), arXiv:1704.05387 [hep- th]

  34. [34]

    Attems, Y

    M. Attems, Y. Bea, J. Casalderrey-Solana, D. Mateos, and M. Zilh˜ ao, JHEP01, 106 (2020), arXiv:1905.12544 [hep-th]

  35. [35]

    Bellantuono, R

    L. Bellantuono, R. A. Janik, J. Jankowski, and H. Soltanpanahi, JHEP10, 146 (2019), arXiv:1906.00061 [hep-th]

  36. [36]

    Li, Z.-Y

    X. Li, Z.-Y. Nie, and Y. Tian, JHEP09, 063 (2020), arXiv:2003.12987 [hep-th]

  37. [37]

    Q. Chen, Y. Liu, Y. Tian, X. Wu, and H. Zhang, Phys. Rev. D108, 106017 (2023), arXiv:2211.11291 [hep-th]

  38. [38]

    Q. Chen, Y. Liu, Y. Tian, X. Wu, and H. Zhang, Sci. China Phys. Mech. Astron.68, 260414 (2025), 6 arXiv:2408.09679 [hep-th]

  39. [39]

    Zhao, Z.-Y

    Z.-Q. Zhao, Z.-Y. Nie, J.-F. Zhang, and X. Zhang, (2026), arXiv:2604.00690 [hep-th]

  40. [40]

    Zhao, Z.-Y

    Z.-Q. Zhao, Z.-Y. Nie, J.-F. Zhang, and X. Zhang, (2026), arXiv:2604.13104 [cond-mat.stat-mech]

  41. [41]

    S. A. Hartnoll, C. P. Herzog, and G. T. Horowitz, Phys. Rev. Lett.101, 031601 (2008), arXiv:0803.3295 [hep-th]

  42. [42]

    S. A. Hartnoll, C. P. Herzog, and G. T. Horowitz, JHEP 12, 015 (2008), arXiv:0810.1563 [hep-th]

  43. [43]

    C. P. Herzog, Phys. Rev. D81, 126009 (2010), arXiv:1003.3278 [hep-th]. Appendix A: Full equations of motion The formulas for the nonequilibrium evolution of a system withZ 2 symmetry are ∂zψf ′ 2 + ψf ′ 2z − 1 4 αψz2eαψ2z2 f ∂zAx 2 +f ∂ zAy 2 −2∂ tAx∂zAx −2∂ tAy∂zAy + 2∂xAt∂zAx +∂ xAy 2 −2∂ xAy∂yAx +2∂yAt∂zAy +∂ yAx 2 −∂ zAt 2 + f ∂z∂zψ 2 − f ψ z2 −λψ 3 −...