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REVIEW 3 major objections 4 minor 42 references

Exact Modular Completion of the ABJM Effective Twisted Superpotential

T0 review · 3 major / 4 minor · reviewed 2026-08-15 · deepseek-v4-flash

Pith's one-line read For ABJM theory at $k=1,2,4$, the nonperturbative remainder of the on-shell effective twisted superpotential is exactly one absolutely convergent divisor-sum $q$-series built from a weight-four Eisenstein–Eichler integral, reproducing…

desk verdict A strong numerical discovery with a central typo: Eq. (12) and Eq. (15) are off by m^4, so the paper as printed is not internally consistent. read the letter →

arxiv 2608.04107 v1 pith:R4B74H5R submitted 2026-08-04 hep-th

classification hep-th MSC 11F1181T13
keywords ABJMtheorytwistedsuperpotentialEisensteinseriesEichlerintegraldivisor-sumq-seriesconstantmapinteger-relationdetectionBethevacua
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

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

The reading

This paper claims that the nonperturbative sector of a central quantity in three-dimensional supersymmetric field theory is simpler than the standard transseries picture suggests. In ABJM theory at Chern–Simons levels $k=1,2,4$, the exponentially small tail of the effective twisted superpotential is exactly a single absolutely convergent divisor-sum $q$-series. The paper also fixes the full perturbative part for every level and gives a closed all-genus coefficient formula. If the claims are right, the complete coefficient of $1/\omega$ in the Cardy limit of the topologically twisted index is known in closed form at those levels, including finite-$N$ nonperturbative corrections, and the same exponentials become testable microscopic data for the $\mathrm{AdS}_4$ black hole entropy function. The evidence is high-precision numerical discovery, reproducing 800-digit Bethe-vacuum data to about $10^{-797}$.

What carries the argument

The carrying object is the first-order operator $(1+tD)$ acting on Eichler integrals, where $D=Q\,\mathrm{d}/\mathrm{d}Q$ multiplies the $m$-th Fourier coefficient by $m$. Weight-four Eisenstein combinations $E_4(Q)-L^2 E_4(Q^L)$ on $\Gamma_0(L)$, with $L=2$ for $k=1,2$ and $L=4$ for $k=4$, have Fourier coefficients $\sigma_3(m)-L^2\sigma_3(m/L)$. Their coefficientwise Eichler primitive, the third antiderivative, sends $a_m Q^m$ to $a_m m^{-3}Q^m$. Applying $(1+tD)$ then turns $a_m/m^3$ into $a_m(t/m^2+1/m^3)$, reproducing the series in (11). Absolute convergence follows from $\sigma_3(m)/m^2=O(m^{1+\epsilon})$ and from the subtraction terms; the paper shows $\limsup_m |c_m^{(k)}|^{1/m}=1$, so the physical remainder converges absolutely for $0<q<1$. This object carries the argument by packaging the entire exponentially small tail into classical modular data.

What would settle it

Compute the on-shell $\operatorname{Im}W$ for a rank $N>100$ at $k=1,2,4$ with the same 800-digit precision and compare with (10)–(12); any residual above the data rounding floor, about $5\times10^{-797}$, would falsify the exact completion. Alternatively, a direct derivation from the Bethe equations that produces a correction to (12) which is exponentially small on the computed ranks but nonzero for larger $N$ would also settle the claim.

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Extended reading notes

Core claim

The paper's central claim is that the on-shell effective twisted superpotential of $U(N)_k\times U(N)_{-k}$ ABJM theory at the universal twist and the dominant Bethe vacuum, $\operatorname{Im} W(N,k)$, decomposes exactly as $\frac{\pi^2}{3}\sqrt{k/2}\,\hat b_N^{3/2}+C(k)+W_{\mathrm{np}}(N,k)$. The perturbative part closes after two terms: the shifted-rank $3/2$ power with $\hat b_N=N-k/24+2/(3k)$, and an $N$-independent constant map $C(k)$ given by parity-dependent finite Clausen sums at every integer level. At $k=1,2,4$ the entire finite-$N$ remainder is the absolutely convergent divisor-sum series $W_{\mathrm{np}}(N,k)=\frac{k^2}{2\pi}\sum_{m\ge1} c_m^{(k)}(t+1/m)\,q^m$, with $c_m^{(k)}$ given by divisor sums $\sigma_3(m)$ with subtraction terms, equivalently by $(1+tD)\Phi_k(-q)$, where $\Phi_k$ is the Eichler integral of a weight-four Eisenstein combination on $\Gamma_0(2)$ or $\Gamma_0(4)$. This closed form reproduces 800-digit Bethe-vacuum data to about $10^{-797}$ for every rank $2\le N\le 100$ at those levels. The paper also gives a closed coefficient formula for the asymptotic type-IIA genus expansion at arbitrary genus, involving binomial coefficients and Bernoulli numbers.

Load-bearing premise

The exactness claim rests on the assumption that the numbers reconstructed from high-precision data — the rank shift $\hat b_N=N-k/24+2/(3k)$, the constant plateau $C(k)$, and the divisor-sum coefficients fitted for $N\le 100$ — are exactly correct for all $N$ and all ranks, rather than merely extraordinarily accurate numerical coincidences on the computed range.

Editorial extensions

If this is right

  • At $k=1,2,4$, the nonperturbative instanton sector of $\operatorname{Im}W$ is not an asymptotic expansion that must be stopped at an optimal order; the remainder converges absolutely for $0<q<1$, so the finite-$N$ answer can be evaluated to any precision by truncating (11).
  • The full Cardy-limit coefficient of the superconformal index at the universal twist is determined at those levels, including its exponentially small finite-$N$ tail, not just the leading $N^{3/2}$ term.
  • The series provides explicit exponential corrections that a quantum-corrected $\mathrm{AdS}_4$ black hole entropy function would have to reproduce, giving a concrete microscopic target.
  • The constant map $C(k)$ is fixed in closed form for every positive integer level, so the previously undetermined $N$-independent constant in the on-shell twisted superpotential is no longer a free parameter.
  • The parity-dependent Clausen formulas and the level-dependent modular groups ($\Gamma_0(2)$ for $k=1,2$ and $\Gamma_0(4)$ for $k=4$) give arithmetic constraints that any exact derivation from the Bethe equations will have to explain.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the Eisenstein–Eichler organization is not a numerical accident, the same operator $(1+tD)$ may appear in the nonperturbative completion of other twisted-superpotential observables at these levels, with the universal twist acting as a projection onto a modular subsector; the paper raises this as an interpretation and does not claim a transformation law for $(1+tD)\Phi_k$.
  • Because the divisor coefficients are reconstructed rather than derived, a proof from the Bethe equations would likely reveal how root-of-unity dilogarithm identities assemble into Eisenstein coefficients; absent that proof, the sharpest test is to compute new ranks $N>100$ at $k=1,2,4$ and require the residual to stay on the $10^{-797}$ floor.
  • One could probe the specialness of $k=1,2,4$ by running the same discovery approach on other twists or on the topologically twisted index, where the paper notes a parallel constant map and a modular subsector appear in the companion work; if that modular structure persists, it would suggest a broader arithmetic organization rather than an accident of the universal twist.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

3 major / 4 minor

Summary. The paper analyzes the on-shell effective twisted superpotential of U(N)_k × U(N)_-k ABJM theory at the universal twist and the dominant Bethe vacuum, using high-precision numerical data (up to 800 digits) and machine-learning techniques (PSLQ integer-relation detection and sparse regression). It claims that the perturbative part terminates after a shifted-rank 3/2-power plus an N-independent constant map C(k) with closed-form expressions for every integer k (Eqs. (4)–(5), equivalently (6)), that the fixed-λ genus expansion has an explicit all-genus coefficient formula (7)–(9) and is asymptotic, and that for k=1,2,4 the entire finite-N remainder is an absolutely convergent divisor-sum q-series (10)–(12), equivalent term-by-term to the Eichler-integral representation (15) of a weight-four Eisenstein series on Γ0(2) or Γ0(4). The claimed numerical precision is extremely high: residuals reach ~10^-797 across 297 data points. The paper is candid about the status of its statements: the constant map and divisor coefficients are arithmetically reconstructed, and the proof of the all-level integral reduction is deferred to a companion paper.

Significance. If the central claims hold, the result is significant: it would show that the nonperturbative completion of the ABJM twisted superpotential at special levels is a single absolutely convergent Eisenstein–Eichler q-series rather than an asymptotic multi-instanton transseries, and it would provide closed-form constant-map and all-genus data relevant to supersymmetric AdS4 black-hole entropy. The paper's strengths include the extraordinary numerical agreement (800 digits, systematically cross-checked), the independent numerical audit of the Clausen, Euler, and integral representations using no Bethe data (Supplemental Material, Eq. (25)), and the explicit admission, in the text, of which statements are derived and which are reconstructed. These strengths make the conjectures credible, but they do not replace the missing derivations.

major comments (3)
  1. [Exact modular completion, Eq. (12) vs Eq. (15)]
  2. [Constant map and the deferred proof]
  3. [Exactness for all N and the status of Eq. (12)]
minor comments (4)
  1. [Comparison with literature]
  2. [Supplementary Figure 3 caption]
  3. [Data availability]
  4. [Conventions for q and Q]

Circularity Check

2 steps flagged · score 5.0 of 10

Partially circular: constant-map proof is deferred to a same-author companion paper, and the modular completion is an analytic repackaging of coefficients fitted from the same data; Eqs. (12) and (15) are additionally inconsistent as printed.

  1. self citation load bearing [Eq. (6) and Supplemental Material, 'Status of the general evaluation']
    "A companion paper [24] proves that, for every positive integer k, C(k) =− k2ζ(3) 16π + 2k π Z ∞ 0 log(2 coshx) log (1−e−kx) dx. ... The remaining root-of-unity evaluation of that rational-argument Euler sum is deferred to Ref. [24]."

    The paper's claim of a closed-form constant map for every integer level depends on the integral identity (6), whose proof is not contained in this manuscript. The only support offered here is a 'to appear' companion paper by the same author, plus a 70-digit numerical audit. The general-C(k) statement is therefore load-bearing and rests on an unverified self-citation rather than on a proof established in the present work.

  2. self definitional [Exact modular completion, text after Eq. (15)]
    "The status of each statement is worth fixing here: (13) and (15) are analytic identities once (12) is given, whereas (12) itself is arithmetically reconstructed—exact rationals, identical when extracted independently from the 200- and 800-digit data—and established against the data rather than derived from the Bethe equations."

    This admits that the Eichler-integral identity (15) is not an independent derivation of the finite-N remainder; it is an analytic restatement of the fitted coefficients (12). The modular 'completion' therefore reduces, by construction, to the same high-precision Bethe-vacuum data used to fix (12). Moreover, the claimed term-by-term equivalence is false as printed: Eqs. (14)-(15) force coefficients proportional to [σ3(m)−L^2σ3(m/L)]/m^2, while (12) prints m^2 times the same bracket, a discrepancy visible already at k=1, m=2 (c_2=−100 vs −25/4).

full rationale

The paper is unusually transparent: it explicitly labels (12) as arithmetically reconstructed and (15) as an identity once (12) is given. That transparency turns the central 'exact completion' into a by-construction restatement rather than a derivation, and the deferred proof of (6) makes the all-level constant-map claim depend on a same-author companion paper. Nevertheless, large parts of the paper are genuinely non-circular and independently grounded: the shift (2) and the constant-map formulas (4)-(5) are validated on levels withheld from their assembly; the genus expansion (7)-(9) follows by direct expansion of the parent; and the independent Clausen/Euler/integral audit (25) uses no Bethe-vacuum data. The score reflects the two load-bearing reductions identified above, not an absence of content; the printed inconsistency between (12) and (15) is an additional correctness risk that further weakens the exact-completion claim as stated.

Assumptions & free parameters 4 free parameters · 5 assumptions · 0 invented entities

The central formulas rest on fitted rank shifts, fitted coefficients, a chosen PSLQ basis, and two deferred proofs. No new physical entities are introduced; the mathematical objects, Eisenstein series and Eichler integrals, are established constructions from the literature.

free parameters (4)
  • Rank shift s_k = -k/24 + 2/(3k) in bN = s_k = -k/24 + 2/(3k)
    Recovered by fitting a_k [N+s_k]^{3/2}+C(k) to data at each level; recognized as the universal-twist shift from Ref. [14]. All subsequent formulas use bN defined with this shift.
  • Leading 3/2-power coefficient a_k = pi^2/3 sqrt(k/2) = pi^2/3 * sqrt(k/2)
    Fitted together with the shift and constant in the three-parameter model, then identified with the known normalization. The exact value is not derived from the Bethe equations in this paper.
  • Clausen-basis coefficients in C(k) formulas (4)-(5) = Various rationals and the Catalan coefficient (-1)^{(p+1)/2}
    Determined by PSLQ from the plateau values of Im fW - leading term. The paper states the basis choice is an ansatz and that the relations are arithmetically reconstructed rather than derived.
  • Divisor coefficients in (12): (5,-20) for k=1,2 and (1,-16) for k=4 = 5, -20, 1, -16
    Reconstructed as exact integers from a high-precision linear system on q-series features, then recognized as coefficients of Eisenstein series combinations.
assumptions (5)
  • domain assumption The Bethe equations with principal branch and n_i = \tilde n_i = -i define the physical on-shell value.
    Adopted from Ref. [26]. The paper states that every result refers to this dominant vacuum and branch, and that C(k) is not claimed invariant under all admissible branch changes.
  • ad hoc to paper The PSLQ ansatz: C(k) lies in the Q-span of zeta(3)/pi, Catalan's constant, and Cl_2(2πj/k) for j=1,...,k-1.
    The paper calls the basis an ansatz, though a falsifiable one. The pruning and held-out validation reduce the risk, but the choice is not derived.
  • ad hoc to paper The root-of-unity evaluation of the Euler sum proves C_int(k)=C(k) for all positive integer k.
    Deferred to companion paper [24]. The paper relies on this for the claim that the closed constant formulas hold at every integer level.
  • ad hoc to paper High-precision numerical agreement certifies exactness of the q-series for all N beyond the computed range.
    The paper promotes fitted formulas to exact identities while noting that deriving the finite-N divisor structure directly from the Bethe equations remains an open problem.
  • domain assumption The two independent numerical solvers (gradient flow and continuation scheme) reliably produce the correct Bethe vacua.
    All discovery depends on the 200-digit and 800-digit decimal strings. The two methods agree, but no formal proof of correctness is given.

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Pith. "Pith review of Exact Modular Completion of the ABJM Effective Twisted Superpotential." pith.science (2026). https://pith.science/paper/R4B74H5R

@misc{pith2026260804107,
  author       = {Pith},
  title        = {Pith review of: Exact Modular Completion of the ABJM Effective Twisted Superpotential},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/R4B74H5R}},
  note         = {Machine review of arXiv:2608.04107}
}
abstract

The effective twisted superpotential governs the supersymmetric partition functions of three-dimensional $\mathcal{N}=2$ theories in the Cardy limit and, at large $N$, the gravitational blocks that are glued into the entropy function of supersymmetric $\mathrm{AdS}_4$ black holes. We determine its on-shell structure for $\mathrm{U}(N)_k\times\mathrm{U}(N)_{-k}$ ABJM theory at the universal twist, using a machine-learning discovery pipeline---physics-informed symbolic regression with integer-relation detection---applied to Bethe-vacuum data of up to $800$ digits. Its perturbative part terminates after two terms, a shifted-rank $3/2$-power and an $N$-independent constant map, which we obtain in closed form for every integer level. Its type-IIA genus expansion admits a closed coefficient formula at arbitrary genus, involving binomial and Bernoulli-number terms, and is asymptotic. For $k=1,2,4$ the entire finite-$N$ remainder is a single absolutely convergent divisor-sum $q$-series, obtained by applying a first-order differential operator to the Eichler integral of a weight-four Eisenstein series on $\Gamma_0(2)$ or $\Gamma_0(4)$. This closed form reproduces the data to $\sim\!10^{-797}$.

Figures

Figures reproduced from arXiv: 2608.04107 by the authors.

Figure 1
Figure 1. FIG. 1. The machine-learning discovery pipeline. High [PITH_FULL_IMAGE:figures/full_fig_p008_1.png] view at source ↗
Figure 2
Figure 2. FIG. 2. The genus expansion is asymptotic. Plotted is the [PITH_FULL_IMAGE:figures/full_fig_p009_2.png] view at source ↗
Figure 5
Figure 5. FIG. 5. Exactness at the special levels. For every [PITH_FULL_IMAGE:figures/full_fig_p009_5.png] view at source ↗

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Reference graph

Works this paper leans on

42 extracted references · 11 canonical work pages

  1. [1]

    Pasquetti, JHEP04, 120, arXiv:1111.6905 [hep-th]

    S. Pasquetti, JHEP04, 120, arXiv:1111.6905 [hep-th]

  2. [2]

    C. Beem, T. Dimofte, and S. Pasquetti, JHEP12, 177, arXiv:1211.1986 [hep-th]

  3. [3]

    N. A. Nekrasov and S. L. Shatashvili, Nucl. Phys. B Proc. Suppl.192-193, 91 (2009), arXiv:0901.4744 [hep-th]

  4. [4]

    Benini and A

    F. Benini and A. Zaffaroni, JHEP07, 127, arXiv:1504.03698 [hep-th]

  5. [5]

    Choi and C

    S. Choi and C. Hwang, JHEP03, 068, arXiv:1911.01448 [hep-th]

  6. [6]

    S. M. Hosseini and A. Zaffaroni, JHEP12, 025, arXiv:2209.09274 [hep-th]

  7. [7]

    Closset, H

    C. Closset, H. Kim, and B. Willett, JHEP11, 004, arXiv:1807.02328 [hep-th]

  8. [8]

    S. M. Hosseini, K. Hristov, and A. Zaffaroni, JHEP12, 168, arXiv:1909.10550 [hep-th]

Show all 42 references
  1. [9]

    Aharony, O

    O. Aharony, O. Bergman, D. L. Jafferis, and J. Malda- cena, JHEP10, 091, arXiv:0806.1218 [hep-th]

  2. [10]

    Marino and P

    M. Marino and P. Putrov, JHEP06, 011, arXiv:0912.3074 [hep-th]

  3. [11]

    Drukker, M

    N. Drukker, M. Marino, and P. Putrov, Commun. Math. Phys.306, 511 (2011), arXiv:1007.3837 [hep-th]

  4. [12]

    H. Fuji, S. Hirano, and S. Moriyama, JHEP08, 001, arXiv:1106.4631 [hep-th]

  5. [13]

    Marino and P

    M. Marino and P. Putrov, J. Stat. Mech.1203, P03001 (2012), arXiv:1110.4066 [hep-th]

  6. [14]

    Bobev, J

    N. Bobev, J. Hong, and V. Reys, Phys. Rev. Lett.129, 041602 (2022), arXiv:2203.14981 [hep-th]

  7. [15]

    Hatsuda, S

    Y. Hatsuda, S. Moriyama, and K. Okuyama, JHEP01, 158, arXiv:1211.1251 [hep-th]

  8. [16]

    Calvo and M

    F. Calvo and M. Marino, JHEP05, 006, arXiv:1212.5118 [hep-th]

  9. [17]

    Hatsuda, S

    Y. Hatsuda, S. Moriyama, and K. Okuyama, JHEP05, 054, arXiv:1301.5184 [hep-th]

  10. [18]

    Hatsuda, M

    Y. Hatsuda, M. Marino, S. Moriyama, and K. Okuyama, JHEP09, 168, arXiv:1306.1734 [hep-th]

  11. [19]

    Hatsuda, S

    Y. Hatsuda, S. Moriyama, and K. Okuyama, PTEP 2015, 11B104 (2015), arXiv:1507.01678 [hep-th]

  12. [20]

    Udrescu and M

    S.-M. Udrescu and M. Tegmark, Sci. Adv.6, eaay2631 (2020), arXiv:1905.11481 [physics.comp-ph]

  13. [21]

    Cranmer, arXiv e-prints (2023), arXiv:2305.01582 [astro-ph.IM]

    M. Cranmer, arXiv e-prints (2023), arXiv:2305.01582 [astro-ph.IM]

  14. [22]

    Ferguson, D

    H. Ferguson, D. Bailey, and S. Arno, Mathematics of Computation68, 351 (1999)

  15. [23]

    Raayoni, S

    G. Raayoni, S. Gottlieb, Y. Manor, G. Pisha, Y. Har- ris, U. Mendlovic, D. Haviv, Y. Hadad, and I. Kaminer, Nature590, 67 (2021)

  16. [24]

    S. M. Hosseini, to appear

  17. [25]

    Gustavsson and S.-J

    A. Gustavsson and S.-J. Rey, arXiv e-prints (2009), arXiv:0906.3568 [hep-th]

  18. [26]

    Benini, K

    F. Benini, K. Hristov, and A. Zaffaroni, JHEP05, 054, arXiv:1511.04085 [hep-th]

  19. [27]

    C. P. Herzog, I. R. Klebanov, S. S. Pufu, and T. Tesileanu, Phys. Rev. D83, 046001 (2011), arXiv:1011.5487 [hep-th]

  20. [28]

    S. M. Hosseini, Phys. Rev. Lett.136, 091601 (2026), arXiv:2510.24837 [hep-th]

  21. [29]

    S. M. Hosseini and A. Zaffaroni, JHEP08, 064, arXiv:1604.03122 [hep-th]

  22. [30]

    We normalize them byx/(ex−1) = P m≥0Bmxm/m!, so thatB 2 = 1/6,B 4 =−1/30andB 6 = 1/42

  23. [31]

    Diamond and J

    F. Diamond and J. M. Shurman,A first course in mod- ular forms, Vol. 228 (Springer, 2005)

  24. [32]

    Paşol and A

    V. Paşol and A. A. Popa, Proceedings of the London Mathematical Society107, 713 (2013)

  25. [33]

    Drukker, M

    N. Drukker, M. Marino, and P. Putrov, JHEP11, 141, arXiv:1103.4844 [hep-th]

  26. [34]

    Bobev, S

    N. Bobev, S. Choi, J. Hong, and V. Reys, JHEP02, 027, arXiv:2210.15326 [hep-th]

  27. [35]

    Gopakumar and C

    R. Gopakumar and C. Vafa, arXiv e-prints (1998), arXiv:hep-th/9809187

  28. [36]

    Gopakumar and C

    R. Gopakumar and C. Vafa, arXiv e-prints (1998), arXiv:hep-th/9812127

  29. [37]

    Kallen and M

    J. Kallen and M. Marino, Annales Henri Poincare17, 1037 (2016), arXiv:1308.6485 [hep-th]

  30. [38]

    Grassi, Y

    A. Grassi, Y. Hatsuda, and M. Marino, Annales Henri Poincare17, 3177 (2016), arXiv:1410.3382 [hep-th]

  31. [39]

    Bhattacharya, S

    J. Bhattacharya, S. Bhattacharyya, S. Minwalla, and S. Raju, JHEP02, 064, arXiv:0801.1435 [hep-th]

  32. [41]

    Flajolet and B

    P. Flajolet and B. Salvy, Experimental Mathematics7, 15 (1998)

  33. [42]

    Sofo, Integral Transforms and Special Functions30, 978 (2019)

    A. Sofo, Integral Transforms and Special Functions30, 978 (2019). 7 Supplemental Material Constant-map integral: exact Euler reduction and nu- merical audit.—Fork∈Z >0 define Ik = Z ∞ 0 log(2 coshx) log 1−e −kx dx, Cint(k) =− k2ζ(3) 16π + 2k π Ik. (16) ThusC int(k)denotes the ...

  34. [3780]

    Thebλ-dependent piece is the binomial expansion of the shifted3/2-power

    Each term of (9) descends from one term of the parent. Thebλ-dependent piece is the binomial expansion of the shifted3/2-power. The constant comes from the con- stant map: rescalingy=kxin (6), the large-kexpan- sion oflog(2 cosh(y/k))and the moments R∞ 0 y2n log(1− e−y) dy=−(2...

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