REVIEW 3 major objections 6 minor 108 references
Form factors from string amplitudes
T0 review · 3 major / 6 minor · reviewed 2026-08-16 · deepseek-v4-flash
Pith's one-line read The paper constructs a stringy disk amplitude whose α′→0 limit reproduces tree-level scalar and gluon form factors and exposes factorization, soft limits, a 2-split, and a new amplitude relation.
desk verdict Promising new stringy construction for form factors with a real 7-point check, but the off-shell kinematic extension and the monodromy expansion that underpins the field-theory limit are assumed rather than proven. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central object is the integral (2) over the disk or upper half-plane, with measure $d\mu_{n;0}=\int_\Gamma \prod_i dz_i/\mathrm{vol}(SL(2,\mathbb{R}))\int_{H^+} dz_0 d\bar z_0/(z_0-\bar z_0)^2$ and the off-shell Koba-Nielsen factor. The machinery works because the modified contractions $V_i$ encode the off-shell momentum through the $p_i\cdot q$ terms, while puncture pinching produces the massless poles, $q\to0$ decouples the closed-string insertion to yield string amplitudes, and the kinematic constraints $s_{a,b}=s_{a,q}=0$ split the integrand into two disjoint worldsheet parts, giving the 2-split. The same integrand, after contour deforming $z_0,\bar z_0$ to the boundary, becomes a sum of $(n+2)$-point open-string integrands, which is what produces the amplitude-expansion relation.
What would settle it
Take the $n=4$ scalar stringy form factor at fixed nonzero $q^2$, evaluate the integral (2) numerically, and extract the residue at $s_{1,2}=0$; factorization (11) requires the residue to equal $A_3^{\phi^3}(1,2,I)\,F_3^{\phi^3}(-I,3,4;q)$, so a mismatch, or any divergence of the $z_0$ integration that is not cured by a regulator, would show the model does not reproduce field-theory form factors.
Extended reading notes
Core claim
The core discovery is the construction of the stringy form factor as the disk integral $\mathcal{F}^O_n(1,\ldots,n;q)=\int d\mu_{n;0}\,I^O_n\,\mathrm{KN}(1,\ldots,n;q)$, where $n$ open-string states sit on the boundary, one closed-string vertex sits in the bulk, and the Koba-Nielsen factor is extended by $p_i\cdot q$ and $q^2$ couplings so that the closed string carries the off-shell momentum. The integrands for the two Lagrangian operators are the Parke-Taylor factor and the $V/W$ contraction product, respectively, with the closed-string current $J^a(z_0)J^a(\bar z_0)$ providing the $1/(z_0-\bar z_0)^2$ factor that carries the off-shell datum. The paper shows that in the $\alpha'\to0$ limit this integral reduces to the known field-theory form factors, derives the massless-pole factorization, derives the soft behavior $q\to0$, and identifies the new 2-split factorization under the kinematic constraints. In addition, by deforming the closed-string insertions to the real line and applying monodromy relations, it derives an expansion of the stringy form factor into $(n+2)$-point open-string amplitudes, whose field-theory limit is a new linear relation between form factors and Yang-Mills-scalar amplitudes.
Load-bearing premise
The load-bearing premise is that the off-shell kinematics can simply be grafted onto the disk amplitude: the map $2q_1\cdot q_2\to q^2$ and $2p_i\cdot q_1=2p_i\cdot q_2\to -p_i\cdot q$ is not realized by any choice of the metric matrix in the known open-closed disk amplitude, so the integral (2) is assumed to remain $SL(2,\mathbb{R})$-invariant and convergent for $q^2\neq0$.
Editorial extensions
If this is right
- If the model is correct, every tree-level form factor for these Lagrangian operators has a representation as one disk integral, so factorization identities and pole structures follow from worldsheet pinching rather than from diagram-by-diagram analysis.
- The field-theory relation (22) gives a concrete computational shortcut: an $n$-point form factor can be obtained from $2^{n-2}$ color-ordered $(n+2)$-point Yang-Mills-scalar amplitudes, a check the paper runs through seven points.
- The soft limit $q\to0$ is a diagnostic for which local operators are the theory's Lagrangian: the stringy form factor reduces to the string amplitude exactly when the operator is the Lagrangian, explaining why $\mathcal{L}_{\phi^3}$ and $\mathrm{Tr}(F^2)$ appear.
- The 2-split property is a new structural identity for form factors, parallel to the string and particle amplitude 2-split, and should imply zeros and factorization-near-zeros of form factors that were not previously visible.
- The construction is the tree-level seed for extensions: multiple closed-string insertions would describe multi-operator form factors, and higher-genus surfaces would give loop-level stringy form factors.
Reading between the lines
- An implicit and testable extension is to run the amplitude-expansion formula for operators other than the two Lagrangians; if the expansion survives only for operators whose integrand splits cleanly, it would classify which observables admit stringy UV completions.
- The footnote-57 caveat suggests the model's domain of validity is not fixed by the known disk amplitude; a direct check of $SL(2,\mathbb{R})$ invariance of (2) for arbitrary $q^2\ne0$ would either confirm the kinematics as a new stringy datum or identify a constraint on $q^2$.
- If 2-split extends to supersymmetric settings, the zero and factorization structure of supersymmetric form factors could inherit a geometric explanation parallel to the geometry of scattering amplitudes; this is my inference rather than a claim in the paper.
- The $\alpha'$-correction dictionary sketched in the outlook could be tested at next order: the subleading term of $\mathcal{F}^{\mathrm{Tr}(F^2)}$ should reproduce the known matrix element of $\mathrm{Tr}(F^3)$, providing a sharp check of the whole construction.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proposes a stringy completion of tree-level form factors, defining F^O_n(1,...,n;q) in Eq. (2) as a disk integral with n open-string vertex operators and one closed-string insertion carrying off-shell momentum q. It claims that in the field-theory limit alpha' -> 0 this integral reduces to the known field-theory form factor (Eq. (9)), and it uses the stringy representation to discuss factorization (Eq. (11)), soft behavior q -> 0 (Eq. (15)), a new 2-split property (Eqs. (17), (19)), and an expansion of the form factor into open-string amplitudes (Eqs. (21), (22)). The paper validates the construction with low-point examples in Eq. (10) and reports a numerical check of Eq. (22) up to 7 points using independent public codes.
Significance. If the central claim is established, this paper opens a genuinely new connection between string amplitudes and form factors, offering a UV-complete integrand that manifests factorization, soft behavior, and a 2-split structure, and it provides a practical amplitude-expansion formula for computing form factors. The paper is commendable for making no parameter fits and for testing the main expansion against public independent codes up to 7 points. The main weakness is that the off-shell continuation underlying Eq. (2) is not rigorously derived; the kinematic map in footnote 57 is admitted to lie outside the framework of [56], so the SL(2,R)-invariance, convergence, and monodromy expansion of the integral remain assumptions. Filling this gap is necessary before the field-theory-limit claim and its derived properties can be considered established.
major comments (3)
- [Footnote 57 and Eq. (21)] The kinematic map 2 q1·q2 -> q^2 and 2 p_i·q1 = 2 p_i·q2 -> -p_i·q is explicitly stated not to be realizable by any D matrix in [56]. The derivation of the monodromy expansion (21) in [56] relies on the D matrix to fix SL(2,R) weights and to control the contour deformation that produces the phase factors M(rho). Since Eq. (21) is the route to the field-theory limit (9) and to the 7-point check of Eq. (22), the validity of this expansion for q^2 != 0 is a load-bearing assumption. The manuscript should either prove SL(2,R)-invariance and convergence of Eq. (2) for general q^2, or provide an independent derivation of Eq. (21) that does not rely on the D-matrix framework of [56].
- [Soft limit: q -> 0] The argument for Eq. (15) states that the dz0 d bar z0 integral 'will be divergent when q -> 0' and that 'one can introduce a regulator to make the integral finite', but no regulator is specified and no independence of the regulator is shown. This matters because Eq. (15) is used to explain why the chosen operators are Lagrangian operators. Please provide an explicit regularization prescription and demonstrate that the q -> 0 limit of the stringy form factor reproduces the string amplitude, or alternatively state Eq. (15) as a conjecture with a precise limiting procedure.
- [2-split, Eqs. (17)-(19)] The 2-split for the Tr(F^2) stringy form factor is asserted rather than derived. The V_i objects in Eq. (6) contain explicit q-dependent terms, -epsilon_i·q/z_i,0 and -epsilon_i·q/z_i,bar0, which are absent in the bosonic string amplitude case treated in [68,69]. Although the conditions in Eq. (18) are expected to suppress these terms, the paper does not show that all mixed contributions vanish in the split limit, nor does it provide an explicit low-point check of Eq. (19). Please supply a proof sketch or a concrete example, such as n=4 or n=5, demonstrating the claimed split.
minor comments (6)
- [Eq. (3)] The measure contains '(z0,bar0)^2', which presumably means (z0 - bar z0)^2; please correct the notation.
- [Eq. (21) and surrounding text] The number of open string amplitudes contributing to the expansion is written as '2n-2' in the text; this should be 2^{n-2}, and the set of permutations rho in the sum should be defined explicitly rather than left to reference [25,56].
- [Eq. (22)] The proportionality constant in Eq. (22) is not specified. Since the relation is used to calculate form factors from amplitudes, please state how the normalization is fixed for general n, or provide the constant explicitly if it has a simple form.
- [Eq. (10)] The low-point limits in Eq. (10) are stated without derivation; a brief indication of how the integrals are evaluated, or a reference to a companion calculation, would improve verifiability.
- [Seven-point check] The numerical check 'up to 7-point' is reported without presenting the actual comparison. Please include explicit numerical results or a link to reproducible data so the claim can be verified.
- [Notation in Eqs. (6) and (8)] The notation for V_i, W_{i,j}, and C_{i,j} would be clearer if the dependence on alpha', epsilon_i, and the ordering of indices were stated explicitly in one place.
Circularity Check
No circular reduction: footnote 57 is a flagged gap, not a self-referential derivation.
full rationale
The paper's central claim is that the disk integral (2), with the chosen off-shell kinematics, reduces to the known field-theory form factor in the alpha' -> 0 limit. This is tested through explicit low-multiplicity evaluations, factorization checks, soft-limit arguments, and a 7-point numerical comparison against independent public codes for scattering amplitudes [82] and form factors [63]. No parameter is fitted from the target form factors, and the relation (22) is not defined in terms of the field-theory result it is meant to produce. The only self-citations are [68,69], used to justify the 2-split factorization of the Parke-Taylor and Koba-Nielsen factors; these are prior proofs by the same group, but they are not definitions of the present stringy form factor and the central field-theory limit is verified independently. The manuscript itself flags the most serious weakness in footnote 57: the kinematic map 2 q1·q2 -> q^2 and 2 p_i·q1 = 2 p_i·q2 -> -p_i·q cannot be realized by any D matrix in [56], so the SL(2,R) invariance, convergence for q^2 != 0, and the expansion (21) are assumed rather than derived from that reference. This is a genuine gap or correctness risk, but it is not a circular reduction: the claimed result is not equivalent to its inputs by construction. No circular step meets the quote-and-reduction standard, so the circularity burden is low.
Assumptions & free parameters
assumptions (4)
- ad hoc to paper The off-shell continuation of the disk amplitude defined by the map in footnote 57 (2 q1·q2 -> q^2, 2 p_i·q1 = 2 p_i·q2 -> -p_i·q) yields a well-defined, SL(2,R)-invariant string integral for q^2 != 0.
- domain assumption The contour deformation and Monodromy relations used to expand the stringy form factor into open-string amplitudes remain valid under the generalized kinematics of footnote 57.
- domain assumption The integrands I_n^{Lphi3} = PT(1,...,n) and I_n^{Tr(F^2)} built from V_i and W_{i,j} with the modified V_i correctly encode the operators Lphi3 and Tr(F^2) with off-shell momentum.
- domain assumption The 2-split factorization of the PT factor and KN factor for the stringy form factor follows from the proofs in [68,69].
Cite this review
Pith. "Pith review of Form factors from string amplitudes." pith.science (2026). https://pith.science/paper/IW5PH6JG
@misc{pith2026250415702,
author = {Pith},
title = {Pith review of: Form factors from string amplitudes},
year = {2026},
howpublished = {\url{https://pith.science/paper/IW5PH6JG}},
note = {Machine review of arXiv:2504.15702}
}
abstract
In this letter, we propose a stringy model for $n$-point tree-level form factor with the off-shell operator in the scalar and gluon theories, from the bosonic string disk amplitude: $n$ open string states and $1$ closed string state scatter on the disk. In the field-theory limit ($\alpha'\to0$), the stringy form factor reduces to the form factor, helps us to investigate the hidden properties of the field-theory form factors, manifest the factorization and soft behaviors, and uncover more non-trivial relations between form factors and scattering amplitudes.
Figures
Reference graph
Works this paper leans on
-
[56]
S. Stieberger and T. R. Taylor, Nucl. Phys. B 903, 104 (2016), arXiv:1510.01774 [hep-th]
arXiv 2016
-
[1]
Kawai, D
H. Kawai, D. C. Lewellen, and S. H. H. Tye, Nucl. Phys. B 269, 1 (1986)
1986
-
[2]
Bern and D
Z. Bern and D. A. Kosower, Phys. Rev. Lett. 66, 1669 (1991)
1991
-
[3]
Bern and D
Z. Bern and D. A. Kosower, Nucl. Phys. B 362, 389 (1991)
1991
-
[4]
Bern and D
Z. Bern and D. A. Kosower, Nucl. Phys. B 379, 451 (1992)
1992
-
[5]
Z. Bern, V. Del Duca, and C. R. Schmidt, Phys. Lett. B 445, 168 (1998), arXiv:hep-ph/9810409
arXiv 1998
-
[6]
Z. Bern, L. J. Dixon, M. Perelstein, and J. S. Rozowsky, Nucl. Phys. B 546, 423 (1999), arXiv:hep-th/9811140
arXiv 1999
- [7]
Show all 108 references
-
[8]
Cachazo, S
F. Cachazo, S. He, and E. Y. Yuan, Phys. Rev. D 90, 065001 (2014), arXiv:1306.6575 [hep-th]
2014 arXiv
-
[9]
Cachazo, S
F. Cachazo, S. He, and E. Y. Yuan, JHEP 07, 033 (2014), arXiv:1309.0885 [hep-th]
2014 arXiv
-
[10]
Cachazo, S
F. Cachazo, S. He, and E. Y. Yuan, Phys. Rev. Lett. 113, 171601 (2014), arXiv:1307.2199 [hep-th]
2014 arXiv
- [11]
-
[12]
S. He, F. Teng, and Y. Zhang, Phys. Rev. Lett. 122, 211603 (2019), arXiv:1812.03369 [hep-th]
2019 arXiv
-
[13]
S. He, F. Teng, and Y. Zhang, JHEP 09, 085 (2019), arXiv:1907.06041 [hep-th]
2019 arXiv
-
[14]
Bern, in Theoretical Advanced Study Institute (TASI 92): From Black Holes and Strings to Particles (1992) pp
Z. Bern, in Theoretical Advanced Study Institute (TASI 92): From Black Holes and Strings to Particles (1992) pp. 0471–536, arXiv:hep-ph/9304249
1992 arXiv
- [15]
-
[16]
J. M. Henn and J. C. Plefka, Scattering Amplitudes in Gauge Theories , Vol. 883 (Springer, Berlin, 2014)
2014
-
[17]
Travaglini et al
G. Travaglini et al. , J. Phys. A 55, 443001 (2022), arXiv:2203.13011 [hep-th]
2022 arXiv
-
[18]
C. R. Mafra and O. Schlotterer, Phys. Rept. 1020, 1 (2023), arXiv:2210.14241 [hep-th]
2023 arXiv
-
[19]
Berkovits, E
N. Berkovits, E. D’Hoker, M. B. Green, H. Johans- son, and O. Schlotterer, in Snowmass 2021 (2022) arXiv:2203.09099 [hep-th]
2022 arXiv
-
[20]
M. B. Green, J. H. Schwarz, and E. Witten, SUPER- STRING THEORY. VOL. 1: INTRODUCTION , Cam- bridge Monographs on Mathematical Physics (1988)
1988
- [21]
-
[22]
Stieberger and T
S. Stieberger and T. R. Taylor, Nucl. Phys. B 881, 269 (2014), arXiv:1401.1218 [hep-th]
2014 arXiv
-
[23]
Arkani-Hamed, S
N. Arkani-Hamed, S. He, and T. Lam, JHEP 02, 069 (2021), arXiv:1912.08707 [hep-th]
2021 arXiv
-
[24]
N. E. J. Bjerrum-Bohr, P. H. Damgaard, and P. Vanhove, Phys. Rev. Lett. 103, 161602 (2009), arXiv:0907.1425 [hep-th]
2009 arXiv
-
[25]
Stieberger, (2009), arXiv:0907.2211 [hep-th]
S. Stieberger, (2009), arXiv:0907.2211 [hep-th]
2009 arXiv
-
[26]
Kleiss and H
R. Kleiss and H. Kuijf, Nucl. Phys. B 312, 616 (1989)
1989
-
[27]
Z. Bern, J. J. M. Carrasco, and H. Johansson, Phys. Rev. D 78, 085011 (2008), arXiv:0805.3993 [hep-ph]
2008 arXiv
-
[28]
W. L. van Neerven, Z. Phys. C 30, 595 (1986)
1986
-
[29]
Maldacena and A
J. Maldacena and A. Zhiboedov, JHEP 11, 104 (2010), arXiv:1009.1139 [hep-th]
2010 arXiv
-
[30]
Brandhuber, B
A. Brandhuber, B. Spence, G. Travaglini, and G. Yang, JHEP 01, 134 (2011), arXiv:1011.1899 [hep-th]
2011 arXiv
-
[31]
L. V. Bork, D. I. Kazakov, and G. S. Vartanov, JHEP 02, 063 (2011), arXiv:1011.2440 [hep-th]
2011 arXiv
-
[32]
Brandhuber, O
A. Brandhuber, O. Gurdogan, R. Mooney, G. Travaglini, and G. Yang, JHEP 10, 046 (2011), arXiv:1107.5067 [hep-th]
2011 arXiv
-
[33]
Brandhuber, G
A. Brandhuber, G. Travaglini, and G. Yang, JHEP 05, 082 (2012), arXiv:1201.4170 [hep-th]
2012 arXiv
-
[34]
Brandhuber, B
A. Brandhuber, B. Penante, G. Travaglini, and C. Wen, JHEP 08, 100 (2014), arXiv:1406.1443 [hep-th]
2014 arXiv
-
[35]
R. H. Boels, B. A. Kniehl, O. V. Tarasov, and G. Yang, JHEP 02, 063 (2013), arXiv:1211.7028 [hep-th]
2013 arXiv
-
[36]
L. V. Bork, JHEP 12, 111 (2014), arXiv:1407.5568 [hep- th]
2014 arXiv
-
[37]
Frassek, D
R. Frassek, D. Meidinger, D. Nandan, and M. Wilhelm, JHEP 01, 182 (2016), arXiv:1506.08192 [hep-th]
2016 arXiv
-
[38]
L. V. Bork and A. I. Onishchenko, JHEP12, 076 (2016), arXiv:1607.00503 [hep-th]
2016 arXiv
-
[39]
L. V. Bork and A. I. Onishchenko, JHEP04, 019 (2017), arXiv:1607.02320 [hep-th]
2017 arXiv
- [40]
-
[41]
L. V. Bork and A. I. Onishchenko, Phys. Rev. D 97, 126013 (2018), arXiv:1704.04758 [hep-th]
2018 arXiv
-
[42]
Bianchi, A
L. Bianchi, A. Brandhuber, R. Panerai, and G. Travaglini, JHEP 02, 182 (2019), arXiv:1812.09001 [hep-th]
2019 arXiv
-
[43]
Hidden structure in the form factors of N = 4 SYM,
D. Nandan and G. Yang, “Hidden structure in the form factors of N = 4 SYM,” (2018)
2018
-
[44]
Yang, Sci
G. Yang, Sci. China Phys. Mech. Astron. 63, 270001 (2020), arXiv:1912.11454 [hep-th]
2020 arXiv
- [45]
- [46]
-
[47]
To be precise, while we believe that a stringy model of form factors may exist on higher-genus Riemann sur- faces, we restrict our focus here to the simplest case: the disk topology, which corresponds to the tree-level
-
[48]
Some literature studies the one massive string ampli- tudes [105–108]
-
[49]
I. R. Klebanov and L. Thorlacius, Phys. Lett. B 371, 51 (1996), arXiv:hep-th/9510200
1996 arXiv
-
[50]
S. S. Gubser, A. Hashimoto, I. R. Klebanov, and J. M. Maldacena, Nucl. Phys. B 472, 231 (1996), arXiv:hep- th/9601057
1996
-
[51]
M. R. Garousi and R. C. Myers, Nucl. Phys. B 475, 193 (1996), arXiv:hep-th/9603194
1996 arXiv
-
[52]
Hashimoto and I
A. Hashimoto and I. R. Klebanov, Nucl. Phys. B Proc. Suppl. 55, 118 (1997), arXiv:hep-th/9611214
1997 arXiv
-
[53]
Hashimoto and I
A. Hashimoto and I. R. Klebanov, Phys. Lett. B 381, 437 (1996), arXiv:hep-th/9604065
1996 arXiv
-
[54]
Sen, Phys
A. Sen, Phys. Rev. D 68, 106003 (2003), arXiv:hep- th/0305011
2003
-
[55]
Sen, Phys
A. Sen, Phys. Rev. Lett. 91, 181601 (2003), arXiv:hep- th/0306137
2003
-
[57]
If we actually choose the metric matrix Dµν (the same notation as in [56]) to be a specific value, we cannot realize the kinematic condition for the form factor (q2̸= 0). Here we actually generalize the kinematics part of disk string amplitude to the stringy form factor in (2)...
-
[58]
Koba and H
Z. Koba and H. B. Nielsen, Nucl. Phys. B 10, 633 (1969)
1969
-
[59]
S. J. Parke and T. R. Taylor, Phys. Rev. Lett. 56, 2459 (1986)
1986
-
[60]
Broedel, O
J. Broedel, O. Schlotterer, and S. Stieberger, Fortsch. Phys. 61, 812 (2013), arXiv:1304.7267 [hep-th]
2013 arXiv
-
[61]
J. J. M. Carrasco, C. R. Mafra, and O. Schlotterer, JHEP 06, 093 (2017), arXiv:1608.02569 [hep-th]
2017 arXiv
-
[62]
J. J. M. Carrasco, C. R. Mafra, and O. Schlotterer, JHEP 08, 135 (2017), arXiv:1612.06446 [hep-th]
2017 arXiv
-
[63]
J. Dong, S. He, and G. Lin, JHEP 02, 076 (2023), arXiv:2208.00592 [hep-th]
2023 arXiv
-
[64]
J. Dong, S. He, and L. Hou, Phys. Rev. D 105, 105007 (2022), arXiv:2111.10525 [hep-th]
2022 arXiv
-
[65]
Q. Cao, J. Dong, S. He, and F. Zhu, Phys. Rev. D 111, 065015 (2025), arXiv:2412.19629 [hep-th]
2025 arXiv
-
[66]
Cachazo, L
F. Cachazo, L. Mason, and D. Skinner, SIGMA 10, 051 (2014), arXiv:1207.4712 [hep-th]
2014 arXiv
-
[67]
Baadsgaard, N
C. Baadsgaard, N. E. J. Bjerrum-Bohr, J. L. Bour- jaily, and P. H. Damgaard, JHEP 09, 129 (2015), arXiv:1506.06137 [hep-th]
2015 arXiv
-
[68]
Q. Cao, J. Dong, S. He, and C. Shi, (2024), arXiv:2403.08855 [hep-th]
2024 arXiv
-
[69]
Q. Cao, J. Dong, S. He, C. Shi, and F. Zhu, JHEP 09, 049 (2024), arXiv:2406.03838 [hep-th]
2024 arXiv
-
[70]
Arkani-Hamed, Q
N. Arkani-Hamed, Q. Cao, J. Dong, C. Figueiredo, and S. He, (2023), arXiv:2312.16282 [hep-th]
2023 arXiv
- [71]
-
[72]
Zhou, JHEP 03, 154 (2025), arXiv:2411.07944 [hep- th]
K. Zhou, JHEP 03, 154 (2025), arXiv:2411.07944 [hep- th]
2025 arXiv
-
[73]
Cachazo, N
F. Cachazo, N. Early, and B. Gim´ enez Umbert, JHEP 08, 252 (2022), arXiv:2112.14191 [hep-th]
2022 arXiv
- [74]
-
[75]
Zhang, (2024), arXiv:2406.08969 [hep-th]
Y. Zhang, (2024), arXiv:2406.08969 [hep-th]
2024
-
[76]
Zhang, JHEP 02, 074 (2025), arXiv:2412.15198 [hep- th]
Y. Zhang, JHEP 02, 074 (2025), arXiv:2412.15198 [hep- th]
2025 arXiv
-
[77]
Gim´ enez Umbert and B
B. Gim´ enez Umbert and B. Sturmfels, (2025), arXiv:2501.10805 [hep-th]
2025 arXiv
-
[78]
One of the subset A or B can be empty
-
[79]
See the ref [25, 56] for the detailed derivation and dis- cussion
-
[80]
Cachazo, S
F. Cachazo, S. He, and E. Y. Yuan, JHEP 07, 149 (2015), arXiv:1412.3479 [hep-th]
2015 arXiv
-
[81]
Cheung, C.-H
C. Cheung, C.-H. Shen, and C. Wen, JHEP 02, 095 (2018), arXiv:1705.03025 [hep-th]
2018 arXiv
-
[82]
S. He, L. Hou, J. Tian, and Y. Zhang, JHEP 08, 118 (2021), [Erratum: JHEP 06, 037 (2022)], arXiv:2103.15810 [hep-th]
2021 arXiv
-
[83]
Ramond, Phys
P. Ramond, Phys. Rev. D 3, 2415 (1971)
1971
-
[84]
Neveu and J
A. Neveu and J. H. Schwarz, Nucl. Phys. B 31, 86 (1971)
1971
-
[85]
Berkovits, JHEP 04, 018 (2000), arXiv:hep- th/0001035
N. Berkovits, JHEP 04, 018 (2000), arXiv:hep- th/0001035
2000
-
[86]
Berkovits, JHEP 09, 047 (2004), arXiv:hep- th/0406055
N. Berkovits, JHEP 09, 047 (2004), arXiv:hep- th/0406055
2004
-
[87]
Berkovits, JHEP 10, 089 (2005), arXiv:hep- th/0509120
N. Berkovits, JHEP 10, 089 (2005), arXiv:hep- th/0509120
2005
-
[88]
O. T. Engelund and R. Roiban, JHEP 03, 172 (2013), arXiv:1209.0227 [hep-th]
2013 arXiv
- [89]
-
[90]
Ahmed, P
T. Ahmed, P. Banerjee, A. Chakraborty, P. K. Dhani, and V. Ravindran, Phys. Rev. D 102, 061701 (2020), arXiv:1911.11886 [hep-th]
2020 arXiv
-
[91]
Stieberger, (2021), arXiv:2105.06888 [hep-th]
S. Stieberger, (2021), arXiv:2105.06888 [hep-th]
2021 arXiv
-
[92]
Arkani-Hamed, H
N. Arkani-Hamed, H. Frost, G. Salvatori, P.-G. Pla- mondon, and H. Thomas, (2023), arXiv:2309.15913 [hep-th]
2023 arXiv
-
[93]
Arkani-Hamed, H
N. Arkani-Hamed, H. Frost, G. Salvatori, P.-G. Pla- mondon, and H. Thomas, (2023), arXiv:2311.09284 [hep-th]
2023 arXiv
-
[94]
Arkani-Hamed, Q
N. Arkani-Hamed, Q. Cao, J. Dong, C. Figueiredo, and S. He, (2023), arXiv:2401.00041 [hep-th]
2023 arXiv
-
[95]
Arkani-Hamed, Q
N. Arkani-Hamed, Q. Cao, J. Dong, C. Figueiredo, and S. He, (2024), arXiv:2401.05483 [hep-th]
2024 arXiv
-
[96]
Arkani-Hamed, C
N. Arkani-Hamed, C. Figueiredo, H. Frost, and G. Sal- vatori, (2024), arXiv:2402.06719 [hep-th]
2024 arXiv
-
[97]
Arkani-Hamed, Q
N. Arkani-Hamed, Q. Cao, J. Dong, C. Figueiredo, and S. He, (2024), arXiv:2408.11891 [hep-th]
2024 arXiv
-
[98]
Arkani-Hamed, C
N. Arkani-Hamed, C. Figueiredo, and G. N. Remmen, (2024), arXiv:2412.20639 [hep-th]
2024 arXiv
-
[99]
Arkani-Hamed, H
N. Arkani-Hamed, H. Frost, and G. Salvatori, (2024), arXiv:2412.21027 [hep-th]
2024 arXiv
-
[100]
S. De, A. Pokraka, M. Skowronek, M. Spradlin, and A. Volovich, JHEP 09, 160 (2024), arXiv:2406.04411 [hep-th]
2024 arXiv
- [101]
-
[102]
Arkani-Hamed, S
N. Arkani-Hamed, S. He, T. Lam, and H. Thomas, Phys. Rev. D 107, 066015 (2023), arXiv:1912.11764 [hep-th]
2023 arXiv
-
[103]
Arkani-Hamed, S
N. Arkani-Hamed, S. He, G. Salvatori, and H. Thomas, JHEP 11, 049 (2022), arXiv:1912.12948 [hep-th]
2022 arXiv
-
[104]
Lin and G
G. Lin and G. Yang, Phys. Rev. Lett. 129, 251601 (2022), arXiv:2111.12719 [hep-th]
2022 arXiv
-
[105]
Guillen, H
M. Guillen, H. Johansson, R. L. Jusinskas, and O. Schlotterer, Phys. Rev. Lett. 127, 051601 (2021), arXiv:2104.03314 [hep-th]
2021 arXiv
-
[106]
S. P. Kashyap, C. R. Mafra, M. Verma, and L. A. Ypanaque, (2023), arXiv:2311.12100 [hep-th]
2023 arXiv
-
[107]
S. P. Kashyap, C. R. Mafra, M. Verma, and L. Ypanaqu´ e, JHEP02, 215 (2025), arXiv:2407.02436 [hep-th]
2025 arXiv
-
[108]
C. R. Mafra, JHEP 11, 045 (2024), arXiv:2407.11849 [hep-th]
2024 arXiv
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