REVIEW 3 major objections 6 minor 1 cited by
Comments on Minitwistors and the Celestial Supersphere
T0 review · 3 major / 6 minor · reviewed 2026-08-10 · deepseek-v4-flash
Pith's one-line read Minitwistor sigma models reproduce celestial MHV gluon and graviton amplitudes.
desk verdict The minitwistor reformulation of leaf amplitudes is a real step, but the sigma-model semiclassical reduction has a normalization problem that suppresses the determinant, so the central claim doesn't follow. 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 load-bearing objects are minitwistor wavefunctions $\hat f_{\Delta,w}$, defined as Mellin transforms of twistor wavefunctions and realized as cohomology classes in $\Omega^{0,1}(\mathbf{MT},\mathcal{O}(\Delta-w,-\Delta))$; they are the vertex-operator building blocks of the $\sigma$ model. The celestial RSVW identity, Eq. (45), is the distributional bridge that replaces an integral over projective superspace $\mathbb{RP}^{3|8}$ or $\mathbb{RP}^{3|16}$ by an integral over minitwistor lines $L(X)$; the celestial BMS identity, Eq. (34), is the $n$-fold Penrose-transform relation that converts products of bulk-to-boundary propagators into minitwistor integrals, making the Quillen determinant $\log\det(\bar\partial+\omega)$ into a generating functional. The action (196) with kinetic terms for the embedding fields and the fermionic system gives a semiclassical path integral whose saddle points are exactly the minitwistor superlines.
What would settle it
Compute the left and right sides of Eq. (45) for a concrete four-point configuration with explicit minitwistor wavefunctions and delta functions; any mismatch for generic boundary insertion points and conformal weights would falsify the identity. A simpler check is to evaluate one four-gluon leaf amplitude directly from Eq. (60) and compare it with the minitwistor-line integral in Eq. (69) after performing the $X$-integral.
Extended reading notes
Core claim
The paper's central claim is that the celestial RSVW identity, an $n$-fold distributional identity on minitwistor space, allows every tree-level MHV celestial leaf amplitude for gluons and gravitons to be written as a Fourier transform over minitwistor superspace, with the support of the Fourier-transformed amplitude localized to incidence curves that are minitwistor lines; hence the amplitude vanishes unless all insertion points lie on a common minitwistor line. The same wavefunctions satisfy a second identity, the celestial BMS identity, which is used to show that the Quillen-determinant functional $\int \log\det(\bar\partial+\omega)$ restricted to minitwistor superlines generates all MHV leaf amplitudes. The paper then constructs an action for a $\sigma$ model with worldsheet the celestial supersphere $\mathbb{CP}^{1|2}$ and target the minitwistor superspace $\mathbf{MT}^{2|\mathcal{N}}$, and shows that in the semiclassical limit the path integral localizes on embeddings of the celestial sphere as minitwistor superlines, with the fermionic determinant giving exactly the Quillen-determinant generating functional. Thus the semiclassical effective action reproduces the MHV gluonic and gravitational leaf amplitudes.
Load-bearing premise
The full $n$-point celestial RSVW identity, Eq. (45), is assumed to hold as a distributional identity; the paper sketches an induction but does not give a complete proof, and if the identity fails, the minitwistor-line representation of the leaf amplitudes and the generating functional built on it no longer follow.
Editorial extensions
If this is right
- MHV gluon and graviton celestial leaf amplitudes acquire a geometric meaning: they are supported only on configurations where all insertion points lie on a common minitwistor line, so the amplitudes vanish otherwise.
- The generating functional $\mathfrak{W}[\omega]=\int_{\mathbb{RP}^{3|2\mathcal{N}}} D^{3|2\mathcal{N}}X \, \log\det(\bar\partial+\omega)\big|_{L(X,\theta)}$ packages all tree-level MHV leaf amplitudes into one object.
- The sigma model gives a semiclassical path-integral realization of the supersymmetric celestial CFT proposal, with the worldsheet being the celestial supersphere and the target the minitwistor superspace.
- If the formalism is extended to the NMHV sector, celestial amplitudes should be expressible as integrals over moduli spaces of higher-degree curves in minitwistor space, as the paper suggests.
Reading between the lines
- A rigorous proof of the $n$-fold celestial RSVW identity, rather than the sketched induction, would put the whole construction on solid ground; the identity is strong enough that it could be checked numerically for four points.
- The same Fourier-transform structure may transfer to other bulk geometries: any space whose twistor space admits a minitwistor quotient with the same incidence geometry would have a celestial CFT of this type.
- The semiclassical limitation suggests the sigma model is an effective description; understanding the anomalies that block full quantization could connect loop corrections to the model, possibly along the lines of celestial Liouville theory.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper continues the author's program of deriving aspects of celestial holography from string theory. It proposes a reformulation of tree-level MHV celestial leaf amplitudes for gluons in N=4 SYM and gravitons in N=8 supergravity as integrals over the moduli space of minitwistor lines, using minitwistor wavefunctions defined as cohomology classes on the minitwistor space MT. It also constructs a generating functional for these amplitudes via the Quillen determinant line bundle, extending the Boels-Mason-Skinner approach, and proposes supersymmetric celestial CFTs as sigma models on the celestial supersphere CP^{1|2} with target space MT^{2|N}. The central claim is that the semiclassical effective action of these sigma models reproduces the gluonic and gravitational MHV leaf amplitudes.
Significance. If the construction is correct, it would provide a concrete realization of Tropper's supersymmetric celestial CFT framework and forge a new link between celestial holography and twistorial string-theoretic methods. The paper contains explicit integral formulas, a clear identification of minitwistor wavefunctions, and a proposed action for the sigma model, building on prior work by Bu and Seet and by Boels, Mason, and Skinner. However, the verification is incomplete: the critical n-fold identities are only sketched, and the semiclassical reduction of the sigma model contains a normalization inconsistency that invalidates the claimed result as written.
major comments (3)
- [V.D.2, Eqs. (196)-(201)] The semiclassical effective action W defined in Eq. (200) with the action I in Eq. (196) cannot equal ∫ log det(∂ + ω) as claimed. For a free fermion, ∫ dψ d\barψ exp(-b \barψ D ψ) = b det D up to sign, so its contribution to -b log Z is -b log(b det D), which vanishes in the limit b→0+. The bosonic sector, with action of order 1/b, contributes its on-shell value at O(1). Therefore W would be the on-shell bosonic action, not the chiral determinant. The paper asserts that the fermionic path integral 'results in the chiral determinant' and that W becomes the generating functional, but no computation is provided. This is a load-bearing error for the sigma-model claim.
- [II.C.2-II.C.3, Eqs. (34) and (45)] The celestial BMS identity (34) and the celestial RSVW identity (45) are central bridges that convert leaf amplitude integrals into integrals over minitwistor lines and underpin the generating functional construction. Both are justified only by an 'inductive argument' or 'direct evaluation' with no detailed proof. Eq. (45) is a nontrivial distributional identity on minitwistor space; without a proof or a precise statement of its domain of validity, the reformulation of the amplitudes and the generating functionals built on it are not established.
- [III.C, Eqs. (76)-(78)] The Penrose transform of the background potential ω in Eq. (76) is written as K_Δ(X;z,\bar z), but according to Eq. (33) the transform of F_Δ alone gives C(Δ)/⟨z|X|\bar z]^Δ; the factor |X|^Δ is required to obtain K_Δ. The BMS identity (34) also includes |X|^{Δ_i} on its left-hand side. The generating functional expansion in Eqs. (77)-(78) therefore omits these factors and does not follow as written. The same issue appears in the gravitational generating functional in Eqs. (145)-(147).
minor comments (6)
- [III.B.1 and IV.B.2, Eqs. (59), (119)] The notation '+ (z̄_i → i z̄_i)' (and similarly in Eq. (119)) is not explained; please define this shorthand explicitly.
- [IV.D.2, Eq. (141)] In the definition of L(X,θ), the set is written with Z^I ∈ MT^{2|4}, but for the N=8 supergravity case it should be MT^{2|8}.
- [IV.A and IV.B, Eqs. (108)-(112)] The vertex operators \hat G_i, \hat H_i, U_i, and V_i mix the notations χ and \hatχ; the two-point function in Eq. (90) uses χ, while the operators use \hatχ, which is confusing.
- [IV.C, Eq. (124)] Eq. (124) contains unbalanced parentheses and an unclear product/sum structure; please rewrite it with proper grouping.
- [General] The manuscript contains numerous typos and grammatical errors, e.g., 'aproach' in the Introduction and 'seem' for 'seen' in Section V.C.3.
- [V.D.1, Eqs. (195)-(196)] The action in Eq. (196) is written as an integral over \tilde L(X,θ), but \tilde L is not defined in the text; clarify its relation to L(X,θ).
Circularity Check
No significant circularity: the sigma-model claim is a path-integral computation (with normalization gaps) and the generating functional construction is a legitimate application of the stated BMS/RSVW identities.
full rationale
I find no circular step in the derivation chain. The minitwistor wavefunctions are defined independently by Mellin transform (Eqs. 21-25), and the BMS/RSVW identities (Eqs. 34 and 45) are stated as integral identities derived from the Penrose transform; their RHS is the same bulk-to-boundary propagator K that defines leaf amplitudes, so substituting the identity into Eq. (60) is a change of representation rather than a self-referential definition. The generating functional Psi[omega] = integral log det(dbar + omega) is expanded via the standard Quillen determinant expansion, and the functional derivative in Eq. (80) reproduces the leaf amplitude as a computation, not by fitting. The sigma-model action in Eq. (196) is engineered so that the fermionic sector yields the chiral determinant, and Eq. (201) is asserted as the semiclassical result; this is a proposed derivation rather than a circular definition. The main issues are the lack of a detailed proof of the n-fold RSVW identity in Eq. (45) and an apparent b-normalization inconsistency in Eqs. (196)-(201) that would suppress the fermion determinant; these are correctness risks, not circularity. The author's self-citations are programmatic and not load-bearing, and no parameter is fitted and renamed as a prediction.
Assumptions & free parameters
free parameters (1)
- sigma-model coupling b =
not fixed
assumptions (5)
- ad hoc to paper The n-fold celestial Boels-Mason-Skinner identity, Eq. (34), holds as an identity of Penrose transforms on minitwistor space.
- ad hoc to paper The n-fold celestial RSVW identity, Eq. (45), holds as a distributional identity on MT.
- domain assumption Analytic continuations of Dirac delta functions and distributional forms, including delta(z) = (1/2 pi i) dbar z^{-1}, define valid distributions on minitwistor space.
- domain assumption The path integral over the fermionic system (psi, psibar) equals the chiral determinant Tr log(dbar + omega), and the saddle-point approximation localizes the full path integral onto incidence relations.
- domain assumption The minitwistor superspace MT^{2|N} is the trivial superbundle MT x CP^{0|N}, and the celestial supersphere CP^{1|2} is the correct worldsheet for the proposed sigma model.
Cite this review
Pith. "Pith review of Comments on Minitwistors and the Celestial Supersphere." pith.science (2026). https://pith.science/paper/J2YQCU4X
@misc{pith2026250109371,
author = {Pith},
title = {Pith review of: Comments on Minitwistors and the Celestial Supersphere},
year = {2026},
howpublished = {\url{https://pith.science/paper/J2YQCU4X}},
note = {Machine review of arXiv:2501.09371}
}
abstract
Continuing our program of deriving aspects of celestial holography from string theory, we extend the Roiban-Spradlin-Volovich-Witten (RSVW) formalism to celestial amplitudes. We reformulate the tree-level maximally-helicity-violating (MHV) celestial leaf amplitudes for gluons in $\mathcal{N}=4$ supersymmetric Yang-Mills (SYM) theory and for gravitons in $\mathcal{N}=8$ Supergravity in terms of minitwistor wavefunctions. These are defined as representatives of cohomology classes on the minitwistor space $\mathbf{MT}$, associated to the three-dimensional Euclidean anti-de Sitter space. In this framework, celestial leaf amplitudes are expressed as integrals over the moduli space of minitwistor lines. We construct a minitwistor generating functional for MHV leaf amplitudes using the Quillen determinant line bundle, extending the approach originally developed by Boels, Mason and Skinner. Building on this formalism, we propose supersymmetric celestial conformal field theories (CFTs) as $\sigma$-models, where the worldsheet is given by the celestial supersphere $\mathbf{CP}^{1|2}$, and the target space is the minitwistor superspace $\mathbf{MT}^{2|\mathcal{N}}$. We demonstrate that the semiclassical effective action of these $\sigma$-models reproduces the MHV gluonic and gravitational leaf amplitudes in $\mathcal{N}=4$ SYM theory and $\mathcal{N}=8$ Supergravity. This construction provides a concrete realisation of the supersymmetric celestial CFT framework recently introduced by Tropper (2024).
Forward citations
Cited by 1 Pith paper
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A Supersymmetric $w_{1+\infty}$ Symmetry, the Extended Supergravity and the Celestial Holography
An N=4 supersymmetric w_{1+∞} algebra at λ=1/4 is proposed as the celestial soft current algebra of N=4 SO(4) supergravity, with truncations covering N=2,3 and matter-coupled cases.
Reference graph
Works this paper leans on
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[1]
vertex operators
CP1 Fermionic Doublet The factorisation procedure to be employed in this section i s based on the method developed by Nair [75]. In this formalism, tree-level MHV gravitation al scattering amplitudes are expressed in terms of a correlator of “vertex operators.” These operat ors are constructed with the aid of an auxiliary fermionic doublet ( ˆχ, ˆχ †) defi...
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[2]
vertex operators
BGKn Formula from CP1 Correlators The graviton “vertex operators” are defined as: Gi := exp ( i ⟨νi|x |νi] ) χ † νiχ νi, Hi := [ νi| (−i∂ ) |ω⟩ νi ·ω exp ( i ⟨νi|x |ν i] ) . (91) In the above expressions, (∂ )A ˙A := (σµ)A ˙A ∂ ∂xµ and ωA := ( i 2π ) 1/2 (ω, −1 ) is an auxiliary two- component spinor parametrised by [ω] ∈ CP1. This spinor serves as a refer...
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[3]
(96) explicitly in terms of the graviton frequencies si and the normalised spinor basis {zA i ,zi ˙A}
Frequency Dependency To proceed with our aim of performing the Mellin transform of Mn, thereby yielding the corres- ponding celestial amplitude, it is necessary to re-express Eq. (96) explicitly in terms of the graviton frequencies si and the normalised spinor basis {zA i ,zi ˙A}. This reformulation takes the form: Mn = ( κ 2 ) n−2 (z1 ·z2)8 ˆ R4 d4x (2π)...
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[4]
dimensions,
N = 8 Supergravity The transition from Einstein’s gravity to N = 8 Supergravity is facilitated by adopting the on-shell superfield formalism, as reviewed in Wess and Bagger [43]. On-shell Superfield Expansion. This formalism introduces Grassmann-valued two-componen t spinors, denoted ηα A (1 ≤α ≤ 8) and normalised according to the relation: ˆ R0|2 d0|2η ηα ...
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[5]
23 We follow standard conventions in abstract index notation
Mellin Transform Let us first recall that the celestial superamplitude ˆMn (zi, ¯zi, ∆ i) for gravitons in N = 8 Su- pergravity is defined as the ε-regulated Mellin transform of the corresponding scatteri ng amplitude Mn (zi, ¯zi,s i), as follows: ˆMn (zi,zi, ∆ i) := n∏ i=1 ˆ R× + dsi si s∆ i i e−εsi Mn (zi,zi,s i), (105) where R× + denotes the multiplicati...
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[6]
integral
Gravitational Celestial Leaf Amplitudes To reformulate the graviton celestial amplitude as an integ ral over the moduli space of min- itwistor lines, we employ the formalism of leaf amplitudes. However, a technical complication immediately presents itself: the celestial wavefunctions φ2hi (x;zi,zi), which appear as multiplic- ative factors in the vertex o...
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[7]
Preliminaries: A Celestial Correlator LetO :=O[ωA, Pi, Ψ ∆ i] be an operator depending on the auxiliary spinor ωA, the weight-shifting operators Pi, and the minitwistor graviton wavefunctions Ψ ∆ i (Zi;zi, ¯zi). Define the expectation value of O over the auxiliary spinor and the fermionic doublet (χ,χ †) as: ⟨O⟩ω,n = ˛ Cn ⟨ωdω⟩ ⟨ω ⏐ ⏐O[ωA, Pi, Ψ ∆ i] ⏐ ⏐ω⟩...
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[8]
spacetime
Minitwistor Gravitational Background We now proceed to construct the generating functional. The fi rst step is to introduce the minitwistor gravitational background potential as a representative of a cohomology class: ω i ∈ D Λ [Hc] ⊗ Ω 0,1( MT2|8, O(−2, −∆) ) . (140) Recall that the minitwistor superline L (X,θ ) ⊂ MT2|8, associated with the point X ˆI = ...
Show all 122 references
-
[9]
boundary conditions
(158) These coordinates ωA are postulated to be projectively related to the minitwisto r coordinates λA through the relation: λA ≡ ωA ω1ω2 = κA 1 ω2 + κA 2 ω1 . (159) Within this trivialisation, the holomorphic function F ˙A (X,λ ), which determines the embedding map σX : CP1 ...
-
[10]
fermionic degrees of freedom
Projective Superspace We begin by observing that the minitwistor space MT is the space of oriented geodesics on the hyperboloid H + 3 . A model for the hyperbolic geometry of H + 3 can be derived from the projective geometry of the three-dimensional real projective space RP3, ...
-
[11]
fermionic di mensions
Minitwistor Superspace The minitwistor superspace MT2|N (associated with the hyperbolic geometry modelled on RP3|2N ) is constructed by extending the bosonic minitwistor space MT through the inclusion of Grassmann-odd coordinates that encode the “fermionic di mensions.” More p...
-
[12]
spacetime
Minitwistor Superlines In minitwistor superspace, the minitwistor lines are gener alised to superlines L (X,θ ), each associated with a “spacetime” point (XA ˙A,θ α A) ∈ RP3|2N . The incidence relation defining these supercurves is determined by sections of the projective spino...
-
[13]
Construction of the Action First Step: Dynamical Variables. To formulate a theory whose solutions to the equations of motion correspond to embeddings of the celestial sphere int o minitwistor superspace MT2|N , it suffices to specify the holomorphic sections F ˙A (X,θ ;λ) and Gα...
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[14]
Fermionic System We begin with the following physical motivations. First, th e generating functional ̥[ω ], derived in Subsection III C for N = 4 SYM theory and in Subsection IV D for N = 8 Supergravity, is expressed as an integral over projective superspace RP3|2N of the Quil...
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[15]
(196) yields the generating func tional ̥[ω ]
Semiclassical Analysis We turn now to the task of demonstrating that the semiclassic al effective action arising from the theory described by Eq. (196) yields the generating func tional ̥[ω ]. Prior to presenting the path-integral formulation of the eff ective action, we recall ...
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[16]
gauge tr ansformations
Hyperbolic Space from Projective Geometry Let the four-vectorX A ˙A be homogeneous coordinates on CP3, subject to the equivalence relation X A ˙A ∼a ·X A ˙A, where a is any non-zero complex scalar. A necessary and sufficient con dition for a set of components of a holomorphic me...
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[17]
Any such curve C is referred to as a minitwistor line or a Hitchin special curve
Minitwistor Space A minitwistor space 37 M is defined as any two-dimensional complex manifold containi ng a rational curve C (a holomorphic embedding of CP1 into M) with a normal bundle isomorphic to O (2). Any such curve C is referred to as a minitwistor line or a Hitchin spec...
1982
-
[18]
The Holomorphic V ector Bundle O (p,q ) − →MT In this subsection, we shall define the holomorphic vector bu ndle O (p,q ) − → MT which serves as the domain upon which the minitwistor Penrose tran sform is defined. We establish that this bundle can be identified with the infinite-d...
-
[19]
This formalism requires the analytic continuation of Minkowski spacetime R(1,3) from a Lorentzian (− + ++) to a Kleinian (− − ++) signature
Klein Space The leaf representation of celestial amplitudes is our main motivation for introduc ing multi-gluon and multi-graviton wavefunctions using minitwistor varia bles. This formalism requires the analytic continuation of Minkowski spacetime R(1,3) from a Lorentzian (− +...
-
[20]
The lowering and raising of spinor indices adhere to the sta ndard convention, according to which µA :=εABµB andνA =εABνB with εAB satisfying εACεCB =δA B
Spinor Algebra Employing the Van der Waerden formalism, as reviewed by Veblen [102] and Penrose and Rindler [103], the inner product of two undotted two-component spin ors, denoted µA andνA, is defined as: ⟨µν⟩ :=µ ·ν :=εABµAνB =µAνA, (B24) whereεAB is the Levi-Civita symbol, a...
-
[21]
Celestial Wavefunctions and the Leaf Amplitude Represen tation The leaf representation of celestial amplitudes, introduc ed by Melton, Sharma, and Strominger [58], arises from the consideration of the following integr al over spacetime: I (πi, ¯πi) := ˆ R(2, 2) d4X n∏ i=1 φ2hi...
- [22]
-
[23]
Bu and S
W. Bu and S. Seet, Journal of High Energy Physics 2023, 1 (2023)
2023
-
[24]
Kim and V
C. Kim and V. Nair, Physical Review D 55, 3851 (1997)
1997
-
[25]
Casali, W
E. Casali, W. Melton, and A. Strominger, Journal of High E nergy Physics 2022, 1 (2022)
2022
-
[26]
Melton, A
W. Melton, A. Sharma, A. Strominger, and T. Wang, arXiv pr eprint arXiv:2403.18896 (2024)
2024 arXiv
-
[27]
Guillemin, Contemp
V. Guillemin, Contemp. Math. 63, 135 (1987)
1987
-
[28]
Helgason et al
S. Helgason et al. , Integral geometry and Radon transforms , Vol. 1 (Springer, 2011)
2011
-
[29]
Helgason, Groups and geometric analysis: integral geometry, invariant d ifferential operators, and spherical functions , Vol
S. Helgason, Groups and geometric analysis: integral geometry, invariant d ifferential operators, and spherical functions , Vol. 83 (American Mathematical Society, 2022)
2022
-
[30]
Helgason, Geometric analysis on symmetric spaces , Vol
S. Helgason, Geometric analysis on symmetric spaces , Vol. 39 (American Mathematical Society, 2024)
2024
-
[31]
E. T. Quinto, F. Gonzalez, and J. G. Christensen, Geometric Analysis and Integral Geometry , Vol. 598 (American Mathematical Soc., 2013)
2013
-
[32]
Penrose, Journal of mathematical Physics 10, 38 (1969)
R. Penrose, Journal of mathematical Physics 10, 38 (1969)
1969
-
[33]
P. E. Jones, Minitwistors, Ph.D. thesis, University of Oxford (1984)
1984
-
[34]
Jones and K
P. Jones and K. Tod, Classical and Quantum Gravity 2, 565 (1985)
1985
-
[35]
N. J. Hitchin, Communications in Mathematical Physics 83, 579 (1982)
1982
-
[36]
Hitchin, Lecture Notes in Mathematics 970 (1982)
N. Hitchin, Lecture Notes in Mathematics 970 (1982)
1982
-
[37]
Honda and F
N. Honda and F. Nakata, Annals of Global Analysis and Geo metry 39, 293 (2011)
2011
-
[38]
Adamo, arXiv preprint arXiv:1712.02196 (2017)
T. Adamo, arXiv preprint arXiv:1712.02196 (2017)
2017 arXiv
-
[39]
Atiyah, M
M. Atiyah, M. Dunajski, and L. J. Mason, Proceedings of t he Royal Society A: Mathematical, Physical and Engineering Sciences 473, 20170530 (2017)
2017
-
[40]
Witten, Communications in Mathematical Physics 252, 189 (2004)
E. Witten, Communications in Mathematical Physics 252, 189 (2004)
2004
-
[41]
Adamo, D
T. Adamo, D. Skinner, and J. Williams, Journal of High En ergy Physics 2016, 1 (2016)
2016
-
[42]
Forster, Lectures on Riemann Surfaces , 96 (1981)
O. Forster, Lectures on Riemann Surfaces , 96 (1981)
1981
-
[43]
Teschner, arXiv preprint hep-th/9705214 (1997)
J. Teschner, arXiv preprint hep-th/9705214 (1997)
1997 arXiv
-
[44]
Teschner, Nuclear Physics B 546, 369 (1999)
J. Teschner, Nuclear Physics B 546, 369 (1999). 39 The Green’s function G∆ may be obtained by the analytic continuation of the correspo nding AdS3 propagator, as studied by Costa, Gonçalves, and Penedones [30] and reviewe d by Penedones [31]. Alternatively, G∆ may also be deri...
1999
-
[45]
Teschner, Nuclear Physics B 546, 390 (1999)
J. Teschner, Nuclear Physics B 546, 390 (1999)
1999
-
[46]
Teschner, Nuclear Physics B 571, 555 (2000)
J. Teschner, Nuclear Physics B 571, 555 (2000)
2000
-
[47]
Ribault and J
S. Ribault and J. Teschner, Journal of High Energy Physi cs 2005, 014 (2005)
2005
-
[48]
Boels, L
R. Boels, L. Mason, and D. Skinner, Physics Letters B 648, 90 (2007)
2007
-
[49]
Generalized f unctions vol. 5, integral geometry and rep- resentation theory, 1966,
I. Gelfand, M. Graev, and N. Y. Vilenkin, “Generalized f unctions vol. 5, integral geometry and rep- resentation theory, 1966,” (1966)
1966
-
[50]
M. S. Costa, V. Gonçalves, and J. Penedones, Journal of H igh Energy Physics 2014, 1 (2014)
2014
-
[51]
Penedones, in New Frontiers in Fields and Strings: TASI 2015 Proceedings of t he 2015 Theoretical Advanced Study Institute in Elementary Particle Physics (World Scientific, 2017) pp
J. Penedones, in New Frontiers in Fields and Strings: TASI 2015 Proceedings of t he 2015 Theoretical Advanced Study Institute in Elementary Particle Physics (World Scientific, 2017) pp. 75–136
2015
-
[52]
De Rham, Differentiable manifolds: forms, currents, harmonic forms , Vol
G. De Rham, Differentiable manifolds: forms, currents, harmonic forms , Vol. 266 (Springer Science & Business Media, 2012)
2012
-
[53]
Schwartz, Journal d?Analyse Mathématique 4, 88 (1954)
L. Schwartz, Journal d?Analyse Mathématique 4, 88 (1954)
1954
-
[54]
Schwartz, in Annales de l’institut Fourier , Vol
L. Schwartz, in Annales de l’institut Fourier , Vol. 7 (1957) pp. 1–141
1957
-
[55]
Schwartz, in Annales de l’institut Fourier , Vol
L. Schwartz, in Annales de l’institut Fourier , Vol. 8 (1958) pp. 1–209
1958
-
[56]
S. J. Parke and T. R. Taylor, Physical Review Letters 56, 2459 (1986)
1986
-
[57]
F. A. Berends and W. Giele, Nuclear Physics B 306, 759 (1988)
1988
-
[58]
Elvang and Y.-t
H. Elvang and Y.-t. Huang, arXiv preprint arXiv:1308.1 697 (2013)
2013
-
[59]
Badger, J
S. Badger, J. Henn, J. C. Plefka, and S. Zoia, Scattering Amplitudes in Quantum Field Theory (Springer Nature, 2024)
2024
-
[60]
M. T. Grisaru and H. Pendleton, Nuclear Physics B 124, 81 (1977)
1977
-
[61]
Brink, J
L. Brink, J. H. Schwarz, and J. Scherk, Nuclear Physics B 121, 77 (1977)
1977
-
[62]
A. C. Ferber, Supertwistors and conformal supersymmetry. , Ph.D. thesis, The University of Chicago (1977)
1977
-
[63]
Wess and J
J. Wess and J. Bagger, Supersymmetry and Supergravity: Revised Edition, Vol. 25 (Princeton university press, 2020)
2020
-
[64]
F. A. Berezin, Introduction to superanalysis, Vol. 9 (Springer Science & Business Media, 2013)
2013
-
[65]
B. S. DeWitt, Supermanifolds (Cambridge University Press, 1992)
1992
-
[66]
Y. I. Manin, Gauge Field Theory and Complex Geometry , 18 1 (1997)
1997
-
[67]
Pasterski and S.-H
S. Pasterski and S.-H. Shao, Physical Review D 96, 065022 (2017)
2017
-
[68]
Pasterski, S.-H
S. Pasterski, S.-H. Shao, and A. Strominger, Physical R eview D 96, 085006 (2017)
2017
-
[69]
Pasterski, S.-H
S. Pasterski, S.-H. Shao, and A. Strominger, Physical R eview D 96, 065026 (2017)
2017
-
[70]
Arkani-Hamed, M
N. Arkani-Hamed, M. Pate, A.-M. Raclariu, and A. Stromi nger, Journal of High Energy Physics 2021, 1 (2021)
2021
-
[71]
Banerjee, S
S. Banerjee, S. Ghosh, P. Pandey, and A. P. Saha, Journal of High Energy Physics 2020, 1 (2020)
2020
-
[72]
Banerjee and S
S. Banerjee and S. Ghosh, Journal of High Energy Physics 2021, 1 (2021)
2021
-
[73]
Pasterski, The European Physical Journal C 81, 1062 (2021)
S. Pasterski, The European Physical Journal C 81, 1062 (2021)
2021
-
[74]
Raclariu, arXiv preprint arXiv:2107.02075 (202 1)
A.-M. Raclariu, arXiv preprint arXiv:2107.02075 (202 1). 61
-
[75]
Strominger, Lectures on the infrared structure of gravity and gauge theory (Princeton University Press, 2018)
A. Strominger, Lectures on the infrared structure of gravity and gauge theory (Princeton University Press, 2018)
2018
-
[76]
P. B. Aneesh, G. Compère, L. Pipolo de Gioia, I. Mol, and B . Swidler, SciPost Physics Lecture Notes , 047 (2022)
2022
-
[77]
Pasterski, arXiv preprint arXiv:2310.04932 (2023)
S. Pasterski, arXiv preprint arXiv:2310.04932 (2023)
2023 arXiv
-
[78]
Melton, A
W. Melton, A. Sharma, and A. Strominger, arXiv preprint arXiv:2312.07820 (2023)
2023 arXiv
-
[79]
I. M. Gel_fand, S. G. Gindikin, and M. I. Graev, Selected topics in integral geometry , Vol. 220 (American Mathematical Soc., 2003)
2003
-
[80]
Sämann, Advances in Mathematical Physics 2009, 784215 (2009)
C. Sämann, Advances in Mathematical Physics 2009, 784215 (2009)
2009
-
[81]
Rogers, Supermanifolds: theory and applications (World Scientific, 2007)
A. Rogers, Supermanifolds: theory and applications (World Scientific, 2007)
2007
-
[82]
Movshev, arXiv preprint math/0611061 (2006)
M. Movshev, arXiv preprint math/0611061 (2006)
2006 arXiv
-
[83]
Adamo and M
T. Adamo and M. Groechenig, (2013)
2013
-
[84]
Quillen, Functional Analysis and Its Applications 19, 31 (1985)
D. Quillen, Functional Analysis and Its Applications 19, 31 (1985)
1985
-
[85]
Biswas and G
I. Biswas and G. Schumacher, Geometric and Functional A nalysis 9, 226 (1999)
1999
-
[86]
Brylinski, in Advances in geometry (Springer, 1999) pp
J.-L. Brylinski, in Advances in geometry (Springer, 1999) pp. 107–146
1999
-
[87]
D. S. Freed, Mathematical aspects of string theory 1, 189 (1987)
1987
-
[89]
Mason and D
L. Mason and D. Skinner, Communications in mathematica l physics 294, 827 (2010)
2010
-
[90]
Mason and D
L. Mason and D. Skinner, Journal of High Energy Physics 2010, 1 (2010)
2010
-
[91]
Bullimore, L
M. Bullimore, L. Mason, and D. Skinner, Journal of High E nergy Physics 2010, 1 (2010)
2010
-
[92]
F. A. Berends, W. Giele, and H. Kuijf, Physics Letters B 211, 91 (1988)
1988
-
[93]
Miller, arXiv preprint arXiv:2408.11139 (2024)
N. Miller, arXiv preprint arXiv:2408.11139 (2024)
2024
-
[94]
Nair, Physical Review D?Particles, Fields, Gravita tion, and Cosmology 71, 121701 (2005)
V. Nair, Physical Review D?Particles, Fields, Gravita tion, and Cosmology 71, 121701 (2005)
2005
-
[95]
Abou-Zeid, C
M. Abou-Zeid, C. M. Hull, and L. J. Mason, Communication s in mathematical physics 282, 519 (2008)
2008
-
[96]
Adamo and L
T. Adamo and L. Mason, Classical and Quantum Gravity 30, 075020 (2013)
2013
-
[97]
Mason and D
L. Mason and D. Skinner, Journal of High Energy Physics 2014, 1 (2014)
2014
-
[98]
D. A. Leites, Russian Mathematical Surveys 35, 1 (1980)
1980
-
[99]
Geyer, A
Y. Geyer, A. E. Lipstein, and L. Mason, Physical review l etters 113, 081602 (2014)
2014
-
[100]
Geyer, A
Y. Geyer, A. E. Lipstein, and L. Mason, Classical and Qua ntum Gravity 32, 055003 (2015)
2015
-
[101]
Geyer and L
Y. Geyer and L. Mason, Journal of Physics A: Mathematica l and Theoretical 55, 443007 (2022)
2022
-
[102]
Roiban, M
R. Roiban, M. Spradlin, and A. Volovich, Journal of High Energy Physics 2004, 012 (2004)
2004
-
[103]
Wolf, On Supertwistor geometry and integrability in super gauge the ory, Other thesis (2006), arXiv:hep-th/0611013
M. Wolf, On Supertwistor geometry and integrability in super gauge the ory, Other thesis (2006), arXiv:hep-th/0611013
2006 arXiv
-
[104]
Berkovits, Physical review letters 93, 011601 (2004)
N. Berkovits, Physical review letters 93, 011601 (2004)
2004
- [105]
-
[106]
Sharma, Twistor sigma models , Ph.D
A. Sharma, Twistor sigma models , Ph.D. thesis, University of Oxford (2022)
2022
-
[107]
Chiou, O
D.-W. Chiou, O. J. Ganor, Y. P. Hong, B. S. Kim, and I. Mitr a, Physical Review D?Particles, Fields, Gravitation, and Cosmology 71, 125016 (2005)
2005
-
[108]
Sämann, arXiv preprint hep-th/0603098 (2006)
C. Sämann, arXiv preprint hep-th/0603098 (2006)
2006 arXiv
-
[109]
Dunajski, Journal of Physics A: Mathematical and The oretical 42, 404004 (2009)
M. Dunajski, Journal of Physics A: Mathematical and The oretical 42, 404004 (2009)
2009
-
[110]
Adamo, D
T. Adamo, D. Skinner, and J. Williams, Journal of Mathem atical Physics 59 (2018)
2018
-
[111]
Schwinger, Physical Review 152, 1219 (1966)
J. Schwinger, Physical Review 152, 1219 (1966)
1966
-
[112]
Nair, Notes for lectures at BUSSTEPP (2005)
V. Nair, Notes for lectures at BUSSTEPP (2005)
2005
-
[113]
Mol, arXiv preprint arXiv:2409.05936 (2024)
I. Mol, arXiv preprint arXiv:2409.05936 (2024)
2024 arXiv
-
[114]
Kobayashi and K
S. Kobayashi and K. Nomizu, Foundations of differential geometry, volume 2 , Vol. 61 (John Wiley & Sons, 1996)
1996
-
[115]
Kodaira, Proceedings of the National Academy of Scie nces 50, 218 (1963)
K. Kodaira, Proceedings of the National Academy of Scie nces 50, 218 (1963)
1963
-
[116]
Barrett, G
J. Barrett, G. Gibbons, M. Perry, C. Pope, and P. Ruback, International Journal of Modern Physics A 9, 1457 (1994)
1994
-
[117]
Bhattacharjee and C
B. Bhattacharjee and C. Krishnan, Physical Review D 106, 106018 (2022)
2022
-
[118]
Crawley, A
E. Crawley, A. Guevara, N. Miller, and A. Strominger, Jo urnal of High Energy Physics 2022, 1 (2022)
2022
-
[119]
Y.-K. E. Cheung, Y. Oz, and Z. Yin, Journal of High Energ y Physics 2003, 026 (2003)
2003
- [120]
-
[121]
Veblen, Proceedings of the National Academy of Scie nces 19, 462 (1933)
O. Veblen, Proceedings of the National Academy of Scie nces 19, 462 (1933)
1933
-
[122]
Penrose and W
R. Penrose and W. Rindler, Spinors and space-time , Vol. 1 (Cambridge university press, 1984)
1984
-
[123]
Donnay, S
L. Donnay, S. Pasterski, and A. Puhm, Journal of High En ergy Physics 2020, 1 (2020)
2020
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