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Twistor space

Twistor space is a complex three-dimensional projective space, denoted ℂP³, introduced by Roger Penrose in 1967 as a geometric arena for reformulating the conformal structure of four-dimensional Minkowski space-time in terms of complex variables and null geodesics, or light rays.^[1] In this framework, points in twistor space correspond to pairs of spinors that encode lightlike directions, allowing space-time events to be represented as holomorphic curves within the twistor manifold.^[2] The construction draws on the Plücker-Klein correspondence, associating lines in projective space to points in a dual space, thereby prioritizing conformal invariance over the full metric of space-time.^[3] Penrose's twistor theory emerged from efforts to unify general relativity and quantum mechanics by incorporating complex geometry at a fundamental level, contrasting with the real-valued descriptions typical of classical space-time physics.^[4] Key developments include the Penrose transform, which maps cohomology classes of sheaves on twistor space to solutions of differential equations for massless fields, such as those governing photons and gravitons.^[2] This approach naturally encodes self-dual Yang-Mills fields and anti-self-dual gravitational instantons, facilitating exact solutions in gauge theories.^[3] Twistor space's chiral structure distinguishes left- and right-handed components of fields, providing tools for contour integrals that simplify representations of physical quantities like scattering amplitudes in quantum field theory.^[5] Since its inception, twistor theory has evolved beyond flat space-time to curved geometries and higher dimensions, with applications in string theory and integrable systems.^[4] Edward Witten's 2003 twistor-string theory extended the framework to incorporate both chiral sectors, yielding compact formulas for particle interaction probabilities and inspiring geometric objects like the amplituhedron.^[2] Ongoing research at institutions such as the University of Oxford explores twistor methods for computational efficiency in high-energy physics, underscoring its enduring influence on mathematical physics.^[5]

Introduction

Overview

Twistor space is a fundamental construct in mathematical physics, introduced as a complex manifold that provides a geometric framework for understanding spacetime and quantum phenomena. The non-projective twistor space T is isomorphic to \mathbb{C}^4, equipped with a Hermitian inner product of signature (2,2), while the projective twistor space PT, which is the primary space of interest, is isomorphic to the complex projective space \mathbb{CP}^3, a three-complex-dimensional manifold.^[6] At its core, twistor space encodes the geometry of Minkowski spacetime through holomorphic structures, where points in complexified Minkowski space correspond to complex lines in PT, and light rays (null geodesics) correspond to points in PT. This correspondence is inherently conformal invariant, preserving angles but not distances, which aligns with the causal structure of relativistic physics.^[7] The conceptual motivation for twistor space arises from the challenges in reconciling quantum mechanics with general relativity, proposing a shift from the real Lorentzian geometry of spacetime to complex holomorphic geometries that may facilitate quantization. Physically, it represents massless particles—such as photons or gravitons—as points in PT, with their associated fields manifesting as holomorphic hypersurfaces or cohomology classes therein.^[7] This framework, originating from Roger Penrose's work in 1967, has found applications in computing scattering amplitudes in quantum field theory.

Historical Development

Twistor space was introduced by Roger Penrose in his 1967 paper "Twistor Algebra," where he proposed it as a novel framework for incorporating quantum principles into general relativity, motivated by the geometry of null geodesics and the conformal compactness of spacetime. This approach aimed to represent spacetime points via lines in a complex projective space, emphasizing the role of light rays as fundamental entities in physical descriptions. The development of twistor theory drew significant early influences from Ivor Robinson's work on shear-free null geodesic congruences, known as Robinson congruences, explored in the early 1960s, which highlighted geometric structures in general relativity that aligned with Penrose's interests.^[8] Penrose's prior investigations into spinor methods and asymptotic structures in general relativity during the mid-1960s further shaped the theory, providing tools to handle the conformal infinity of spacetime and the causal structure of null directions. In the 1970s, Penrose and Richard Ward extended twistor methods to describe solutions of self-dual Yang-Mills equations through the Penrose-Ward transform, establishing a correspondence between holomorphic bundles on twistor space and anti-self-dual gauge fields on spacetime.^[9] During the 1980s and 1990s, twistor theory found prominent applications in the study of integrable systems, where it facilitated the analysis of nonlinear partial differential equations via holomorphic structures and cohomology on twistor spaces. A major revival occurred in 2003 with Edward Witten's formulation of twistor string theory, which embedded perturbative gauge theory amplitudes into a string theory on twistor space, bridging twistor geometry with modern quantum field theory computations.^[10] In the 2010s, Freddy Cachazo and David Skinner advanced the field by developing recursive formulas for scattering amplitudes in twistor space, leveraging BCFW recursion to construct tree-level amplitudes for both Yang-Mills and gravity theories.^[11] These efforts addressed gaps in the original theory, which initially emphasized left-handed self-duality, through extensions like Penrose's 2015 palatial twistor theory, which introduced "palaces" to incorporate right-handed (or "googly") structures and resolve chirality issues in gravitational contexts.

Mathematical Foundations

Prerequisites

Complex manifolds form the foundational geometric structures underlying twistor space, where the complex projective space \mathbb{CP}^n is defined as the quotient of \mathbb{C}^{n+1} \setminus \{0\} by the equivalence relation identifying points via scalar multiplication by nonzero complex numbers, thus representing lines through the origin in \mathbb{C}^{n+1}. Points in \mathbb{CP}^n are described using homogeneous coordinates [z_0 : z_1 : \dots : z_n], where (z_0, \dots, z_n) \in \mathbb{C}^{n+1} \setminus \{0\} and scaling by \lambda \in \mathbb{C}^\times yields the same point, endowing \mathbb{CP}^n with the structure of a compact complex manifold of complex dimension n.^[12] In four-dimensional Minkowski space, the spinor formalism provides a double-cover representation of the Lorentz group, with \mathrm{SL}(2, \mathbb{C}) acting as the universal cover of \mathrm{SO}^+(1,3), mapping two-component complex spinors to four-vectors via the identification x^{AA'} = x^{\mu} \sigma^{AA'}_{\mu}, where \sigma^{AA'}_{\mu} are Pauli matrices extended to include the identity. Weyl spinors consist of left-handed spinors \omega^A transforming under the fundamental representation of \mathrm{SL}(2, \mathbb{C}) and right-handed spinors \pi_{A'} under the conjugate representation, with index notation A, A' = 0,1 facilitating contractions like the position bivector x^{AA'}. This formalism captures the chiral structure of massless fields, where the Lorentz transformations preserve the null cone through these spinorial descriptions.^[13] The conformal group of Minkowski space extends the Poincaré group by including inversions and dilations, realized as \mathrm{SU}(2,2), the double cover of \mathrm{SO}(4,2), which preserves angles and the light cone structure while acting linearly on the six-dimensional embedding space containing Minkowski space as a hyperboloid. This group, with Lie algebra \mathfrak{su}(2,2) \cong \mathfrak{so}(4,2), generates transformations that map null geodesics to null geodesics, crucial for the conformal invariance underlying twistor constructions.^[14] Hermitian forms on \mathbb{C}^4 play a key role in distinguishing twistor types, defined by a nondegenerate sesquilinear inner product of signature (2,2), such as \Phi(Z, \bar{W}) = Z^0 \bar{W}^0 + Z^1 \bar{W}^1 - Z^2 \bar{W}^2 - Z^3 \bar{W}^3, which is preserved by \mathrm{SU}(2,2) and classifies twistors as null (\Phi(Z,\bar{Z})=0), positive, or negative based on the sign of this form. This (2,2) signature reflects the split between timelike and spacelike directions in the conformal compactification of Minkowski space, providing the metric structure for twistor space.^[15] Holomorphic functions on twistor space, along with sheaf cohomology, enable the representation of massless fields through contour integrals over suitable cycles, where solutions to field equations correspond to cohomology classes in the Dolbeault complex, capturing global obstructions and ensuring analytic continuation. Specifically, the Penrose transform reconstructs spacetime fields from holomorphic sections or cohomology elements on open sets in twistor space, with contour integrals providing explicit formulas for zero-rest-mass fields of arbitrary helicity.^[16]

Formal Definition

Twistor space originates from the algebraic structure introduced by Penrose, where the non-projective twistor space T is defined as the complex vector space \mathbb{C}^4 equipped with coordinates Z^\alpha = (\omega^A, \pi_{A'}), with A, A' = 0, 1 indexing the undotted and dotted spinor components, respectively. This space carries a natural holomorphic volume form \varepsilon_{\alpha\beta\gamma\delta}, the totally antisymmetric Levi-Civita symbol, which provides a canonical orientation and is invariant under the holomorphic transformations of the space. Twistor space T also carries a natural holomorphic symplectic form induced by the volume form, which is crucial for the Penrose transform. Additionally, T admits a Hermitian inner product H(Z, W) = \omega^A \bar{\pi}_{A'} + \bar{\omega}^{A'} \pi_{A'}, which is indefinite with signature (2,2), enabling the distinction between space-like, time-like, and null structures in the correspondence to spacetime.^[17] The projective twistor space PT, which forms the primary arena for twistor geometry, is obtained by projectivizing T \setminus \{0\} under the action of \mathbb{C}^*, yielding PT \cong \mathbb{CP}^3. As a compact complex manifold, PT inherits a Kähler structure from the Fubini-Study metric, making it a natural space for holomorphic constructions in complex geometry. The homogeneous coordinates on PT satisfy [Z^\alpha] = [\lambda Z^\alpha] for \lambda \in \mathbb{C}^*, with the zero section excluded to avoid the origin in T. The fundamental incidence relation establishes the correspondence between twistor space and complexified Minkowski spacetime \mathbb{CM} \cong \mathbb{C}^4 with coordinates x^{AA'}. For a point x \in \mathbb{CM}, the associated twistor line L_x \subset PT consists of all projective twistors satisfying

\omega^A = i x^{AA'} \pi_{A'}

for \pi_{A'} \neq 0, parameterizing a \mathbb{CP}^1 in PT. Dually, this correspondence implies that lines in PT are in bijective relation with points in \mathbb{CM}, while points in PT correspond to null geodesics in \mathbb{CM}, each represented as a Riemann sphere \mathbb{CP}^1.^[17] To incorporate physical reality conditions, real twistors are those satisfying H(Z, \bar{Z}) = 0, corresponding to null rays in real Minkowski spacetime. Normalization is often imposed, such as \pi_{A'} \pi^{A'} = 1 for non-vanishing \pi, to fix the scaling on representative twistors. The infinity twistor I_{\alpha \beta}, with spinor components I_{AA' BB'} = \varepsilon_{AB} \varepsilon_{A' B'}, encodes the conformal structure at infinity, defining the boundary of compactified Minkowski space and facilitating the treatment of conformal invariance via the reality condition I_{\alpha \beta} Z^\alpha \bar{Z}^\beta = 0.^[17]

Geometric and Algebraic Structure

Twistor Correspondence

The twistor correspondence establishes a duality between elements of projective twistor space \mathbb{PT} \cong \mathbb{CP}^3 and geometric objects in complexified Minkowski spacetime \mathcal{M}^6 \cong \mathbb{C}^4. Specifically, each point x in \mathcal{M}^6 corresponds to a complex projective line \mathbb{CP}^1 in \mathbb{PT}, parameterized by the solutions to the incidence relation that links spacetime coordinates to twistor components. Conversely, each point in \mathbb{PT} corresponds to a null line (or \alpha-plane, a totally null 2-dimensional subspace) in \mathcal{M}^6. This point-line duality highlights the non-local nature of the mapping, where two such \mathbb{CP}^1 lines in \mathbb{PT} intersect if and only if their corresponding spacetime points are null-separated.^[18] This duality generalizes the classical Klein correspondence from nineteenth-century projective geometry, which identifies lines in projective 3-space with points on a quadric in projective 5-space. In twistor theory, the Klein correspondence extends this to flags—incident point-line pairs—in \mathbb{PT}, which map bijectively to flags in \mathcal{M}^6. Such flags encode higher-order incidences, like the intersection of null lines, providing a projective framework for spacetime geometry that preserves the conformal structure.^[18] The full correspondence operates in the complexified spacetime \mathcal{M}^6, where twistor space captures all holomorphic structures without restriction. Physical Minkowski spacetime \mathbb{M}^4 emerges as a real slice of \mathcal{M}^6, selected by imposing reality conditions via conjugate twistors \bar{Z}^\alpha, which ensure Hermitian positivity and Lorentzian signature. This complex-to-real reduction preserves the duality while restricting to observable geometries, such as real null geodesics.^[18] Asymptotic twistors play a crucial role in extending the correspondence to the conformal completion \bar{\mathcal{M}} of Minkowski spacetime, incorporating null infinity \mathcal{I} as a \mathbb{CP}^1 at the boundary. The infinity twistor I^{\alpha \dot{\beta}} defines this structure by specifying the conformal class at infinity, where lines in \mathbb{PT} tangent to the infinity \mathbb{CP}^1 correspond to null directions approaching \mathcal{I}. This allows the twistor framework to handle asymptotic behaviors, such as radiation fields, uniformly across the compactified spacetime.^[18] Codimension-1 subspaces in \mathbb{PT}, which are complex hyperplanes of dimension 2, correspond to 3-dimensional null hypersurfaces in \mathcal{M}^6. These hypersurfaces are ruled by null geodesics and arise from the orthogonal complement defined by a dual twistor, linking the projective structure of \mathbb{PT} to codimension-1 null foliations in spacetime.

Key Properties

Twistor space possesses a rich topological structure that underpins its geometric utility. The projective twistor space \mathbb{PT}, which is the complex projective space \mathbb{CP}^3, is simply connected with a trivial fundamental group and an Euler characteristic of 4. In contrast, the full twistor space \mathbb{T} \cong \mathbb{C}^4 is contractible, reflecting its non-compact nature as a vector space.^[19] A key feature is the Kähler structure on \mathbb{PT}, induced by the Fubini-Study metric, which provides a natural Hermitian metric compatible with the complex structure. This metric is Kähler-Einstein with positive Ricci curvature, though twistor constructions for certain self-dual metrics yield scalar-flat Kähler structures away from singular loci associated with conformal infinity. Complementing this, \mathbb{T} admits a holomorphic symplectic form \Omega = \sum_{A=0}^{1} d\omega^A \wedge d\pi_{A'}, endowing it with a natural Poisson structure that facilitates quantization and integration over cycles.^[19] Null twistors, characterized by vanishing Hermitian form H(Z, \bar{Z}) = 0, correspond directly to light rays (null geodesics) in Minkowski spacetime via the twistor correspondence.^[20] The sign of this form distinguishes further: positive norms identify with timelike elements, while negative norms align with spacelike ones, enabling a classification of causal structures in the dual spacetime geometry.^[6] Cohomological properties are central to the representational power of twistor space. The Dolbeault cohomology groups H^{0,p}(\mathbb{PT}, \mathcal{O}(-k)), where \mathcal{O}(-k) denotes the holomorphic line bundle of degree -k, classify global sections and cohomology classes that represent scalar and higher-spin functions on twistor space.^[19] The Penrose transform provides an explicit isomorphism by inverting the incidence relation through contour integrals over suitable chains in \mathbb{PT}, mapping these classes to solutions of differential equations on spacetime.^[19] The symmetry group of twistor space is SL(2,ℂ) × SL(2,ℂ), acting linearly on the coordinates of \mathbb{T} via the left and right spinor representations, with the quotient by the ℂ* scaling yielding the action on \mathbb{PT}. This group is the double cover of the conformal group SO(2,4) of compactified Minkowski space, preserving the incidence structure.^[19] Real structures induced by conjugation fix loci such as the Poincaré disk, modeling the space of real null twistors and facilitating the embedding of physical observables.^[21]

Physical Applications

In Spacetime and Conformal Geometry

Twistor space provides a natural framework for incorporating the conformal structure of spacetime, where the conformally invariant twistor equation allows solutions to be defined on the compactified Minkowski space \bar{\mathcal{M}}, obtained by adjoining null infinity \mathcal{I}^\alpha to the original Minkowski space \mathcal{M}.^[22] This compactification preserves the conformal geometry, enabling twistor theory to treat massless fields and gravitational phenomena in a way that is invariant under conformal transformations of the underlying spacetime.^[23] By mapping spacetime points to lines in projective twistor space \mathbb{PT}, the theory idealizes flat Minkowski space into a compact complex manifold, facilitating the study of asymptotic behaviors at null infinity.^[22] In this setting, self-dual null congruences in spacetime correspond to holomorphic curves in projective twistor space \mathbb{[PT](/page/PT)}, as established by Kerr's theorem, which links shear-free null geodesic congruences to rational holomorphic functions on twistor space.^[23] Penrose's nonlinear graviton construction extends this correspondence to generate anti-self-dual Einstein metrics, where deformations of the flat twistor space yield curved anti-self-dual vacuum solutions to the Einstein equations, representing gravitational fields with left-handed helicity.^[24] These metrics arise from holomorphic data on twistor space, providing an integrable system for constructing exact gravitational solutions without solving the full nonlinear Einstein equations directly.^[25] Twistor space also captures the asymptotic structure of spacetime through its description of the Bondi-Metzner-Sachs (BMS) group acting at null infinity \mathcal{I}, where BMS transformations correspond to holomorphic vector fields on the twistor space of \mathcal{I}.^[26] This formulation allows the cut equations, defined via intersections of twistors with cuts of null infinity, to encode gravitational radiation, relating the shear and news functions to twistor data for computing asymptotic quantities like angular momentum flux.^[27] Such cut equations ensure continuity of conserved quantities across radiating regions, providing a twistor-based tool for analyzing the Bondi mass loss due to gravitational waves.^[28] For geometric optics and wave equations, zero-rest-mass fields, such as the Maxwell field, are represented as cohomology classes in projective twistor space \mathbb{PT}, where solutions satisfy the Dolbeault equation \bar{\partial} \phi = 0 on appropriate sheaves.^[22] The Penrose transform reconstructs these fields in spacetime from holomorphic representatives in twistor cohomology, yielding exact solutions to the source-free Maxwell equations and more generally to higher-helicity zero-rest-mass equations, with the cohomology groups classifying the radiative degrees of freedom.^[3] This approach leverages the incidence relation between twistors and spacetime null geodesics to propagate wave solutions conformally.^[29] The original twistor formalism exhibited a left-handed bias, primarily encoding anti-self-dual (left-helicity) components due to its reliance on the standard twistor correspondence, which favored one chiral sector in curved spaces.^[24] This asymmetry, known as the googly problem, has been addressed through extensions like palatial twistor theory, which introduces dual structures to incorporate right-handed fields symmetrically.^[24] Twistor methods have proven effective for exact solutions, such as pp-wave spacetimes, where the twistor space remains flat despite the curved spacetime, allowing initial data on twistor lines to characterize these plane-fronted waves with parallel rays as solutions to the vacuum Einstein equations.^[30]

In Quantum Field Theory

In quantum field theory, twistor space facilitates efficient computations of scattering amplitudes, especially in supersymmetric gauge theories, by reformulating momentum-space expressions as geometric integrals over projective space. The maximally helicity-violating (MHV) amplitudes in Yang-Mills theory are particularly simplified in twistor variables, where the Parke-Taylor formula emerges naturally from the twistor-string construction, expressing the amplitude for n gluons with two negative helicities as

A_n(1^+, \dots, i^-, j^-, \dots, n^+) = \frac{\langle i j \rangle^4}{\prod_{k=1}^n \langle k \, k+1 \rangle},

with spinor products \langle ab \rangle and cyclic identification n+1 \equiv 1.^[10] This representation arises from contour integrals localizing on intersection patterns in twistor space, highlighting the holomorphic structure underlying MHV configurations. Extending this approach, Bourjaily, Cachazo, and Trnka developed a formula for all tree-level amplitudes in \mathcal{N}=4 super Yang-Mills using multidimensional contours over \mathbb{CP}^3, capturing higher helicity sectors (NkMHV) through residues that enforce momentum conservation and supersymmetry.^[31] Twistor string theory provides a unified framework for generating these amplitudes, as proposed by Witten, by interpreting perturbative expansions as worldsheet integrals of a holomorphic Chern-Simons theory on supertwistor space \mathbb{CP}^{3|4}.^[10] In this setup, the action is

S = \frac{1}{2} \int_{\mathbb{CP}^{3|4}} \Omega \wedge \Tr \left( A \bar{\partial} A + \frac{2}{3} A \wedge A \wedge A \right),

where A is a \mathfrak{u}(N) (0,1)-form connection, \Omega the holomorphic volume form, and D-instanton contributions yield tree-level Yang-Mills amplitudes while loop corrections produce gravity ones, bridging gauge and gravitational sectors without explicit Feynman diagrams.^[10] This duality reveals hidden simplicities in amplitude factorization and dual conformal invariance. Twistor space also illuminates integrable structures in quantum field theories, particularly through the Ward equations for self-dual Yang-Mills, which are recast as holomorphy conditions on cohomology classes in Penrose twistor space via the Penrose-Ward transform.^[32] Solutions to these equations correspond to holomorphic bundles over twistor lines, enabling exact treatments of the self-dual sector. This perspective extends to \mathcal{N}=4 super Yang-Mills, where twistor variables uncover Yangian symmetries and integrability in spectral problems, facilitating computations of anomalous dimensions and Wilson loops beyond perturbation theory.^[33] A landmark recent development is the amplituhedron, introduced by Arkani-Hamed and Trnka, which geometrizes tree-level \mathcal{N}=4 super Yang-Mills amplitudes as volumes of a positive Grassmannian embedded in momentum twistor space, bypassing traditional locality and unitarity to directly encode the S-matrix.^[34] This "jewel of geometry" triangulates into cells whose canonical forms yield amplitudes, with the full volume integrating to the all-loop integrand in select cases. Due to the inherent chirality of twistor space—favoring positive helicity via homogeneous coordinates of degree -1—handling negative helicity requires non-homogeneous coordinates or extensions to dual (palatial) twistor space, allowing symmetric treatment of both chiral sectors in amplitude computations.

Extensions and Developments

Higher-Dimensional Generalizations

Twistor spaces can be generalized to Euclidean signature spacetime \mathbb{R}^4, where the conformal group SU(2,2) of the Lorentzian case is replaced by SU(4), acting on \mathbb{C}^4 while preserving a Hermitian form.^[35] In this framework, the projective twistor space PT is identified with \mathbb{CP}^3, providing a natural arena for spinor degrees of freedom and gauge symmetries.^[35] The reality structure differs from the Minkowski case, incorporating a degree of freedom for an imaginary time direction that facilitates analytic continuation between signatures and supports applications in gauge theories, such as the study of instantons through holomorphic bundles over this twistor space.^[35] In higher dimensions, twistor constructions extend to six-dimensional Minkowski spacetime with signature (1,5), where twistors correspond to spinors of the conformal group SO(2,6), realized via the double cover Spin(2,6).^[36] These 6D twistors enable formulations of massless fields and infinite spin representations, mapping spacetime points to lines in the twistor space.^[36] Ambitwistor spaces, which parametrize complex null geodesics, generalize further to arbitrary dimensions n, targeting spacetimes of signature (n-1,1), and serve as targets for chiral string models that yield scattering amplitudes in field theories. For hyperkähler four-manifolds, twistor spaces are constructed as \mathbb{CP}^1-bundles over the base manifold, assembling the S^2-family of compatible complex structures into a single complex structure on the total space Z = M \times S^2.^[37] This Ward construction, originally for self-dual metrics, extends to hyperkähler geometries, yielding non-Kähler Calabi-Yau structures on branched covers of Z and balanced Hermitian metrics under certain conditions.^[37]^[38] Such twistor spaces find applications in type II string compactifications on Calabi-Yau manifolds, providing a non-perturbative description of the effective action through holomorphic Chern-Simons theory on the twistor space. In split-signature spacetimes, such as (3,3) for six-dimensional theories, the corresponding twistor space PT becomes non-compact, reflecting the indefinite metric and leading to real-variable formulations akin to X-ray transforms for field representations. Higher-dimensional generalizations face challenges, including the loss of compactness in twistor spaces beyond four dimensions, which complicates holomorphic cohomology and Penrose transform analogs.^[38] Partial results exist for five and seven dimensions through extensions via supergroups, such as in ambitwistor string models that incorporate supersymmetry to handle odd-dimensional cases. Ambitwistor space is a five-dimensional complex manifold that parameterizes complex null geodesics in complexified Minkowski spacetime, extending the twistor framework to encode both position and momentum along light rays.^[39] It arises as the space of holomorphic maps relevant to ambitwistor string theories, which unify the description of scattering amplitudes across different helicity sectors, unlike the original twistor strings focused on self-dual fields.^[40] The connection to twistor space is established through a Legendre transform, relating the symplectic structure of ambitwistor space to the twistor correspondence for null geodesics.^[39] This formulation has been pivotal in the Cachazo-Skinner approach to loop-level scattering amplitudes in gauge theories and gravity, where integration over the moduli space of ambitwistor strings yields compact expressions for multi-loop integrands.^[39] Twistor cohomology provides a sheaf-theoretic generalization of the Penrose transform, allowing the description of massive fields on Minkowski space through cohomology classes on appropriate bundles over projective twistor space \mathbb{P}^3.^[41] Originally developed for massless fields, the transform maps holomorphic sections or cohomology groups on twistor space to solutions of field equations in spacetime; for massive particles, it involves higher-degree bundles and Dolbeault cohomology to incorporate mass parameters while preserving conformal invariance at the twistor level.^[16] This cohomological approach, as detailed in works on twistor-particle models, enables the construction of massive wave functions and has applications in extending twistor methods to non-conformal theories. Supertwistor space incorporates fermionic coordinates to accommodate supersymmetry, with the prototypical example being the supertwistor space \mathbb{C}^{4|4} for \mathcal{N}=4 super Yang-Mills theory.^[42] This graded manifold extends the bosonic twistor space by adding four Grassmann-odd variables, allowing the Penrose-Ward transform to map supertwistor cohomology to supersymmetric field configurations on spacetime, including both gauge and matter multiplets.^[42] The resulting twistor actions for \mathcal{N}=4 SYM capture the full supersymmetric spectrum and have facilitated computations of supersymmetric Wilson loops and scattering amplitudes in this theory.^[43] Twistor space has inspired holographic dualities beyond the standard AdS/CFT framework, particularly through "twistor uplifts" that map flat-space amplitudes to conformal field theory correlators via celestial holography.^[44] In this context, twistor variables provide a projective geometry for boundary CFTs on the celestial sphere, linking momentum-space amplitudes in four dimensions to Witten diagrams in anti-de Sitter space and enabling the study of infrared divergences and soft theorems holographically.^[45] These connections, explored in celestial twistor formulations, offer a pathway to understand amplitude factorization and unitarity in holographic settings.^[44] Despite these advances, twistor theory remains incomplete in unifying quantum gravity with the standard model, as it primarily addresses classical and perturbative aspects without a full non-perturbative quantization of general relativity.^[46] Efforts to bridge this gap have explored links to non-commutative geometry, where twistor spaces inform operator algebras for quantized spacetimes, but a comprehensive framework integrating fermions, gravity, and quantum effects is still lacking.^[47] As of 2025, ongoing developments include twistor sigma models for minimal tension holography and workshops such as the 2024 "Twistors in Geometry & Physics" at the Isaac Newton Institute, leveraging supertwistor extensions and holographic insights to address these challenges.^[46]^[48]^[49]

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Palatial twistor theory and the twistor googly problem - Journals
Aug 6, 2015 · If s=0, such a history is a null geodesic—henceforth called a ray—which provides the most immediate picture of what is referred to as a null ...
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[PDF] The Nonlinear Graviton as an Integrable System - DAMTP
It is explained how to construct ASDVE metrics from solutions of various. 2D integrable systems by exploiting the fact that the Lax formulations of both systems ...
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Twistorial description of Bondi-Metzner-Sachs symmetries at null ...
We will use the definition of asymptotic flatness given by Penrose's conformal completion (see [5, 14] ) and denote null infinity as I ≅ R × S 2 . Abstract ...<|control11|><|separator|>
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[PDF] arXiv:2110.00140v1 [gr-qc] 1 Oct 2021
Oct 1, 2021 · Whereas the BMS-based formulas were quadratic in the gravitational radiation, the twistor formulas had first- and third-order terms, present ...
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Structure of asymptotic twistor space - American Institute of Physics
We show that asymptotic projective twistor space &' Y+ is an Einstein-Kahler manifold of positive curvature. We then use the Chern-Moser theory of hyper ...
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The Twistor Program - Inspire HEP
Free massless fields can be represented in terms of the sheaf cohomology of portions of this space. Twistor space (or a suitable part of it) can be expressed in ...
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[PDF] Curved Twistor Spaces - Oxford University Research Archive
This states essentially that a shear-free congruence of null geodesies in Minkowski space-time corresponds to a holomorphic 2-surface in twistor space IPX7. In ...
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Perturbative Gauge Theory As A String Theory In Twistor Space - arXiv
Dec 15, 2003 · 252:189-258,2004 ... Access Paper: View a PDF of the paper titled Perturbative Gauge Theory As A String Theory In Twistor Space, by Edward Witten.
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On Supertwistors, the Penrose-Ward Transform and N=4 super ...
Jan 23, 2006 · We review the supertwistor description of self-dual and anti-self-dual N-extended SYM theory as the integrability of super Yang-Mills fields on complex (2|N)- ...
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[1410.6310] A Twistorial Approach to Integrability in N=4 SYM - arXiv
Oct 23, 2014 · In this note, we propose that viewing the problem through the lens of twistor theory should help to clarify the reasons for integrability.
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[1312.2007] The Amplituhedron - arXiv
Dec 6, 2013 · Title:The Amplituhedron. Authors:Nima Arkani-Hamed, Jaroslav Trnka ... Amplituhedron--generalizing the positive Grassmannian. Locality and ...Missing: twistor | Show results with:twistor
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[2104.05099] Euclidean Twistor Unification - arXiv
Apr 11, 2021 · Taking Euclidean signature space-time with its local Spin(4)=SU(2)xSU(2) group of space-time symmetries as fundamental, one can consistently ...
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Twistor formulation of massless 6D infinite spin fields - ScienceDirect
We construct massless infinite spin irreducible representations of the six-dimensional Poincaré group in the space of fields depending on twistor variables.
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[1309.4759] Generalized twistor spaces for hyperkähler manifolds
Sep 18, 2013 · The S^2-family of complex structures compatible with the hyperkähler metric can be assembled into a single complex structure on Z=MxS^2.Missing: 4- Ward string compactifications
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[1609.09438] Higher dimensional generalizations of twistor spaces
Sep 29, 2016 · Abstract:We construct a generalization of twistor spaces of hypercomplex manifolds and hyper-Kahler manifolds M, by generalizing the twistor ...
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[1311.2564] Ambitwistor strings and the scattering equations - arXiv
Nov 11, 2013 · Geometrically they describe holomorphic maps to spaces of complex null geodesics, known as ambitwistor spaces. They have the standard critical ...
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Ambitwistor Strings in Four Dimensions | Phys. Rev. Lett.
Aug 19, 2014 · We develop ambitwistor string theories for four dimensions to obtain new formulas for tree-level gauge and gravity amplitudes with arbitrary ...Missing: 2n- | Show results with:2n-
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On the Twistor Description of Massive Fields - jstor
Secondly, the function appearing in the integrand is not a general holomorphic function (as is the case for massless fields) but is assumed to be in eigenstates ...
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[hep-th/0604040] Supersymmetric Gauge Theories in Twistor Space
Apr 6, 2006 · We also provide twistor actions for gauge theories with N<4 supersymmetry, and show how matter multiplets may be coupled to the gauge sector.Missing: SYM | Show results with:SYM
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Composite Operators in the Twistor Formulation of Supersymmetric ...
Jun 29, 2016 · The action of N = 4 SYM in twistor space is the sum of two parts S 1 + S 2 , with S 1 , introduced in Ref. [10] , describing the self-dual part ...
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[2306.11850] Celestial holography and AdS3/CFT2 from a scaling ...
Jun 20, 2023 · Here we provide a framework to work on the projective spinor bundle of hyperbolic slices, obtained from a careful scaling reduction of the twistor space of 4d ...
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Celestial twistor amplitudes | Phys. Rev. D
Sep 14, 2023 · This is motivated by a refined holographic correspondence between the twistor transform and the light transform in the boundary Lorentzian CFT.
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Twistor theory at fifty: from contour integrals to twistor strings - PMC
The Robinson congruence in figure 2 is taken from the front cover of Penrose & Rindler [3].
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https://www.worldscientific.com/doi/10.1142/9789812700988_0017