twistor theory

{{Short description|Possible path to quantum gravity proposed by Roger Penrose}}

In theoretical physics, twistor theory was proposed by Roger Penrose in 1967{{cite journal|last1=Penrose|first1=R.|date=1967|title=Twistor Algebra|journal=Journal of Mathematical Physics|volume=8|issue=2|pages=345–366|bibcode=1967JMP.....8..345P|doi=10.1063/1.1705200}} as a possible path{{Cite journal|last1=Penrose|first1=R.|last2=MacCallum|first2=M.A.H.|title=Twistor theory: An approach to the quantisation of fields and space-time|journal=Physics Reports|volume=6|issue=4|pages=241–315|doi=10.1016/0370-1573(73)90008-2|year=1973|bibcode=1973PhR.....6..241P}} to quantum gravity and has evolved into a widely studied branch of theoretical and mathematical physics. Penrose's idea was that twistor space should be the basic arena for physics from which space-time itself should emerge. It has led to powerful mathematical tools that have applications to differential and integral geometry, nonlinear differential equations and representation theory, and in physics to general relativity, quantum field theory, and the theory of scattering amplitudes.

Twistor theory arose in the context of the rapidly expanding mathematical developments in Einstein's theory of general relativity in the late 1950s and in the 1960s and carries a number of influences from that period. In particular, Roger Penrose has credited Ivor Robinson as an important early influence in the development of twistor theory, through his construction of so-called Robinson congruences.{{cite book |first=Roger |last=Penrose |chapter=On the Origins of Twistor Theory |title=Gravitation and Geometry, a Volume in Honour of Ivor Robinson |editor-first=Wolfgang |editor-last=Rindler |editor2-first=Andrzej |editor2-last=Trautman |publisher=Bibliopolis |year=1987 |isbn=88-7088-142-3 }}

Overview

Projective twistor space $\mathbb{PT}$ is projective 3-space $\mathbb{CP}^3$ , the simplest 3-dimensional compact algebraic variety. It has a physical interpretation as the space of massless particles with spin. It is the projectivisation of a 4-dimensional complex vector space, non-projective twistor space $\mathbb{T}$ , with a Hermitian form of signature (2, 2) and a holomorphic volume form. This can be most naturally understood as the space of chiral (Weyl) spinors for the conformal group $SO(4,2)/\mathbb{Z}_2$ of Minkowski space; it is the fundamental representation of the spin group $SU(2,2)$ of the conformal group. This definition can be extended to arbitrary dimensions except that beyond dimension four, one defines projective twistor space to be the space of projective pure spinors{{cite journal | last1=Harnad | first1=J. | last2=Shnider | first2=S. | title=Isotropic geometry and twistors in higher dimensions. I. The generalized Klein correspondence and spinor flags in even dimensions | journal=Journal of Mathematical Physics | volume=33 | issue=9 | year=1992 | doi=10.1063/1.529538 | pages=3197–3208 | bibcode=1992JMP....33.3197H }}{{cite journal | last1=Harnad | first1=J. | last2=Shnider | first2=S. | title=Isotropic geometry and twistors in higher dimensions. II. Odd dimensions, reality conditions, and twistor superspaces | journal=Journal of Mathematical Physics | volume=36 | issue=9 | year=1995 | doi=10.1063/1.531096 | pages=1945–1970 | doi-access=free | bibcode=1995JMP....36.1945H }} for the conformal group.{{Cite book |title=Spinors and Space-Time |last1=Penrose |first1=Roger |last2=Rindler |first2=Wolfgang |publisher=Cambridge University Press |year=1986 |isbn=9780521252676 |pages=Appendix |language=en |doi=10.1017/cbo9780511524486}}{{Cite journal |last1=Hughston |first1=L. P. |last2=Mason |first2=L. J. |date=1988 |title=A generalised Kerr-Robinson theorem |journal=Classical and Quantum Gravity |language=en |volume=5 |issue=2 |pages=275 |doi=10.1088/0264-9381/5/2/007 |issn=0264-9381 |bibcode=1988CQGra...5..275H |s2cid=250783071 }}

In its original form, twistor theory encodes physical fields on Minkowski space in terms of complex analytic objects on twistor space via the Penrose transform. This is especially natural for massless fields of arbitrary spin. In the first instance these are obtained via contour integral formulae in terms of free holomorphic functions on regions in twistor space. The holomorphic twistor functions that give rise to solutions to the massless field equations can be more deeply understood as Čech representatives of analytic cohomology classes on regions in $\mathbb{PT}$ . These correspondences have been extended to certain nonlinear fields, including self-dual gravity in Penrose's nonlinear graviton construction{{cite journal | last1 = Penrose | first1 = R. | year = 1976 | title = Non-linear gravitons and curved twistor theory | url = | journal = Gen. Rel. Grav. | volume = 7 | issue = 1 | pages = 31–52 | doi = 10.1007/BF00762011 | bibcode = 1976GReGr...7...31P | s2cid = 123258136 }} and self-dual Yang–Mills fields in the so-called Ward construction;{{Cite journal |last=Ward |first=R. S. |author-link=Richard S. Ward |title=On self-dual gauge fields |journal=Physics Letters A |volume=61 |issue=2 |pages=81–82 |doi=10.1016/0375-9601(77)90842-8 |year=1977 |bibcode=1977PhLA...61...81W}} the former gives rise to deformations of the underlying complex structure of regions in $\mathbb{PT}$ , and the latter to certain holomorphic vector bundles over regions in $\mathbb{PT}$ . These constructions have had wide applications, including inter alia the theory of integrable systems.{{Cite book |title=Twistor geometry and field theory |last=Ward |first=R. S. |date=1990 |publisher=Cambridge University Press |others=Wells, R. O. |isbn=978-0521422680 |location=Cambridge [England] |oclc=17260289}}{{Cite book |title=Integrability, self-duality, and twistor theory |last1=Mason |first1=Lionel J. |last2=Woodhouse |first2=Nicholas M. J. |date=1996 |publisher=Clarendon Press |isbn=9780198534983 |location=Oxford |oclc=34545252}}{{Cite book |title=Solitons, instantons, and twistors |last=Dunajski |first=Maciej |date=2010 |publisher=Oxford University Press |isbn=9780198570622 |location=Oxford |oclc=507435856}}

The self-duality condition is a major limitation for incorporating the full nonlinearities of physical theories, although it does suffice for Yang–Mills–Higgs monopoles and instantons (see ADHM construction).{{Cite journal |last1=Atiyah |first1=M. F. |last2=Hitchin |first2=N. J. |last3=Drinfeld |first3=V. G. |last4=Manin |first4=Yu. I. |title=Construction of instantons |journal=Physics Letters A |volume=65 |issue=3 |pages=185–187 |doi=10.1016/0375-9601(78)90141-x |year=1978 |bibcode=1978PhLA...65..185A}} An early attempt to overcome this restriction was the introduction of ambitwistors by Isenberg, Yasskin and Green,{{Cite journal| last1=Isenberg |first1=James |last2=Yasskin |first2=Philip B. |last3=Green |first3=Paul S. |title=Non-self-dual gauge fields |journal=Physics Letters B |volume=78 |issue=4 |pages=462–464 |doi=10.1016/0370-2693(78)90486-0 |year=1978 |bibcode=1978PhLB...78..462I}} and their superspace extension, super-ambitwistors, by Edward Witten.{{Cite journal |last=Witten |first=Edward |title=An interpretation of classical Yang–Mills theory |journal=Physics Letters B |volume=77 |issue=4–5 |pages=394–398 |doi=10.1016/0370-2693(78)90585-3 |year=1978 |bibcode=1978PhLB...77..394W}} Ambitwistor space is the space of complexified light rays or massless particles and can be regarded as a complexification or cotangent bundle of the original twistor description. By extending the ambitwistor correspondence to suitably defined formal neighborhoods, Isenberg, Yasskin and Green showed the equivalence between the vanishing of the curvature along such extended null lines and the full Yang–Mills field equations. Witten showed that a further extension, within the framework of super Yang–Mills theory, including fermionic and scalar fields, gave rise, in the case of N = 1 or 2 supersymmetry, to the constraint equations, while for N = 3 (or 4), the vanishing condition for supercurvature along super null lines (super ambitwistors) implied the full set of field equations, including those for the fermionic fields. This was subsequently shown to give a {{clarify span|1-1|date=May 2024}} equivalence between the null curvature constraint equations and the supersymmetric Yang-Mills field equations.{{Cite journal | last1=Harnad | first1=J. | last2=Légaré | first2=M. | last3=Hurtubise | first3=J. | last4=Shnider | first4=S. | title=Constraint equations and field equations in supersymmetric N = 3 Yang-Mills theory | journal=Nuclear Physics B | volume=256 | pages=609–620 | doi=10.1016/0550-3213(85)90410-9 | year=1985 | bibcode=1985NuPhB.256..609H }}{{Cite journal | last1=Harnad | first1=J. | last2=Hurtubise | first2=J. | last3=Shnider | first3=S. | title=Supersymmetric Yang-Mills equations and supertwistors | journal=Annals of Physics | volume=193 | issue=1 | pages=40–79 | doi=10.1016/0003-4916(89)90351-5 | year=1989 | bibcode=1989AnPhy.193...40H }} Through dimensional reduction, it may also be deduced from the analogous super-ambitwistor correspondence for 10-dimensional, N = 1 super-Yang–Mills theory.{{cite journal | first1=E. | last1=Witten | title=Twistor-like transform in ten dimensions | journal=Nuclear Physics | volume=B266 | pages=245–264 | year=1986 | issue=2 | doi=10.1016/0550-3213(86)90090-8 | bibcode=1986NuPhB.266..245W }}{{cite journal | first1=J. | last1=Harnad | first2=S. | last2=Shnider | title=Constraints and Field Equations for Ten Dimensional Super Yang-Mills Theory | journal=Commun. Math. Phys. | volume=106 | pages=183–199 | year=1986 | issue=2 | doi=10.1007/BF01454971 | bibcode=1986CMaPh.106..183H | s2cid=122622189 | url=http://projecteuclid.org/euclid.cmp/1104115696 }}

Twistorial formulae for interactions beyond the self-dual sector also arose in Witten's twistor string theory,{{cite journal |last1=Witten |first1=Edward |date=2004 |title=Perturbative Gauge Theory as a String Theory in Twistor Space |journal=Communications in Mathematical Physics |volume=252 |issue=1–3 |pages=189–258 |arxiv=hep-th/0312171 |bibcode=2004CMaPh.252..189W |doi=10.1007/s00220-004-1187-3 |s2cid=14300396}} which is a quantum theory of holomorphic maps of a Riemann surface into twistor space. This gave rise to the remarkably compact RSV (Roiban, Spradlin and Volovich) formulae for tree-level S-matrices of Yang–Mills theories,{{Cite journal |last1=Roiban |first1=Radu |last2=Spradlin |first2=Marcus |last3=Volovich |first3=Anastasia |date=2004-07-30 |title=Tree-level S matrix of Yang–Mills theory |journal=Physical Review D |volume=70 |issue=2 |pages=026009 |doi=10.1103/PhysRevD.70.026009 |bibcode=2004PhRvD..70b6009R |arxiv=hep-th/0403190 |s2cid=10561912}} but its gravity degrees of freedom gave rise to a version of conformal supergravity limiting its applicability; conformal gravity is an unphysical theory containing ghosts, but its interactions are combined with those of Yang–Mills theory in loop amplitudes calculated via twistor string theory.{{Cite journal |last1=Berkovits |first1=Nathan |last2=Witten |first2=Edward |date=2004 |title=Conformal supergravity in twistor-string theory |journal=Journal of High Energy Physics |language=en |volume=2004 |issue=8 |pages=009 |doi=10.1088/1126-6708/2004/08/009 |issn=1126-6708 |bibcode=2004JHEP...08..009B |arxiv=hep-th/0406051 |s2cid=119073647}}

Despite its shortcomings, twistor string theory led to rapid developments in the study of scattering amplitudes. One was the so-called MHV formalism{{Cite journal |last1=Cachazo |first1=Freddy |last2=Svrcek |first2=Peter |last3=Witten |first3=Edward |date=2004 |title=MHV vertices and tree amplitudes in gauge theory |journal=Journal of High Energy Physics |language=en |volume=2004 |issue=9 |pages=006 |doi=10.1088/1126-6708/2004/09/006 |issn=1126-6708 |bibcode=2004JHEP...09..006C |arxiv=hep-th/0403047 |s2cid=16328643}} loosely based on disconnected strings, but was given a more basic foundation in terms of a twistor action for full Yang–Mills theory in twistor space.{{Cite journal |last1=Adamo |first1=Tim |last2=Bullimore |first2=Mathew |last3=Mason |first3=Lionel |last4=Skinner |first4=David |title=Scattering amplitudes and Wilson loops in twistor space |journal=Journal of Physics A: Mathematical and Theoretical |volume=44 |issue=45 |pages=454008 |doi=10.1088/1751-8113/44/45/454008 |year=2011 |bibcode=2011JPhA...44S4008A |arxiv=1104.2890 |s2cid=59150535}} Another key development was the introduction of BCFW recursion.{{Cite journal |last1=Britto |first1=Ruth |author1-link= Ruth Britto |last2=Cachazo |first2=Freddy |last3=Feng |first3=Bo |last4=Witten |first4=Edward |date=2005-05-10 |title=Direct Proof of the Tree-Level Scattering Amplitude Recursion Relation in Yang–Mills Theory |journal=Physical Review Letters |volume=94 |issue=18 |pages=181602 |doi=10.1103/PhysRevLett.94.181602 |pmid=15904356 |bibcode=2005PhRvL..94r1602B |arxiv=hep-th/0501052 |s2cid=10180346}} This has a natural formulation in twistor space{{Cite journal |last1=Mason |first1=Lionel |last2=Skinner |first2=David |date=2010-01-01 |title=Scattering amplitudes and BCFW recursion in twistor space |journal=Journal of High Energy Physics |language=en |volume=2010 |issue=1 |pages=64 |doi=10.1007/JHEP01(2010)064 |issn=1029-8479 |bibcode=2010JHEP...01..064M |arxiv=0903.2083 |s2cid=8543696}}{{Cite journal |last1=Arkani-Hamed |first1=N. |last2=Cachazo |first2=F. |last3=Cheung |first3=C. |last4=Kaplan |first4=J. |date=2010-03-01 |title=The S-matrix in twistor space |journal=Journal of High Energy Physics |language=en |volume=2010 |issue=3 |pages=110 |doi=10.1007/JHEP03(2010)110 |issn=1029-8479 |bibcode=2010JHEP...03..110A |arxiv=0903.2110 |s2cid=15898218}} that in turn led to remarkable formulations of scattering amplitudes in terms of Grassmann integral formulae{{Cite journal |last1=Arkani-Hamed |first1=N. |last2=Cachazo |first2=F. |last3=Cheung |first3=C. |last4=Kaplan |first4=J. |date=2010-03-01 |title=A duality for the S matrix |journal=Journal of High Energy Physics |language=en |volume=2010 |issue=3 |pages=20 |doi=10.1007/JHEP03(2010)020 |issn=1029-8479 |bibcode=2010JHEP...03..020A |arxiv=0907.5418 |s2cid=5771375}}{{Cite journal |last1=Mason |first1=Lionel |last2=Skinner |first2=David |date=2009 |title=Dual superconformal invariance, momentum twistors and Grassmannians |journal=Journal of High Energy Physics |language=en |volume=2009 |issue=11 |pages=045 |doi=10.1088/1126-6708/2009/11/045 |issn=1126-6708 |bibcode=2009JHEP...11..045M |arxiv=0909.0250 |s2cid=8375814}} and polytopes.{{Cite journal |last=Hodges |first=Andrew |date=2013-05-01 |title=Eliminating spurious poles from gauge-theoretic amplitudes |journal=Journal of High Energy Physics |language=en |volume=2013 |issue=5 |pages=135 |doi=10.1007/JHEP05(2013)135 |issn=1029-8479 |bibcode=2013JHEP...05..135H |arxiv=0905.1473 |s2cid=18360641}} These ideas have evolved more recently into the positive Grassmannian{{cite arXiv |last1=Arkani-Hamed |first1=Nima |last2=Bourjaily |first2=Jacob L. |last3=Cachazo |first3=Freddy |last4=Goncharov |first4=Alexander B. |last5=Postnikov |first5=Alexander |last6=Trnka |first6=Jaroslav |date=2012-12-21 |title=Scattering Amplitudes and the Positive Grassmannian |eprint=1212.5605 |class=hep-th}} and amplituhedron.

Twistor string theory was extended first by generalising the RSV Yang–Mills amplitude formula, and then by finding the underlying string theory. The extension to gravity was given by Cachazo & Skinner,{{Cite journal |last1=Cachazo |first1=Freddy |last2=Skinner |first2=David |date=2013-04-16 |title=Gravity from Rational Curves in Twistor Space |journal=Physical Review Letters |volume=110 |issue=16 |pages=161301 |doi=10.1103/PhysRevLett.110.161301 |pmid=23679592 |bibcode=2013PhRvL.110p1301C |arxiv=1207.0741 |s2cid=7452729}} and formulated as a twistor string theory for maximal supergravity by David Skinner.{{cite arXiv |last=Skinner |first=David |date=2013-01-04 |title=Twistor Strings for N = 8 Supergravity |eprint=1301.0868 |class=hep-th}} Analogous formulae were then found in all dimensions by Cachazo, He and Yuan for Yang–Mills theory and gravity{{Cite journal |last1=Cachazo |first1=Freddy |last2=He |first2=Song |last3=Yuan |first3=Ellis Ye |date=2014-07-01 |title=Scattering of massless particles: scalars, gluons and gravitons |journal=Journal of High Energy Physics |language=en |volume=2014 |issue=7 |pages=33 |doi=10.1007/JHEP07(2014)033 |issn=1029-8479 |bibcode=2014JHEP...07..033C |arxiv=1309.0885 |s2cid=53685436}} and subsequently for a variety of other theories.{{Cite journal |last1=Cachazo |first1=Freddy |last2=He |first2=Song |last3=Yuan |first3=Ellis Ye |date=2015-07-01 |title=Scattering equations and matrices: from Einstein to Yang–Mills, DBI and NLSM |journal=Journal of High Energy Physics |language=en |volume=2015 |issue=7 |pages=149 |doi=10.1007/JHEP07(2015)149 |issn=1029-8479 |bibcode=2015JHEP...07..149C |arxiv=1412.3479 |s2cid=54062406}} They were then understood as string theories in ambitwistor space by Mason and Skinner{{Cite journal |last1=Mason |first1=Lionel |last2=Skinner |first2=David |date=2014-07-01 |title=Ambitwistor strings and the scattering equations |journal=Journal of High Energy Physics |language=en |volume=2014 |issue=7 |pages=48 |doi=10.1007/JHEP07(2014)048 |issn=1029-8479 |bibcode=2014JHEP...07..048M |arxiv=1311.2564 |s2cid=53666173}} in a general framework that includes the original twistor string and extends to give a number of new models and formulae.{{Cite journal |last=Berkovits |first=Nathan |date=2014-03-01 |title=Infinite tension limit of the pure spinor superstring |journal=Journal of High Energy Physics |language=en |volume=2014 |issue=3 |pages=17 |doi=10.1007/JHEP03(2014)017 |issn=1029-8479 |bibcode=2014JHEP...03..017B |arxiv=1311.4156 |s2cid=28346354}}{{Cite journal |last1=Geyer |first1=Yvonne |last2=Lipstein |first2=Arthur E. |last3=Mason |first3=Lionel |date=2014-08-19 |title=Ambitwistor Strings in Four Dimensions |journal=Physical Review Letters |volume=113 |issue=8 |pages=081602 |doi=10.1103/PhysRevLett.113.081602 |pmid=25192087 |bibcode=2014PhRvL.113h1602G |arxiv=1404.6219 |s2cid=40855791}}{{Cite journal |last1=Casali |first1=Eduardo |last2=Geyer |first2=Yvonne |last3=Mason |first3=Lionel |last4=Monteiro |first4=Ricardo |last5=Roehrig |first5=Kai A. |date=2015-11-01 |title=New ambitwistor string theories |journal=Journal of High Energy Physics |language=en |volume=2015 |issue=11 |pages=38 |doi=10.1007/JHEP11(2015)038 |issn=1029-8479 |bibcode=2015JHEP...11..038C |arxiv=1506.08771 |s2cid=118801547}} As string theories they have the same critical dimensions as conventional string theory; for example the type II supersymmetric versions are critical in ten dimensions and are equivalent to the full field theory of type II supergravities in ten dimensions (this is distinct from conventional string theories that also have a further infinite hierarchy of massive higher spin states that provide an ultraviolet completion). They extend to give formulae for loop amplitudes{{Cite journal |last1=Adamo |first1=Tim |last2=Casali |first2=Eduardo |last3=Skinner |first3=David |date=2014-04-01 |title=Ambitwistor strings and the scattering equations at one loop |journal=Journal of High Energy Physics |language=en |volume=2014 |issue=4 |pages=104 |doi=10.1007/JHEP04(2014)104 |issn=1029-8479 |bibcode=2014JHEP...04..104A |arxiv=1312.3828 |s2cid=119194796}}{{Cite journal |last1=Geyer |first1=Yvonne |last2=Mason |first2=Lionel |last3=Monteiro |first3=Ricardo |last4=Tourkine |first4=Piotr |date=2015-09-16 |title=Loop Integrands for Scattering Amplitudes from the Riemann Sphere |journal=Physical Review Letters |volume=115 |issue=12 |pages=121603 |doi=10.1103/PhysRevLett.115.121603 |pmid=26430983 |bibcode=2015PhRvL.115l1603G |arxiv=1507.00321 |s2cid=36625491}} and can be defined on curved backgrounds.{{Cite journal |last1=Adamo |first1=Tim |last2=Casali |first2=Eduardo |last3=Skinner |first3=David |date=2015-02-01 |title=A worldsheet theory for supergravity |journal=Journal of High Energy Physics |language=en |volume=2015 |issue=2 |pages=116 |doi=10.1007/JHEP02(2015)116 |issn=1029-8479 |bibcode=2015JHEP...02..116A |arxiv=1409.5656 |s2cid=119234027}}

The twistor correspondence

Denote Minkowski space by $M$ , with coordinates $x^a = (t, x, y, z)$ and Lorentzian metric $\eta_{ab}$ signature $(1, 3)$ . Introduce 2-component spinor indices $A = 0, 1;\; A' = 0', 1',$ and set

: $x^{AA'} = \frac{1}{\sqrt{2}}\begin{pmatrix} t - z & x + iy \\ x - iy & t + z \end{pmatrix}.$

Non-projective twistor space $\mathbb{T}$ is a four-dimensional complex vector space with coordinates denoted by $Z^{\alpha} = \left(\omega^{A},\, \pi_{A'}\right)$ where $\omega^A$ and $\pi_{A'}$ are two constant Weyl spinors. The hermitian form can be expressed by defining a complex conjugation from $\mathbb{T}$ to its dual $\mathbb{T}^*$ by $\bar Z_\alpha = \left(\bar\pi_A,\, \bar \omega^{A'}\right)$ so that the Hermitian form can be expressed as

: $Z^\alpha \bar Z_\alpha = \omega^{A}\bar\pi_{A} + \bar\omega^{A'}\pi_{A'}.$

This together with the holomorphic volume form, $\varepsilon_{\alpha\beta\gamma\delta} Z^\alpha dZ^\beta \wedge dZ^\gamma \wedge dZ^\delta$ is invariant under the group SU(2,2), a quadruple cover of the conformal group C(1,3) of compactified Minkowski spacetime.

Points in Minkowski space are related to subspaces of twistor space through the incidence relation

: $\omega^{A} = ix^{AA'}\pi_{A'}.$

The incidence relation is preserved under an overall re-scaling of the twistor, so usually one works in projective twistor space $\mathbb{PT},$ which is isomorphic as a complex manifold to $\mathbb{CP}^3$ . A point $x\in M$ thereby determines a line $\mathbb{CP}^1$ in $\mathbb{PT}$ parametrised by $\pi_{A'}.$ A twistor $Z^\alpha$ is easiest understood in space-time for complex values of the coordinates where it defines a totally null two-plane that is self-dual. Take $x$ to be real, then if $Z^\alpha \bar Z_\alpha$ vanishes, then $x$ lies on a light ray, whereas if $Z^\alpha \bar Z_\alpha$ is non-vanishing, there are no solutions, and indeed then $Z^{\alpha}$ corresponds to a massless particle with spin that are not localised in real space-time.

Variations

=Supertwistors=

Supertwistors are a supersymmetric extension of twistors introduced by Alan Ferber in 1978.{{Citation|bibcode=1978NuPhB.132...55F|doi = 10.1016/0550-3213(78)90257-2|title=Supertwistors and conformal supersymmetry|year=1978|last1=Ferber|first1=A.|journal=Nuclear Physics B|volume=132|issue = 1|pages=55–64|postscript=. }} Non-projective twistor space is extended by fermionic coordinates where $\mathcal{N}$ is the number of supersymmetries so that a twistor is now given by $\left(\omega^A,\, \pi_{A'},\, \eta^i\right), i = 1, \ldots, \mathcal{N}$ with $\eta^i$ anticommuting. The super conformal group $SU(2,2|\mathcal{N})$ naturally acts on this space and a supersymmetric version of the Penrose transform takes cohomology classes on supertwistor space to massless supersymmetric multiplets on super Minkowski space. The $\mathcal{N} = 4$ case provides the target for Penrose's original twistor string and the $\mathcal{N} = 8$ case is that for Skinner's supergravity generalisation.

= Higher dimensional generalization of the Klein correspondence =

A higher dimensional generalization of the Klein correspondence underlying twistor theory, applicable to isotropic subspaces of conformally compactified (complexified) Minkowski space and its super-space extensions, was developed by J. Harnad and S. Shnider.

= Hyperkähler manifolds =

Hyperkähler manifolds of dimension $4k$ also admit a twistor correspondence with a twistor space of complex dimension $2k+1$ .{{cite journal|last4=Roček | first4=M. | last3=Lindström | first3=U. | last2=Karlhede | first2=A. | last1=Hitchin | first1=N. J. | title=Hyper-Kähler metrics and supersymmetry | url=https://projecteuclid.org/download/pdf_1/euclid.cmp/1104116624 |mr=877637 | year=1987 | journal=Communications in Mathematical Physics | issn=0010-3616 | volume=108 | issue=4 | pages=535–589 | doi=10.1007/BF01214418| bibcode=1987CMaPh.108..535H | s2cid=120041594 }}

=Palatial twistor theory=

The nonlinear graviton construction encodes only anti-self-dual, i.e., left-handed fields. A first step towards the problem of modifying twistor space so as to encode a general gravitational field is the encoding of right-handed fields. Infinitesimally, these are encoded in twistor functions or cohomology classes of homogeneity −6. The task of using such twistor functions in a fully nonlinear way so as to obtain a right-handed nonlinear graviton has been referred to as the (gravitational) googly problem.Penrose 2004, p. 1000. (The word "googly" is a term used in the game of cricket for a ball bowled with right-handed helicity using the apparent action that would normally give rise to left-handed helicity.) The most recent proposal in this direction by Penrose in 2015 was based on noncommutative geometry on twistor space and referred to as palatial twistor theory.{{Cite journal|doi=10.1098/rsta.2014.0237|title=Palatial twistor theory and the twistor googly problem|year=2015|last1=Penrose|first1=Roger|journal=Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences|volume=373|issue=2047|pmid=26124255|s2cid=13038470|page=20140237|bibcode=2015RSPTA.37340237P |doi-access=free}} The theory is named after Buckingham Palace, where Michael Atiyah[https://www.quantamagazine.org/20160303-michael-atiyahs-mathematical-dreams/ "Michael Atiyah's Imaginative State of Mind"] – Quanta Magazine suggested to Penrose the use of a type of "noncommutative algebra", an important component of the theory. (The underlying twistor structure in palatial twistor theory was modeled not on the twistor space but on the non-commutative holomorphic twistor quantum algebra.)

Notes

References

Roger Penrose (2004), The Road to Reality, Alfred A. Knopf, ch. 33, pp. 958–1009.
Roger Penrose and Wolfgang Rindler (1984), Spinors and Space-Time; vol. 1, Two-Spinor Calculus and Relativitic Fields, Cambridge University Press, Cambridge.
Roger Penrose and Wolfgang Rindler (1986), Spinors and Space-Time; vol. 2, Spinor and Twistor Methods in Space-Time Geometry, Cambridge University Press, Cambridge.

External links

Penrose, Roger (1999), "[http://online.itp.ucsb.edu/online/gravity99/penrose/ Einstein's Equation and Twistor Theory: Recent Developments]"
Penrose, Roger; Hadrovich, Fedja. "[http://users.ox.ac.uk/~tweb/00006/index.shtml Twistor Theory.]"
Hadrovich, Fedja, "[http://users.ox.ac.uk/~tweb/00004/ Twistor Primer.]"
Penrose, Roger. "[http://users.ox.ac.uk/~tweb/00001/index.shtml On the Origins of Twistor Theory.]"
Jozsa, Richard (1976), "[http://users.ox.ac.uk/~tweb/00003/index.shtml Applications of Sheaf Cohomology in Twistor Theory.]"
{{cite journal |last=Dunajski |first=Maciej |title=Twistor Theory and Differential Equations |arxiv=0902.0274 |date=2009 |journal=J. Phys. A: Math. Theor. |volume=42 |issue=40 |page=404004 |doi=10.1088/1751-8113/42/40/404004 |bibcode=2009JPhA...42N4004D |s2cid=62774126 }}
Andrew Hodges, [https://www.twistordiagrams.org.uk/papers/index.html Summary of recent developments.]
Huggett, Stephen (2005), "[http://people.maths.ox.ac.uk/lmason/Tws/Huggett.pdf The Elements of Twistor Theory.]"
Mason, L. J., "[http://www.theorie.physik.uni-muenchen.de/Twistor/twistor_files/Talks/Mason.pdf The twistor programme and twistor strings: From twistor strings to quantum gravity?]"
{{cite thesis |type=PhD |last=Sämann |first=Christian |date=2006 |title=Aspects of Twistor Geometry and Supersymmetric Field Theories within Superstring Theory |arxiv=hep-th/0603098 |publisher=Universität Hannover}}
Sparling, George (1999), "[https://www.mat.univie.ac.at/~esiprpr/esi731.pdf On Time Asymmetry.]"
{{cite web |last=Spradlin |first=Marcus |date=2012 |url=https://conservancy.umn.edu/bitstream/handle/11299/130081/1/spradlin.pdf |title=Progress and Prospects in Twistor String Theory |hdl=11299/130081 }}
[http://mathworld.wolfram.com/Twistor.html MathWorld: Twistors.]
Universe Review: "[http://universe-review.ca/R15-19-twistor.htm Twistor Theory.]"
[http://people.maths.ox.ac.uk/lmason/Tn/ Twistor newsletter] archives.