Twistor space

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Short description: Space in mathematics and theoretical physics

In mathematics and theoretical physics (especially twistor theory), twistor space is the complex vector space of solutions of the twistor equation ∇A′(AΩB)=0. It was described in the 1960s by Roger Penrose and Malcolm MacCallum.[1] According to Andrew Hodges, twistor space is useful for conceptualizing the way photons travel through space, using four complex numbers. He also posits that twistor space may aid in understanding the asymmetry of the weak nuclear force.[2]

Informal motivation

In the (translated) words of Jacques Hadamard: "the shortest path between two truths in the real domain passes through the complex domain." Therefore when studying four-dimensional space ℝ4 it might be valuable to identify it with ℂ2. However, since there is no canonical way of doing so, instead all isomorphisms respecting orientation and metric between the two are considered. It turns out that complex projective 3-space ℂℙ3 parametrizes such isomorphisms together with complex coordinates. Thus one complex coordinate describes the identification and the other two describe a point in ℝ4. It turns out that vector bundles with self-dual connections on ℝ4(instantons) correspond bijectively to holomorphic vector bundles on complex projective 3-space ℂℙ3.

Formal definition

For Minkowski space, denoted 𝕄, the solutions to the twistor equation are of the form

ΩA(x)=ωA−ixAA′πA′

where ωA and πA′ are two constant Weyl spinors and xAA′=σμAA′xμ is a point in Minkowski space. The σμ=(I,σ→) are the Pauli matrices, with A,A′=1,2 the indexes on the matrices. This twistor space is a four-dimensional complex vector space, whose points are denoted by Zα=(ωA,πA′), and with a hermitian form

Σ(Z)=ωAπ¯A+ω¯A′πA′

which is invariant under the group SU(2,2) which is 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

ωA=ixAA′πA′.

This incidence relation is preserved under an overall re-scaling of the twistor, so usually one works in projective twistor space, denoted ℙ𝕋, which is isomorphic as a complex manifold to ℂℙ3.

Given a point x∈M it is related to a line in projective twistor space where we can see the incidence relation as giving the linear embedding of a ℂℙ1 parametrized by πA′.

The geometric relation between projective twistor space and complexified compactified Minkowski space is the same as the relation between lines and two-planes in twistor space; more precisely, twistor space is

𝕋:=ℂ4.

It has associated to it the double fibration of flag manifolds ℙ←μ𝔽→ν𝕄 where ℙ is the projective twistor space

ℙ=F1(𝕋)=ℂℙ3=𝐏(ℂ4)

and 𝕄 is the compactified complexified Minkowski space

𝕄=F2(𝕋)=Gr2(ℂ4)=Gr2,4(ℂ)

and the correspondence space between ℙ and 𝕄 is

𝔽=F1,2(𝕋)

In the above, 𝐏 stands for projective space, Gr a Grassmannian, and F a flag manifold. The double fibration gives rise to two correspondences (see also Penrose transform), c=ν∘μ−1 and c−1=μ∘ν−1.

The compactified complexified Minkowski space 𝕄 is embedded in 𝐏5≅𝐏(∧2𝕋) by the Plücker embedding; the image is the Klein quadric.

See also

References

  • Ward, R.S.; Wells, R.O. (1991). Twistor Geometry and Field Theory. Cambridge University Press. ISBN 0-521-42268-X. 
  • Huggett, S.A.; Tod, K.P. (1994). An introduction to twistor theory. Cambridge University Press. ISBN 978-0-521-45689-0.