12.07.2015 Views

100 Years of Relativity Space-Time Structure: Einstein and Beyond ...

100 Years of Relativity Space-Time Structure: Einstein and Beyond ...

100 Years of Relativity Space-Time Structure: Einstein and Beyond ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

The Twistor Approach to <strong>Space</strong>-<strong>Time</strong> <strong>Structure</strong>s 489so if one vanishes so must the other, whence C abcd as a whole must vanish— the condition for (local) conformal flatness. It may be remarked, however,that in the positive-definite case (signature+ + ++) x <strong>and</strong> the splitsignaturecase (signature + + −−) y there is a large family <strong>of</strong> conformally(anti-)self-dual 4-manifolds. These spaces, <strong>and</strong> their twistor spaces, havea considerable pure-mathematical interest, z there being (different) “realityconditions” on each <strong>of</strong> the independent quantities Φ ABCD <strong>and</strong> X A′ B ′ C ′ D ′in these two cases.Yet, complex (anti-)self-spaces are by no means devoid <strong>of</strong> physical interest,especially those which can arise from deformations <strong>of</strong> (parts <strong>of</strong>) T forwhich F has the special form F = ε AB ∂f/∂ω A ∂/∂ω B , as given at the beginning<strong>of</strong> this section. We note that, in these cases, the operator ∂/∂π A ′ doesnot appear, <strong>and</strong> it follows that its infinitesimal action on Z α = (ω A , π A ′)leaves π A ′ unaffected. Thus, F generates a deformation <strong>of</strong> (part <strong>of</strong>) T thatpreserves the projectionF : T → ¯S ∗ ,(where ¯S ∗ is the complex conjugate <strong>of</strong> the dual S ∗ <strong>of</strong> the spin space S; notethat S is the space <strong>of</strong> 2-spinors like ω A , <strong>and</strong> ¯S ∗ is the space <strong>of</strong> those likeπ A ′). In each coordinate patch U i , with st<strong>and</strong>ard twistor coordinates, thisprojection takes the form(ω A , π A ′) ↦→ π A ′ ,<strong>and</strong> this now extends to a projection F that applies to the whole (nonprojective)curved twistor spaceF : T → ¯S ∗The inverse F −1 <strong>of</strong> this projection is a fibration <strong>of</strong> PT , each fibre being theentire complex 2-surface in T which projects down to a particular π in ¯S ∗ .In this case, the lines in PT can be neatly characterized as the projectiveversions <strong>of</strong> the holomorphic cross-sections <strong>of</strong> this fibration. These are theresults <strong>of</strong> maps R : ¯S∗ → T (whose composition F ◦ R with F is theidentity on ¯S ∗ ) which lift ¯S ∗ back into PT , <strong>and</strong> they generalize what in thecanonical flat case would be expressed as π A ′ ↦→ (ir AA′ π A ′, π A ′), where r ais the position vector <strong>of</strong> the point in CM that this cross-section defines.(Note the appearance <strong>of</strong> the basic incidence relation <strong>of</strong> §2.)The 2-surfaces <strong>of</strong> this fibration have tangent directions annihilated bya simple closed 2-form τ which is ( 1 2×) the exterior derivative <strong>of</strong> a 1-formι (<strong>of</strong> homogeneity degree 2):2τ = dι , ι ∧ τ = 0

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!