Abstract
Penrose has given a twistor description of all self-dual complex Riemannian space-times. We modify his construction to characterize all complex Riemannian space-times and all complex teleparallel space-times. This construction may be useful in finding non-self-dual solutions to the gravitational field equations (Einstein's or otherwise) without or with sources. It may also lead to a nonperturbative method for computing path integrals. Whereas Penrose shows that a self-dual space-time may be specified by a deformation of projective twistor space (the set of α planes in complex Minkowski space), we find that a Riemannian or teleparallel space-time may be described by a deformation of projective ambitwistor space (the set of null geodesics in complex Minkowski space).
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This essay received Fifth Award from the Gravity Research Foundation for the year 1981-Ed.
Research supported in part by DOE contract DOE AM 03-76SF00034.
Chaim Weizmann fellow.
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Yasskin, P.B., Isenberg, J.A. Non-self-dual nonlinear gravitons. Gen Relat Gravit 14, 621–627 (1982). https://doi.org/10.1007/BF00761453
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DOI: https://doi.org/10.1007/BF00761453