Twistor Characterization of Stationary Axisymmetric Solutions of Einstein's Equations

Abstract

Introduction One of the nonlinear systems that can be ‘solved’ by twistor methods is a reduced form of Einstein's vacuum equations for gravitational fields with two commuting Killing vectors. It is an intriguing example because it remains one of the central aims of twistor theory to tackle the full Einstein equations without any special assumptions about symmetry or self-duality. The solution of the reduced problem is a step towards achieving this. However, unlike the nonlinear graviton [11], which was based on a direct generalization of the familiar geometry of flat twistor space, the construction in this case is indirect and ungeometric. It was developed by Ward [18], who followed up Witten's observation [19] that the Ernst equation [3] is equivalent to a reduction of the self-dual Yang-Mills equations. Ward's twistor analysis of stationary axisymmetric fields has been extended in two papers. The first (Woodhouse and Mason [21]) describes the connection with the solution generation techniques in relativity and uses twistor theory to ‘explain’ the occurrence of Riemann-Hilbert problems in the construction of exact solutions (the solution generation techniques are reviewed by Cosgrove [2] and in a collection of articles edited by Hoenselaers and Dietz [5]). The second (Woodhouse [20]) applies Ward's construction to gravitational waves with cylindrical symmetry. The connection between the twistor geometry and the space-time geometry remains obscure and it is still possible that the construction reflects no more than an accidental correspondence between equations.