Skip to main content Accessibility help
×
Hostname: page-component-68945f75b7-qvshk Total loading time: 0 Render date: 2024-08-05T17:24:03.829Z Has data issue: false hasContentIssue false

14 - Twistor Characterization of Stationary Axisymmetric Solutions of Einstein's Equations

Published online by Cambridge University Press:  05 May 2013

J. Fletcher
Affiliation:
Mathematical Institute
N.M.J. Woodhouse
Affiliation:
Wadham College, Oxford,
Get access

Summary

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.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 1990

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×