

Lecture note 29/2006
Ernst Equation and Riemann Surfaces - Analytical and Numerical Methods
Christian Klein and Olaf Richter
Contact the author: Please use for correspondence this email.
Submission date: 12. Jan. 2006
Pages: 259
published as:
Klein, Chr. and O. Richter (eds.): Ernst equation and Riemann surfaces : analytical and numerical methods
Berlin [u.a.] : Springer, 2005. - X, 249 p.
(Lecture notes in physics ; 685)
ISBN 978-3-540-28589-2 - ISBN 3-540-28589-x
Bibtex
MSC-Numbers: 83C15, 37K20
PACS-Numbers: 04.20.Jb
Download full preprint: PDF (7416 kB)
Abstract:
Exact solutions to Einstein's equations
have been useful for the understanding of
general relativity in many respects. They
have led to physical concepts as black
holes and event horizons and helped to
visualize interesting features of the theory.
In addition they have been used to test the
quality of various approximation methods
and numerical codes. The most powerful
solution generation methods are due to
the theory of Integrable Systems. In the
case of axisymmetric stationary spacetimes
the Einstein equations are equivalent to
the completely integrable Ernst equation.
In this volume these solutions to the Ernst
equation are studied in detail and physical
and mathematical aspects of this class are
discussed both analytically and numerically.The original publication is available at Springer-Online: www.springeronline.com/3-540-28589-X.