Frauendiener J., Guilini D., Perlick V. (eds.) Analytical and numerical approaches to mathematical relativity (LNP692, Springer, 2006)(290s)_PGr_.pdf

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Jörg Frauendiener
Domenico J.W. Giulini
Volker Perlick
(Eds.)
Analytical and Numerical
Approaches to
Mathematical Relativity
With a Foreword by Roger Penrose
ABC
Editors
Jörg Frauendiener
Institut für Theoretische Astrophysik
Universität Tübingen
Auf der Morgenstelle 10
72076 Tübingen, Germany
E-mail: joergf@tat.physik.uni-
tuebingen.de
Volker Perlick
Institut für Theoretische Physik
TU Berlin
Hardenbergstrasse 36
10623 Berlin
E-mail: vper0433@itp.physik.tu-
berlin.de
Domenico J.W. Giulini
Fakultät für Physik und Mathematik
Universität Freiburg
Hermann-Herder-Str. 3
79104 Freiburg, Germany
E-mail: giulini@physik.uni-freiburg.de
J. Frauendiener et al., Analytical and Numerical Approaches to Mathematical Relativity ,
Lect. Notes Phys. 692 (Springer, Berlin Heidelberg 2006), DOI 10.1007/b11550259
Library of Congress Control Number: 2005937899
ISSN 0075-8450
ISBN-10
3-540-31027-4 Springer Berlin Heidelberg New York
ISBN-13
978-3-540-31027-3 Springer Berlin Heidelberg New York
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Foreword
The general theory of relativity, as formulated by Albert Einstein in 1915,
provided an astoundingly original perspective on the physical nature of grav-
itation, showing that it could be understood as a feature of a curvature in
the four-dimensional continuum of space-time. Now, some 90 years later, this
extraordinary theory stands in superb agreement with observation, provid-
ing a profound accord between the theory and the actual physical behavior
of astronomical bodies, which sometimes attains a phenomenal precision (in
one case to about one part in one hundred million million, where several dif-
ferent non-Newtonian effects, including the emission of gravitational waves,
are convincingly confirmed). Einstein’s tentative introduction, in 1917, of an
additional term in his equations, specified by a “cosmological constant”, ap-
pears now to be observationally demanded, and with this term included, there
is no discrepancy known between Einstein’s theory and classical dynamical
behavior, from meteors to matter distributions at the largest cosmological
scales. One of Einstein’s famous theoretical predictions that light is bent in
a gravitational field (which had been only roughly confirmed by Eddington’s
solar eclipse measurements at the Island of Principe in 1919, but which is now
very well established) has become an important tool in observational cosmol-
ogy, where gravitational lensing now provides a unique and direct means of
measuring the mass of very distant objects.
But long before general relativity and cosmology had acquired this im-
pressive observational status, these areas had provided a prolific source of
mathematical inspiration, particularly in differential geometry and the the-
ory of partial differential equations (where sometimes this had been applied
to situations in which the number of space-time dimensions differs from the
four of direct application to our observed space-time continuum). As we see
from several of the articles in this book, there is still much activity in all
these mathematical areas, in addition to other areas which have acquired
importance more recently. Most particularly, the interest in black holes, with
their horizons, their singularities, and their various other remarkable proper-
ties, both theoretical and in relation to observed highly dramatic astronom-
ical phenomena, has also stimulated much important research. Some have
interesting mathematical implications, involving particular types of mathe-
matical argumentations, such as the involvement of differential topology and
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