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A paperback edition of a classic text, this book gives a unique
survey of the known solutions of Einstein's field equations for
vacuum, Einstein-Maxwell, pure radiation and perfect fluid sources.
It introduces the foundations of differential geometry and
Riemannian geometry and the methods used to characterize, find or
construct solutions. The solutions are then considered, ordered by
their symmetry group, their algebraic structure (Petrov type) or
other invariant properties such as special subspaces or tensor
fields and embedding properties. Includes all the developments in
the field since the first edition and contains six completely new
chapters, covering topics including generation methods and their
application, colliding waves, classification of metrics by
invariants and treatments of homothetic motions. This book is an
important resource for graduates and researchers in relativity,
theoretical physics, astrophysics and mathematics. It can also be
used as an introductory text on some mathematical aspects of
general relativity.
Thoroughly revised and updated, this textbook provides a
pedagogical introduction to relativity. It is self-contained, but
the reader is expected to have a basic knowledge of theoretical
mechanics and electrodynamics. It covers the most important
features of both special and general relativity, as well as
touching on more difficult topics, such as the field of charged
pole-dipole particles, the Petrov classification, groups of
motions, gravitational lenses, exact solutions and the structure of
infinity. The necessary mathematical tools (tensor calculus,
Riemannian geometry) are provided, most of the derivations are
given in full, and exercises are included where appropriate.
Written as a textbook for undergraduate and introductory graduate
courses, it will also be of use to researchers working in the
field. The bibliography gives the original papers and directs the
reader to useful monographs and review papers.
In many branches of physics, mathematics, and engineering, solving a problem means solving a set of ordinary or partial differential equations. Nearly all methods of constructing closed form solutions rely on symmetries. The emphasis in this text is on how to find and use the symmetries; this is supported by many examples and more than 100 exercises. This book will form an introduction accessible to beginning graduate students in physics, applied mathematics, and engineering. Advanced graduate students and researchers in these disciplines will find the book a valuable reference.
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