Sprache: Englisch
Verlag: Cambridge University Press, 2005
ISBN 10: 0521673526 ISBN 13: 9780521673525
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
EUR 70,27
Anzahl: Mehr als 20 verfügbar
In den WarenkorbZustand: New. In.
Sprache: Englisch
Verlag: Cambridge University Press, 2005
ISBN 10: 0521673526 ISBN 13: 9780521673525
Anbieter: Kennys Bookstore, Olney, MD, USA
EUR 134,08
Anzahl: Mehr als 20 verfügbar
In den WarenkorbZustand: New. The first book to show how modern dynamical systems theory can help us both in understanding the evolution of cosmological models, and in relating them to real cosmological observations. Editor(s): Wainwright, J.; Ellis, G. F. R. Num Pages: 360 pages, 34 b/w illus. 4 tables. BIC Classification: PBW; PGK. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 19. Weight in Grams: 570. . 2008. paperback. . . . . Books ship from the US and Ireland.
Sprache: Englisch
Verlag: Cambridge University Press, 2005
ISBN 10: 0521673526 ISBN 13: 9780521673525
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This authoritive volume shows how modern dynamical systems theory can help us in understanding the evolution of cosmological models. It also compares this approach with Hamiltonian methods and numerical studies. A major part of the book deals with the spatially homogeneous (Bianchi) models and their isotropic subclass, the Friedmann-Lemaitre models, but certain classes of inhomogeneous models (for example 'silent universes') are also examined. The analysis leads to an understanding of how special (high symmetry) models determine the evolution of more general families of models; and how these families relate to real cosmological observations. This is the first book to relate modern dynamical systems theory to both cosmological models and cosmological observations. It provides an invaluable reference for graduate students and researchers in relativity, cosmology and dynamical systems theory.