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Dynamical systems in cosmology / edited by J. Wainwright, G.F.R. Ellis

Contributor(s): Publisher: Cambridge : New York : Cambridge University Press, 1997Description: xiv, 343 páginas : gráficos, tablasContent type:
  • texto
Media type:
  • no mediado
Carrier type:
  • volumen
ISBN:
  • 978-0-521-67352-5
Subject(s): DDC classification:
  • 523.101515352 D997s 21
Contents:
Part I. background - Part II. Spatially homogeneous cosmologies - Part III. Inhomogeneous cosmologies - Part IV. Conclusion
Summary: This authoritative 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.
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Item type Current library Collection Call number Status Notes Date due Barcode
Libros Impresos Libros Impresos Ciencias e ingeniería Circulación Proyecto 523.101515352 D997s (Browse shelf(Opens below)) Checked out UPA 22991-LFC 31/10/2026 2025-0323

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Part I. background - Part II. Spatially homogeneous cosmologies - Part III. Inhomogeneous cosmologies - Part IV. Conclusion

This authoritative 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.

Texto en inglés

Encargado de S.A.I | Teléfono: (32)2205911 |Anexo: 5911 | Correo: jonnathan.isla@upla.cl

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