J. Heidmann

Relativistic Cosmology

An Introduction
Übersetzung: Mitton, S.; Mitton, J.

• Broschiertes Buch

Produktbeschreibung

Since the first French edition of the book emphasized rather the solid facts of Cosmology than the detailed discussions of controversial results, relatively few revisions were necessary for the English edition. They were made early in 1979 and affected about 5% of the text. The main revisions referred to the distance scale, the dlstribution of galaxies, the X-ray observations of clusters, the cosmic time evolution of quasars and radiogalaxies and the 3 K radiation. A new short bibliography presents the recent articles and the latest proceedings of Symposia; from these the reader can easily trace a more complete list of refer ences. I am happy to thank Professor Beiglbock for suggestions he made to improve Part lIon Spaces of Constant Curvature, and Drs. S. and J. Mitton for translating the manuscript into English. I also thank with pleasure Marie-Ange Sevin for correcting the final version. J. Heidmann March 1980, Meudon, France Preface The aim of this book is to present the fundamentals of cosmology. Its subject is the study of the universe on a grand scale: - on a grand distance scale, since from the start, we shall be escaping the con fines of our own Galaxy to explore space as far as the limits of the observable universe, some ten thousand million light years away; - and on a grand time scale, as we shall look back into the past to the very first moments of the initial expansion, about twelve thousand million years ago.

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Produktdetails

• Verlag: Springer / Springer Berlin Heidelberg / Springer, Berlin
• Artikelnr. des Verlages: 978-3-540-10138-3
• 1980.
• Seitenzahl: 188
• Erscheinungstermin: 1. September 1980
• Englisch
• Abmessung: 244mm x 170mm x 11mm
• Gewicht: 310g
• ISBN-13: 9783540101383
• ISBN-10: 3540101381
• Artikelnr.: 25651679

Inhaltsangabe

I: The Metagalaxy out to a Distance of One Gigaparsec.- 1. Distance Scale.- 1.1 Cepheids.- 1.2 H II Regions.- 1.3 Luminosity Classes.- 1.4 The Diameter - Luminosity Relation.- 1.5 Groups of Galaxies.- 2. The Distribution of Galaxies in Space.- 2.1 The Local Group.- 2.2 The Nearby Groups.- 2.3 The Virgo Cluster.- 2.4 The Coma Cluster.- 2.5 Rich Clusters.- 2.6 Superclusters.- 2.7 Gradients.- 3. The Expansion of the Universe.- 3.1 The Nature of the Expansion.- 3.2 The Value of the Hubble Constant.- 4. Nearby Intergalactic Matter.- 4.1 Optical Observations.- 4.2 21-cm Radio Observations.- 4.3 X-Ray Observations.- 5. The Density of the Universe.- 5.1 The Contribution of Galaxies.- 5.2 The Contribution of Intergalactic Material.- 5.3 Other Contributions.- 5.4 The Density of the Universe.- 6. The Age of the Universe.- II: Spaces with Constant Curvature.- 7. Locally Euclidean Spaces.- 7.1 Natural Frame.- 7.2 The Riemann-Christoffel Tensor.- 7.3 Locally Euclidean Space.- 7.4 Development.-

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I: The Metagalaxy out to a Distance of One Gigaparsec.- 1. Distance Scale.- 2. The Distribution of Galaxies in Space.- 3. The Expansion of the Universe.- 4. Nearby Intergalactic Matter.- 5. The Density of the Universe.- 6. The Age of the Universe.- II: Spaces with Constant Curvature.- 7. Locally Euclidean Spaces.- 8. Locally Non-Euclidean Spaces.- 9. Spherical and Hyperbolic Spaces.- III: Model Universes.- 10. Uniform Relativistic Model Universes.- 11. Theory of Observations in the Relativistic Zone.- 12. The Cosmological Constant.- 13. Cosmological Horizons.- IV: The Metagalaxy in the Relativistic Zone.- 14. The Hubble Diagram for Galaxies.- 15. Distant Intergalactic Material.- 16. Radio Galaxies and Quasars.- 17. The Cosmic Microwave Background.- Numerical Constants.