Statistical Physics for Cosmic Structures

Language: English

Published by Springer, 2004

3540407456 / 9783540407454

Series: Book 4 of 241 - Lecture Notes in Physics

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Seller: AHA-BUCH GmbH, Einbeck, GermanyAHA-BUCH GmbH

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Druck auf Anfrage Neuware - Printed after ordering - This book has its roots in a series of collaborations in the last decade at the interface between statistical physics and cosmology. The speci c problem which initiated this research was the study of the clustering properties of galaxies as revealed by large redshift surveys, a context in which concepts of modern statistical physics (e. g. scale-invariance, fractality. . ) nd ready application. In recent years we have considerably broadened the range of problems in cosmology which we have addressed, treating in particular more theoretical issues about the statistical properties of standard cosmological models. What is common to all this research, however, is that it is informed by a perspective and methodology which is that of statistical physics. We can say that, beyond its speci c scienti c content, this book has an underlying thesis: such interdisciplinary research is an exciting playground for statistical physics, and one which can bring new and useful insights into cosmology. Thebook does not represent a nal point, but in our view, a marker in the development of this kind of research, which we believe can go very much further in the future. Indeed as we complete this book, new developments - which unfortunately we have not been able to include here - have been made on some of the themes described here. Our focus in this book is on the problem of structure in cosmology.

Seller Inventory # 9783540407454

Title
Statistical Physics for Cosmic Structures
Author
Andrea Gabrielli
Publisher
Springer
Publication year
2004
Condition
Neu
Binding
Buch
Language
English
ISBN 10
3540407456
ISBN 13
9783540407454
Item weight
910 grams
Dimensions
241x160x33 mm
Series
Book 4 of 241: Lecture Notes in Physics

AHA-BUCH GmbH

Einbeck, Germany

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AbeBooks seller since August 14, 2006

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