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Statistical physics for cosmic structures.
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Statistical physics for cosmic structures.

Erschienen 2005. - Hardcover/Pappeinband.

XIII, 424 pages with ill.; 24 cm. Like new. Shrink wrapped. / Wie neu. In Folie verschweißt.
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Kosmologie ; Statistische Physik, Astronomie, Kartographie

Produktart:
📚 Bücher
Autor(en):
Gabrielli, Andrea, Francesco Sylos Labini Michael Joyce a. o.:
Anbieter:
Antiquariat Thomas Haker GmbH & Co. KG
Bestell-Nr.:
815266
Lagerfach:
A
Katalog:
Astronomie
ISBN | EAN:
3540407456 | 9783540407454
Stichworte:
Kosmologie, Statistische, Physik, Astronomie, Kartographie
Zahlungsarten:
Rechnung/Überweisung (Vorauszahlung vorbehalten), Visa, Euro-Card Master-Card, PayPal
Gebraucht, wie neu17,30 EURKostenloser Versand
Statistical physics for cosmic structures.
Statistical physics for cosmic structures.
Gebraucht, wie neu
17,30 EUR
Kostenloser Versand
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.
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