Description |
1 online resource (xiii, 424 pages) : illustrations |
Contents |
Introduction; Uniform and Correlated Mass Density Fields; The Power Spectrum and the Classification of Stationary Stochastic Fields; Fractals; Multifractals and Mass Distributions; Fluctuations in Standard Cosmological Models: A Real Space View; Discrete Representation of Fluctuations in Cosmological Models; Galaxy Surveys: An Introduction to Their Analysis; Characterizing the Observed Distribution of Visible Matter I: The Conditional Average Density in Galaxy Catalogs; Characterizing the Observed Distribution of Visible Matter II: Number Counts and Their Fluctuations |
Summary |
"This book has been conceived as a methodological monograph in which the main methods of modern statistical physics for cosmological structures and density fields (galaxies, Cosmic Microwave Background Radiation, etc.) are presented in detail. The main purpose is to present clearly, to a workable level, these methods, with a certain mathematical accuracy, providing also some paradigmatic examples of applications. This should result in a new and more general framework for the statistical analysis of the many new data concerning the different cosmic structures which characterize the large scale Universe and for their theoretical interpretation and modeling."--Jacket |
Bibliography |
Includes bibliographical references (pages 413-420) and index |
Notes |
English |
In |
OhioLINK electronic book center |
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SpringerLink |
Subject |
Cosmology -- Statistical methods
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Statistical physics.
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Astronomy.
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Astronomy
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astronomy.
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SCIENCE -- Cosmology.
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Cosmology -- Statistical methods.
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Statistical physics.
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Physique.
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Astronomie.
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Statistical physics
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Cosmologia.
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Mecânica estatística.
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Form |
Electronic book
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Author |
Gabrielli, A. (Andrea)
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ISBN |
3540407456 |
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9783540407454 |
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3540269991 |
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9783540269991 |
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6610461570 |
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9786610461578 |
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1280461578 |
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9781280461576 |
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