E-Book, Englisch, 454 Seiten
Vittorio Cosmology
1. Auflage 2017
ISBN: 978-1-4987-3133-1
Verlag: CRC Press
Format: PDF
Kopierschutz: Adobe DRM (»Systemvoraussetzungen)
E-Book, Englisch, 454 Seiten
Reihe: Series in Astronomy and Astrophysics
ISBN: 978-1-4987-3133-1
Verlag: CRC Press
Format: PDF
Kopierschutz: Adobe DRM (»Systemvoraussetzungen)
Modern cosmology has changed significantly over the years, from the discovery to the precision measurement era. The data now available provide a wealth of information, mostly consistent with a model where dark matter and dark energy are in a rough proportion of 3:7. The time is right for a fresh new textbook which captures the state-of-the art in cosmology.
Written by one of the world's leading cosmologists, this brand new, thoroughly class-tested textbook provides graduate and undergraduate students with coverage of the very latest developments and experimental results in the field. Prof. Nicola Vittorio shows what is meant by precision cosmology, from both theoretical and observational perspectives.
This book is divided into three main parts:
- Part I provides a pedagogical, but rigorous, general relativity-based discussion of cosmological models, showing the evidence for dark energy, the constraints from primordial nucleosynthesis and the need for inflation
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Part II introduces density fluctuations and their statistical description, discussing different theoretical scenarios, such as CDM, as well as observations
- Part III introduces the general relativity approach to structure formation and discusses the physics behind the CMB temperature and polarization pattern of the microwave sky
Carefully adapted from the course taught by Prof. Vittorio at the University of Rome Tor Vergata, this book will be an ideal companion for advanced students undertaking a course in cosmology.
Autoren/Hrsg.
Fachgebiete
Weitere Infos & Material
Section I: The Background Universe
Cosmological Models
Testing FLRW Models
The Hot Big-Bang Model
Inflation
Section II: Structure Formation: a Newtonian Approach
The Gravitational Instability Scenario
Density Fluctuations: Statistical Tools and Observables
The Luminous Universe
A Dark Universe
Section III: Structure Formation: a Relativistic Approach
The Lemaitre-Tolman-Bondi Solution
Structure Formation: a Relativistic Approach I
Structure Formation: a Relativistic Approach II
CMB Temperature Anisotropy
CMB Polarisation
Section IV: Future Perspectives.
Precision Cosmology
Appendix 1: Tensors
Appendix 2: Riemannian Spaces
Appendix 3: Curvature of Space
Appendix 4: From Special to General Relativity
Appendix 5: Fields Equation in the Vacuum
Appendix 6: Fields Equation in a Non-empty Space