The Cosmic Microwave Background

The Cosmic Microwave Background

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Opis: The Cosmic Microwave Background

This volume presents the lectures of the nineteenth Canary Islands Winter School, dedicated to the Cosmic Microwave Background (CMB). This relict radiation from the very early Universe provides a fundamental tool for precision cosmology. Prestigious researchers in the field present a comprehensive overview of current knowledge of the CMB, reviewing the theoretical foundations, the main observational results and the most advanced statistical techniques used in this discipline. The lectures give coverage from the basic principles to the most recent research results, reviewing state of the art observational and statistical analysis techniques. The impact of new experiments and the constraints imposed on cosmological parameters are emphasized and put into the broader context of research in cosmology. This is an important resource for both graduate students and experienced researchers, revealing the spectacular progress that has been made in the study of the CMB within the last decade. 'This volume would make highly recommended reading for research students in cosmology, and would not look amiss on the bookshelf of the seasoned researcher as a handy reference.' The ObservatoryList of contributors; List of participants; Preface; Acknowledgements; 1. CMB observations and cosmological constraints Bruce Partridge; 2. The inflationary universe Sabino Matarrese; 3. CMB theory from nucleosynthesis to recombination Wayne Hu; 4. CMB fluctuations in the post-recombination universe Matthias Bartelmann; 5. Statistical techniques for data analysis in cosmology Licia Verde; 6. Gaussianity Enrique Martinez-Gonzalez; 7. Galactic and extragalactic foregrounds Rodney D. Davies; 8. Probes of fundamental cosmology Malcolm Longair.


Szczegóły: The Cosmic Microwave Background

Tytuł: The Cosmic Microwave Background
Producent: Cambridge University Press
ISBN: 9780521764537
Rok produkcji: 2009
Ilość stron: 318
Oprawa: Twarda
Waga: 0.78 kg


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