Brossura

ISBN 10: 0470848359 ISBN 13: 9780470848357

Casa editrice: Wiley, 2003

An Introduction to Modern Cosmology Third Edition is an accessible account of modern cosmological ideas. The Big Bang Cosmology is explored, looking at its observational successes in explaining the expansion of the Universe, the existence and properties of the cosmic microwave background, and the origin of light elements in the universe. Properties of the very early Universe are also covered, including the motivation for a rapid period of expansion known as cosmological inflation. The third edition brings this established undergraduate textbook up-to-date with the rapidly evolving observational situation.

This fully revised edition of a bestseller takes an approach which is grounded in physics with a logical flow of chapters leading the reader from basic ideas of the expansion described by the Friedman equations to some of the more advanced ideas about the early universe. It also incorporates up-to-date results from the Planck mission, which imaged the anisotropies of the Cosmic Microwave Background radiation over the whole sky. The Advanced Topic sections present subjects with more detailed mathematical approaches to give greater depth to discussions. Student problems with hints for solving them and numerical answers are embedded in the chapters to facilitate the reader’s understanding and learning.

Cosmology is now part of the core in many degree programs. This current, clear and concise introductory text is relevant to a wide range of astronomy programs worldwide and is essential reading for undergraduates and Masters students, as well as anyone starting research in cosmology.

From the Back Cover:

An Introduction to Modern Cosmology Second Edition is an accessible account of modern cosmological ideas.  The Big Bang Cosmology is explored, looking at its observational successes in explaining the expansion and age of the universe, the existence and properties of the cosmic microwave background, and the origin of the light elements in the universe.  Properties of the very early universe are also covered, including the motivation for the theory known as cosmological inflation.  The Second Edition includes additiional material on observational cosmology and structure formation.

• Approach grounded in physics rather than mathematics.
• Worked examples, student problems, hints for solving them and numerical answers.
• Latest observational results including WMAP satellite.
• New website with updates, full colour images and links to further information.

Published reviews of the First Edition:

"..a clear, concise and accessible book" New Scientist

"...one of the clearest introductions to cosmology on the market"  Contemporary Physics

About the Author:

Andrew Liddle is Professor of Astrophysics at the University of Sussex. Research interests include the origin and evolution of structure in the universe and the relation between astronomical observations and the physics of the early universe.