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The Primordial Density Perturbation: Cosmology, Inflation and the Origin of Structure, by David H. Lyth, Andrew R. Liddle
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The origin and evolution of the primordial perturbation is the key to understanding structure formation in the earliest stages of the Universe. It carries clues to the types of physical phenomena active in that extreme high-density environment. Through its evolution, generating first the observed cosmic microwave background anisotropies and later the distribution of galaxies and dark matter in the Universe, it probes the properties and dynamics of the present Universe. This graduate-level textbook gives a thorough account of theoretical cosmology and perturbations in the early Universe, describing their observational consequences and showing how to relate such observations to primordial physical processes, particularly cosmological inflation. With ambitious observational programmes complementing ever-increasing sophistication in theoretical modelling, cosmological studies will remain at the cutting edge of astrophysical studies for the foreseeable future.
- Sales Rank: #1723315 in eBooks
- Published on: 2009-06-11
- Released on: 2009-06-11
- Format: Kindle eBook
Review
"...a welcome addition to the growing collection of advanced cosmology textbooks. The two authors have made major contributions to the field, and their presentation is lucid and modern. Their volume warrants a place on the shelves of all researchers in advanced cosmology...." - Physics Today
About the Author
David H. Lyth is Professor of Particle Astrophysics in the Physics Department at Lancaster University.
Andrew R. Liddle is Professor of Astrophysics in the Department of Physics and Astronomy at the University of Sussex.
Most helpful customer reviews
8 of 9 people found the following review helpful.
An excellent textbook
By Georges Melki
For those readers looking for a serious textbook on cosmological inflation, this is it!But of course, they should beware that it is fully technical, and has nothing to do with Andrew Liddle's small book, "An Introduction to Modern Cosmology". This is the real stuff, written by two experts who were instrumental in the development of the "slow-roll inflation" paradigm, and summing up all the latest developments in modern cosmology.
Starting with a small introduction about the hot Big Bang, the authors go on to an in-depth treatment of inflation and its consequences. The simplest model is then exposed and developed into its extensions, such as the Lambda-CDM model, the currently accepted model of inflationary cosmology.
Needless to say, the book offers also a fairly detailed treatment of the CMB and its anisotropies, acoustic oscillations and perturbation theory, and the CMB power spectrum, which are the latest tools in cosmological research.
However, those who are looking for a complete treatment of CMB anisotropies will not find it here.They could turn, for instance, to many articles on arxiv, e.g.the one by Ruth Durrer (astro-ph/0109522)which develops this subject in more detail.
All in all, this book by Liddle and Lyth will probably serve as a textbook on cosmology for the coming ten years.
0 of 0 people found the following review helpful.
It is a good book for large scale structures and perturbations theory in
By Asanka Amarasinghe
I use this as a supplement for Dodelson. It is a good book for large scale structures and perturbations theory in cosmology
0 of 0 people found the following review helpful.
GREAT INFORMATION
By Robert Eaton
Fantastic information detailing the very beginning!! Love it, a must have!!!
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