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Modern Cosmology, by Scott Dodelson
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Modern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe: their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave background (CMB) featuring acoustic peaks and polarization, the matter power spectrum with baryonic wiggles, and their detection via photometric galaxy surveys, redshift distortions, cluster abundances, and weak lensing. The book concludes with a long chapter on data analysis.
Modern Cosmology is the first book to explain in detail the structure of the acoustic peaks in the CMB, the E/B decomposition in polarization which may allow for detection of primordial gravity waves, and the modern analysis techniques used on increasingly large cosmological data sets. Readers will gain the tools needed to work in cosmology and learn how modern observations are rapidly revolutionizing our picture of the universe.
* Provides foundations, calculations, and interpretations which illuminate current thinking in cosmology
* Covers the major advances in cosmology over the past decade
* Includes over 100 unique, pedagogical figures
- Sales Rank: #464517 in Books
- Published on: 2003-03-27
- Original language: English
- Number of items: 1
- Dimensions: 10.00" h x 1.00" w x 7.01" l, 1.81 pounds
- Binding: Hardcover
- 440 pages
Review
"...I like the choice of topics and detailed derivations of some of the basic processes which cannot be found in any other textbook and which really make this book a textbook out of which one can actually learn something. Examples include detailed derivation of inflationary spectrum, Boltzmann equation etc. ... I also like the extensive list of problems at the end of each chapter. This is a great textbook that is long overdue given the importance of the subject..."
- Uros Seljak, Princeton University
"This book is very up to date and gives excellent treatments of structure formation...This provides what is the most complete such description in an textbook."
― Paul H. Frampton, Universtiy of North Carolina at Chapel Hill, CERN COURIER (Oct 2003)
"(In) Dodelson's Modern Cosmology we have recently obtained an appropriate textbook for the dawn of this new epoch...In a sense, this book is postmodern cosmology (with an affirmative connotation!), in being the first to consider the new wave of challenges for this oldest scientific philosophical pursuit...it provides an excellent introduction to some of the most dynamical areas in physics and astronomy, very likely to remain attractive for at least a couple of decades."
― Milan M. Cirkovic, Astronomical Obervatory of Belgrade, FOUNDATIONS OF PHYSICS (Oct 2003)
"Dodelson writes well and the mathematical derivations are generally well laid out and easy to follow. Useful sets of exercises appear at the end of each chapter, along with suggestions for further reading, often with amusing commentaries. New graduate students, Dodelson's intended audience should find it easy to learn from this book."
-George Efstathiou, University of Cambride, England (July 2004)
From the Back Cover
Modern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe:
their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their
observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave
background (CMB) featuring acoustic peaks and polarization, the matter power spectrum with baryonic wiggles, and their detection via photometric galaxy surveys, redshift distortions, cluster abundances, and weak lensing. The book
concludes with a long chapter on data analysis. Modern Cosmology is the first book to explain in detail the structure of the acoustic peaks in the CMB; the E/B decomposition in polarization which may allow for detection of primordial gravity waves; and the modern analysis techniques used on increasingly large cosmological data sets.
Readers will gain the tools needed to work in cosmology and will learn how modern observations are rapidly revolutionizing our picture of the universe.
About the Author
Scott Dodelson is Head of the Theoretical Astrophysics Group
at Fermilab and Associate Professor in the Department of
Astronomy and Astrophysics at the University of Chicago.
He received in Ph.D. at Columbia University and was a research
fellow at Harvard before coming to Fermilab and Chicago.
He is the author of more than seventy papers on cosmology,
most of which focused on the cosmic microwave background and
the large scale structure of the universe.
Most helpful customer reviews
28 of 29 people found the following review helpful.
The best book on graduate cosmology.
By Andrew J. S. Hamilton
I am currently teaching graduate cosmology. Modern cosmology is an extraordinarily beautiful piece of physics that has allowed cosmologists to learn from observations fundamental facts about our universe. Graduate students want to understand this beautiful subject themselves. Dodelson's book is the one that delivers that understanding. Of the several graduate cosmology texts out there, this one is unquestionably the best.
The book is uncompromisingly a graduate level text. The material is intrinsically hard, but Dodelson does a remarkable job of taking the reader through it. The problem sets at the end of each chapter (some with solutions) are well thought out, and fill in many gaps. Each chapter concludes with a thoughtful summary and a guide to further reading. If you are going to teach a graduate level cosmology class with this book, then you should impress on your students that the text is not easy, but it's the real unwatered-down thing.
13 of 14 people found the following review helpful.
Approachable Cosmology
By f. j. busch
This book is a must-have for the cosmos-curious. Well organized and indexed and excellently written, the author puts difficult information within reach of the student who aspires to understand one of the most complex disciplines. A superb accomplishment by a fine teacher and consummate scientist that should become the definitive text for all would-be cosmologists.
68 of 69 people found the following review helpful.
Impressive even at a first look
By A Customer
I stumbled across the title of this book when I was browsing around somebody's cosmology course website. I know that Scott Dodelson is a quite well-known cosmologist, so I start searching for more information. After reading the preliminary detailed table of contents (I found it somewhere on the web) and the book description from Academic Press, I decided to pre-order the book. The book arrived just on March 31. I tried to take a quick but thorough view before write this comment. I haven't read the book in full. Here i would just like to write the Table of Contents in more detail by including the sections.
1. The Standard Model and Beyond. The expanding universe, Hubble diagram, Big Bang Nucleosynthesis (BBN), Cosmic Microwave Background (CMB), beyond Standard Model.
2. The Smooth, Expanding Universe. General relativity (crash course), distances, evolution of energy, cosmic inventory (photons, baryons, matter, neutrinos, dark energy, epoch of matter-radiation equality).
3. Beyond Equilibrium. Boltzmann equation for annihilation, BBN (neutron & light elements abudance), recombination, dark matter.
4. The Boltzmann Equations (BE). BE for harmonic oscillator, the collisionless BE for photons (0th and 1st order), collision terms: Compton scattering, BE for photons, BE for Cold Dark Matter (CDM), BE for baryons.
5. Einstein Equations. Perturbed Ricci tensor and scalar, two components of Einstein Equations, tensor perturbations, decomposition theorems, gauges.
6. Initial conditions. Einstein-Boltzmann equations at early times, the horizon, inflation, gravity wave production, scalar perturbations.
7. Inhomogeneities. Prelude, large scales (super-horizon & through horizon crossing), small scales (horizon & sub-horizon crossing), growth function, beyond CDM.
8. Anisotropies. Overview, large-scale anisotropies, acoustic oscillations (tightly coupled), diffusion (Silk) damping, inhomogeneities to anisotropies (free streaming, C_{l}s), anisotropy spectrum (Sachs-Wolfe, small scales), cosmological parameters.
9. Probe of Inhomogeneities. Angular correlation, peculiar velocities, redshift space distortions, galaxy clusters.
10. Weak Lensing and Polarization. Gravitational distortion, geodesics and shears, ellipticity, weak lensing power spectrum, polarization, quadrupole and Q/U (or E/B as in recent literatures) decomposition, polarization power spectra, detection of gravity waves.
11. Analysis. Likelihood function, signal covariance matrix, Karhunen-Loeve & optimal quadratic, Fisher matrix, mapmaking & inversion, systematics, foregrounds.
Appendix A. Solution to Selected Problems
Appendix B. Numbers
Appendix C. Special Functions
Appendix D. Symbols.
Bibliography.
In addition, each chapter is ended with a summary and further reading list. Quite nice indeed. The bibliography are extensive: there are classic, pioneering papers, recent papers, textbooks. There are some color plates in the middle part of the book.
In my opinion, this book is far better than Peacock in discussing new aspect of anisotropies and inhomogeneities. Lots of topics that were only previously available in research papers, review articles, summer school lectures, preprints, are brought together to the form of a decent book. The chapter of analysis is quite interesting, since the subject has become very demanding but there are still no single treatment of it.
Dodelson said in the preface that the expected audience are advanced undergraduate and beginning graduate students. Some of the necessary materials (GR, inflation, are introduced in the text).
I myself suggests, however, that the reader should have a proficient knowledge in standard undergraduate physics (mechanics, thermodynamics, electromagnetism, quantum physics), mathematical physics, and general relativity if possible. Some knowledge of astrophysics/astronomy, statistics/data analysis, kinetic theory, would certainly be welcomed.
A little bit of cons, however are inevitable. The current development in cosmology is astounding. Just a few weeks before the book was published, the WMAP team released their first result after a year of observations, which put tight constraints for cosmological models. Several numbers and figures in the book then are in the need to be updated. Topics such as distant quasars, cosmic reionization and the end of cosmic dark ages, first-generation stars, might be worthy enough to be included in the future.
This book is definitely a must buy for cosmologist.
Update 2003 July 8
Author's website for the book is available with full table of contents at
home.fnal.gov/~dodelson/book.html
Update 2003 September 8.
You should also get two more books beside this.
1) Kinetic theory in the expanding universe by Jeremy Bernstein, Cambridge, 1988, ISBN 0-521-36050-1. Best reference material to understand relativistic Boltzmann equation in Dodelson chapter 3-5.
2) The Early Universe by Edward W. Kolb and Michael S. Turner, Perseus/Westview, 1994, ISBN 0-201-62674-8. Contains extensive material on FRW metric, detailed discussion on nucleosynthesis and particle physics-cosmology interface, inflation, and structure formation.
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