Cosmology ,


Oxford U. Press
New York
, 2008. $90.00 (593 pp.). ISBN 978-0-19-852682-7

For many years I knew Steven Weinberg was synthesizing and reformulating cosmology for a major new book that would inhabit a vastly different cosmic landscape from that of his masterful Gravitation and Cosmology (Wiley, 1972). I would receive e-mails from him on the finest details of cosmic microwave background (CMB) theory; eventually respond, sometimes at 2:00 am; and get immediate replies. I am sure my heady experience was far from unique. Weinberg has cast his gaze over the vast terrain that cosmology has become since 1972, and his new work ranges from early-universe field and string theory, through inflation and phase transitions, Big Bang nucleosynthesis, and the decoupling of the microwave background radiation, and forward to the nonlinear era of the dissipative formation of galaxies and their large-scale clustering into an interconnected cosmic web.

For me, a tragic aspect of the wondrous growth of cosmology is its fragmentation into many subfields, each requiring special expertise and methods. It is therefore a pleasure to see Weinberg’s finished product and the role it can play in broadening and deepening the cosmic comprehension of graduate students, postdoctoral fellows, and indeed professors.

For decades, Gravitation and Cosmology and the equally famous Gravitation (Freeman, 1973), the Charles Misner, Kip Thorne, and John Wheeler tome, dominated how gravity was taught. Weinberg’s was the simpler and more direct approach of a particle physicist. When I taught advanced gravity I oscillated between the two. Cosmology arrives amidst texts of varying difficulty, several of which have successfully been used in graduate courses. Two noteworthy examples that cover much the same ground as Weinberg’s new text are the nicely accessible Modern Cosmology (Academic Press, 2003) by Scott Dodelson (reviewed in Physics Today, July 2004, page 60) and Physical Foundations of Cosmology (Cambridge University Press, 2005) by Viatcheslav Mukhanov. How does Cosmology do relative to those two? Very well for serious students of the subject; they should probably own all three books.

Cosmology quickly gets into in-depth arguments, relying on extensive and useful appendices and on Gravitation and Cosmology to bring the uninitiated up to speed. The first chapter includes a fast-paced introduction to basic tests showing the universe is homogeneous and isotropic. It elegantly sets up the Friedmann-Robertson-Walker metrics, providing nice historical notes along the way, and discusses the observational support for an accelerating universe. I found it interesting that the word “anthropic” does not appear in the book, despite Weinberg’s influential anthropic explanation for the problematically small value of the cosmological constant.

The next few chapters focus on the basic homogeneous hot Big Bang model and its thermal history. Then the hard work associated with inhomogeneities begins. Weinberg’s emphasis is on linear perturbation theory, a well-founded subject that has given us the exquisite CMB inferences about cosmic densities and fluctuation spectra. He offers coverage of fluctuation development, an extensive and technical treatment of the CMB, a less extensive treatment of strong and weak gravitational lensing, and a relatively complete theory of inflation. He does not, however, indulge in the more speculative aspects of inflationary theory, in particular the string-inspired models so popular now. I think Weinberg was quite right in that omission, given that his book is destined to stand the test of time. Still, it would be nice to have gotten his take on such leading-edge and fun ideas. Cosmology treats the nonlinear development of the cosmic web with simple models to illustrate the physical aspects, but one comes away without insight into why the interconnected web has the texture it has. The great advances in simulation and the methods used to achieve them are not covered.

Weinberg, who is better known as a particle theorist than as a cosmologist, has made an admirable attempt at historical accuracy and credit; nonetheless he does miss a number of works of relevance. Another curious feature of Cosmology —particularly given its visually stunning subject–is the relative lack of figures: There are no WMAP (Wilkinson Microwave Anisotropy Probe) all-sky CMB maps to be seen. Tables are often Weinberg’s preferred method of information delivery. I find that in this age of computer dominance, young people learn visually much more than did prior generations, for whom the equation is the thing. Yet everyone who plans to be a serious cosmologist must endure the strength exercise of equation working to develop physical intuition. Cosmology is one book with which they can develop their chops. Moreover, Weinberg’s reputation as a powerful and insightful deriver is without peer, so the reader can rest assured all equations are well vetted.

Cosmology is a worthy follow-on to Gravitation and Cosmology and continues the earlier work’s effective, straightforward derivational approach. A technical tour de force for the intrepid graduate student, Weinberg’s new book will greatly appeal to particle physicists tooling up in cosmology and be an indispensable source for the practitioner.