Preface to second edition; Preface to first edition; 1. Introduction; 2. Fundamental observations; 3. Newton versus Einstein; 4. Cosmic dynamics; 5. Model universes; 6. Measuring cosmological parameters; 7. Dark matter; 8. The cosmic microwave background; 9. Nucleosynthesis and the early Universe; 10. Inflation and the very early Universe; 11. Structure formation: gravitational instability; 12. Structure formation: baryons and photons; Epilogue; Bibliography; Table of useful constants; Index.
Barbara Ryden received her PhD in astrophysical sciences from Princeton University, New Jersey in 1987. After postdocs at the Harvard-Smithsonian Center for Astrophysics and the Canadian Institute for Theoretical Astrophysics, she joined the astronomy faculty at the Ohio State University, where she is now a full professor. She has over twenty years of experience in teaching, at levels ranging from introductory undergraduate courses to advanced graduate seminars. She won the Chambliss Astronomical Writing Award for the first edition of Introduction to Cosmology (2002), and is the co-author, with Bradley Peterson, of Foundations of Astrophysics (2010).
'This is an excellent textbook, with a clear and pedagogical presentation, which perfectly fills a gap between other introductory books available at either much more basic or much more advanced levels. The easy-to-read style, focus on physics concepts, and self-contained derivations make the book easy to follow. It works well for advanced undergraduates or beginning graduate students, who will come away with a solid and comprehensive understanding of modern cosmology. The additions in this Second Edition, such as galaxy formation and baryon acoustic oscillations, are valuable and bring the book even more up-to-date.' Zoltan Haiman, Columbia University 'Barbara Ryden writes in a very clear and engaging style. This transparency has inspired many undergraduate science majors in my cosmology class to pursue additional coursework and research in astrophysics. The addition of new material on the baryonic component of the universe links cosmology to many modern research topics in astrophysics.' Crystal Martin, University of California, Santa Barbara 'I am delighted that a second edition of Barbara Ryden's Introduction to Cosmology is now available. With the addition of a second chapter on structure formation, the book paints an elegant mathematical picture of the evolution of the Universe from the Big Bang to the formation of stars. Ryden does a masterful job of paring cosmology down to its most fundamental elements and presenting complex topics with exceptional clarity. The conversational style of the text, the imaginative analogies, and the emphasis placed on developing students' conceptual understanding combine to make this book one of the best upper-level astronomy texts available.' Christy Tremonti, University of Wisconsin, Madison 'Barbara Ryden's Introduction to Cosmology is now published in a second edition, following the well-received first edition of 2002 ... This is a course book for physics students; its approach is quantitative and the basic equations and mathematical descriptions are extensively outlined from first principles in all the areas covered. Those equations that are not derived are quoted in such a way as to be understood ... Without this, of course, cosmology cannot be usefully studied ... The style of writing is efficient, while being pleasant and clear, and the explanations are on the whole of a high quality in their attention to the level of detail that is needed for a genuine understanding of the arguments. This is a highly recommendable textbook that deserves to be widely taken up in university courses in physics and astronomy.' Peter J. Bussey, Contemporary Physics