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OverviewFull Product DetailsAuthor: Scott Dodelson (Department of Astronomy and Astrophysics, University of Chicago, NASA Fermilab Astrophysics Center, Illinois, USA) , Fabian Schmidt (Max-Planck-Institute for Astrophysics, Garching, Germany)Publisher: Elsevier Science Publishing Co Inc Imprint: Academic Press Inc Edition: 2nd edition Weight: 0.840kg ISBN: 9780128159484ISBN 10: 0128159480 Pages: 512 Publication Date: 07 July 2020 Audience: College/higher education , Tertiary & Higher Education Replaced By: 9780443288289 Format: Paperback Publisher's Status: Active Availability: Available To Order ![]() We have confirmation that this item is in stock with the supplier. It will be ordered in for you and dispatched immediately. Table of Contents1. The Concordance Model of Cosmology 2. The Expanding Universe 3. The Fundamental Equations of Cosmology 4. The Origin of Species 5. The Inhomogeneous Universe: Matter & Radiation 6. The Inhomogeneous Universe: Gravity 7. Initial Conditions 8. Growth of Structure: Linear Theory 9. The Cosmic Microwave Background 10. The Polarized CMB 11. Probes of Structure: Tracers 12. Growth of Structure: Beyond Linear Theory 13. Probes of Structure: Lensing 14. Analysis and InferenceReviewsAuthor InformationScott Dodelson is Head of the Department of Physics at Carnegie Mellon University. He received his Ph.D. from Columbia University and was a research fellow at Harvard before moving to Fermilab, the University of Chicago, and Carnegie Mellon. He is the author of more than 200 papers on cosmology, most of which focus on the cosmic microwave background and the large-scale structure of the universe. Dodelson serves as the co-Chair of the Science Committee of the Dark Energy Survey. Fabian Schmidt is a research group leader at the Max-Planck-Institut für Astrophysik (MPA) in Garching, Germany. He obtained his Ph.D. in Astronomy & Astrophysics at the University of Chicago in 2009, and moved to MPA after fellowships at Caltech and Princeton. His work in cosmology (approximately 100 papers so far) focuses on theory, numerics, and analysis of quasilinear and nonlinear large-scale structure, and how we can learn from it about gravity, dark energy, and the physics of inflation. Tab Content 6Author Website:Countries AvailableAll regions |