Modern Cosmology, 3rd Edition by Scott Dodelson - ISBN: 9780443288289
Paperback
Explore the universe’s origins, evolution, and mysteries in this comprehensive cosmology guide.

Modern Cosmology, 3rd Edition

$204.28

  • Paperback

    520 pages

  • Release Date

    27 March 2025

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Summary

Modern Cosmology, Third Edition provides a detailed introduction to the field of cosmology. Beginning with the smooth, homogeneous universe described by a Friedmann-Lemaître-Robertson-Walker metric, this trusted resource includes careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. The reader is then introduced to perturbations about an FLRW universe: their evolution with the Einstein-Boltzmann equations, their primordial generation by inflation, and th…

Book Details

ISBN-13:9780443288289
ISBN-10:0443288283
Author:Scott Dodelson, Fabian Schmidt
Publisher:Elsevier Science Publishing Co Inc
Imprint:Academic Press Inc
Format:Paperback
Number of Pages:520
Edition:3rd
Release Date:27 March 2025
Weight:850g
Dimensions:191mm x 235mm
A-Format
B-Format
C-Format
Modern Cosmology, 3rd Edition by Scott Dodelson - ISBN: 9780443288289
191 × 235 mm
A4
mm / in
About The Author

Scott Dodelson

Scott 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.

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