This new graduate textbook adopts a pedagogical approach to contemporary cosmology that enables readers to build an intuitive understanding of theory and data, and of how they interact, which is where the greatest advances in the field are currently being made. Using analogies, intuitive explanations of complex topics, worked examples and computational problems, the book begins with the physics of the early universe, and goes on to cover key concepts such as inflation, dark matter and dark energy, large-scale structure, and cosmic microwave background. Computational and data analysis techniques, and statistics, are integrated throughout the text, particularly in the chapters on late-universe cosmology, while another chapter is entirely devoted to the basics of statistical methods. A solutions manual for end-of-chapter problems is available to instructors, and suggested syllabi, based on different course lengths and emphasis, can be found in the Preface. Online computer code and datasets enhance the student learning experience.
Rezensionen / Stimmen
'An incredibly practical approach to introducing pivotal concepts in cosmology, with a preciously rare focus on preparing its readers to engage with the science of cosmology in a real-life manner.' Vera Gluscevic, University of Southern California 'This superb first introduction to cosmology for advanced undergraduate or graduate students is sure to inspire and teach young inquisitive minds for years to come. Huterer weaves the history of the field with elegant and lucid explanations of the most salient topics in modern cosmology.' Balsa Terzic, Old Dominion University 'This is a welcome addition to the growing number of textbooks on cosmology. The subject is concisely but exceptionally clearly presented, suitable for a one-semester course. The book stands out by covering the full range of material needed for a beginning graduate student contemplating entering research in cosmology: from the foundations all the way to active research topics, such as neutrinos, dark energy, modern large-scale structure and cosmic microwave background experiments, as well as analysis techniques. I am looking forward to adopting this book for my own cosmology course.' Zoltan Haiman, Columbia University 'A clearly written introduction to astrophysical cosmology emphasizing data/theory connections. This text is unique in introducing the relevant techniques for those new to the field.' Curtis Struck, Iowa State University 'A complete guide to form the next generation of well-rounded cosmologists. This book is a unique combination of theoretical, observational, and statistical aspects, with pedagogical and extensive descriptions of modern statistical methods in cosmology.' Alessandra Silvestri, Leiden University
Sprache
Verlagsort
Zielgruppe
Für höhere Schule und Studium
Illustrationen
Worked examples or Exercises
Maße
Höhe: 260 mm
Breite: 208 mm
Dicke: 29 mm
Gewicht
ISBN-13
978-1-316-51359-0 (9781316513590)
Copyright in bibliographic data and cover images is held by Nielsen Book Services Limited or by the publishers or by their respective licensors: all rights reserved.
Schweitzer Klassifikation
Dragan Huterer is a professor of physics at the University of Michigan, where he studies cosmology at the interface of theory and data. He is a leading expert in developing data-driven techniques to understand the nature and origin of 'dark energy,' a component that dominates the dynamics of the universe and causes its accelerated expansion. A fellow of the American Physical Society, he is also a recipient of the University of Michigan's Henry Russel Award and the Humboldt Foundation's Friedrich Wilhelm Bessel Award.
Autor*in
University of Michigan, Ann Arbor
Preface; Acknowledgments; Part I. Foundations: 1. Introduction to cosmology; 2. The Hubble law and geometry of space; 3. Contents of the universe; Part II. The Early Universe: 4. Early-universe thermodynamics; 5. Neutrinos in cosmology; 6. The Boltzmann equation and baryogenesis; 7. Big Bang nucleosynthesis; 8. Inflation; Part III. The Later Universe: 9. Large-scale structure in the universe; 10. Statistical methods in cosmology and astrophysics; 11. Dark matter; 12. Dark energy; 13. Cosmic microwave background; 14. Gravitation lensing; Appendices; References; Index.
