IMIST


Dark energy (notice n° 4936)

000 -LEADER
fixed length control field 02308cam a2200253' 4500
001 - CONTROL NUMBER
control field UNI0000631
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20161122162558.0
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 140919s2010 us a b 001 eng
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 9780521516006 (hardback)
040 ## - CATALOGING SOURCE
Modifying agency IMIST
Description conventions rda
040 ## - CATALOGING SOURCE
Original cataloging agency DLC
Description conventions rda
041 1# - LANGUAGE CODE
Language code of text/sound track or separate title eng
050 #4 - LIBRARY OF CONGRESS CALL NUMBER
Classification number QB791.3
082 04 - DEWEY DECIMAL CLASSIFICATION NUMBER
Classification number 523.1/8
Edition number 22
100 1# - MAIN ENTRY--PERSONAL NAME
Personal name Amendola, Luca,
Titles and other words associated with a name 1963-
245 10 - TITLE STATEMENT
Title Dark energy
Remainder of title theory and observations
Statement of responsibility, etc Luca Amendola, Shinji Tsujikawa.
260 ## - PUBLICATION, DISTRIBUTION, ETC. (IMPRINT)
Place of publication, distribution, etc New York
Name of publisher, distributor, etc Cambridge University Press
Date of publication, distribution, etc 2010.
300 ## - PHYSICAL DESCRIPTION
Extent xiv, 491 pages
Other physical details illustrations
Dimensions 25 cm.
500 ## - GENERAL NOTE
General note "Dark energy, the mysterious cause of the accelerating expansion of the Universe, is one of the most important fields of research in astrophysics and cosmology today. Introducing the theoretical ideas, observational methods and results, this textbook is ideally suited to graduate courses on dark energy, and will also supplement advanced cosmology courses. Providing a thorough introduction to this exciting field, the textbook covers the cosmological constant, quintessence, k-essence, perfect fluid models, extradimensional models, and modified gravity. Observational research is reviewed, from the cosmic microwave background to baryon acoustic oscillations, weak lensing, and cluster abundances. Every chapter ends with problems, with full solutions provided, and any calculations are worked through step-by-step. "--
504 ## - BIBLIOGRAPHY, ETC. NOTE
Bibliography, etc Includes bibliographical references (p. 457-484) and index.
505 ## - FORMATTED CONTENTS NOTE
Formatted contents note Machine generated contents note: 1. Overview; 2. Expansion history of the universe; 3. Correlation function and power spectrum; 4. Basics of cosmological perturbation theory; 5. Observational evidence of dark energy; 6. Cosmological constant; 7. Dark energy as a modified form of matter I: quintessence; 8. Dark energy as a modified form of matter II; 9. Dark energy as a modification of gravity; 10. Cosmic acceleration without dark energy; 11. Dark energy and linear cosmological perturbations; 12. Non-linear cosmological perturbations; 13. Statistical methods in cosmology; 14. Future observational constraints on the nature of dark energy; 15. Conclusion and outlook; 16. Answers to the problems; 17. Mathematical appendix; Index.
650 #0 - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name as entry element Dark energy (Astronomy)
700 1# - ADDED ENTRY--PERSONAL NAME
Personal name Tsujikawa, Shinji.
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        La bibliothèque des Sciences Exactes et Naturelles La bibliothèque des Sciences Exactes et Naturelles   22655   523.18 AME 0000000022493 11/22/2016 11/22/2016 Livre
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