Description
Book SynopsisIntroducing the theoretical ideas, observational methods and results, this textbook is a thorough introduction to the exciting field of dark energy. Ideally suited to graduate courses on dark energy, it contains problems with full solutions. Any calculations are worked through step-by-step.
Trade Review'… tightly-packed, of a high standard, making appreciable demands upon the reader, student and researcher … [this book] succeeds in its purpose of bringing the reader closer to an appreciation of the wonders and the complexities that cosmology sets out to elucidate.' Contemporary Physics
'One strength of Amendola and Tsujikawa's book is the level of detail it provides on dark energy models … comprehensive.' Joshua Frieman, Physics Today
Table of Contents1. 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.
