Dark energy: theory and observations
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 ener...
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| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
2010
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| Subjects: | |
| Online Access: | BSB01 FHN01 Volltext |
| Summary: | 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, extra-dimensional 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 |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (xiv, 491 pages) |
| ISBN: | 9780511750823 |
| DOI: | 10.1017/CBO9780511750823 |
Staff View
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| 505 | 8 | |a 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 | |
| 520 | |a 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, extra-dimensional 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 | ||
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| contents | 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 |
| ctrlnum | (ZDB-20-CBO)CR9780511750823 (OCoLC)967685664 (DE-599)BVBBV043942705 |
| dewey-full | 523.1/8 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1/8 |
| dewey-search | 523.1/8 |
| dewey-sort | 3523.1 18 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
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| indexdate | 2024-07-10T07:39:18Z |
| institution | BVB |
| isbn | 9780511750823 |
| language | English |
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| spelling | Amendola, Luca 1963- Verfasser aut Dark energy theory and observations Luca Amendola, Shinji Tsujikawa Cambridge Cambridge University Press 2010 1 online resource (xiv, 491 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) 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 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, extra-dimensional 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 Dark energy (Astronomy) Dunkle Energie (DE-588)7589166-9 gnd rswk-swf Dunkle Energie (DE-588)7589166-9 s 1\p DE-604 Tsujikawa, Shinji Sonstige oth Erscheint auch als Druckausgabe 978-0-521-51600-6 Erscheint auch als Druckausgabe 978-1-107-45398-2 https://doi.org/10.1017/CBO9780511750823 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Amendola, Luca 1963- Dark energy theory and observations 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 Dark energy (Astronomy) Dunkle Energie (DE-588)7589166-9 gnd |
| subject_GND | (DE-588)7589166-9 |
| title | Dark energy theory and observations |
| title_auth | Dark energy theory and observations |
| title_exact_search | Dark energy theory and observations |
| title_full | Dark energy theory and observations Luca Amendola, Shinji Tsujikawa |
| title_fullStr | Dark energy theory and observations Luca Amendola, Shinji Tsujikawa |
| title_full_unstemmed | Dark energy theory and observations Luca Amendola, Shinji Tsujikawa |
| title_short | Dark energy |
| title_sort | dark energy theory and observations |
| title_sub | theory and observations |
| topic | Dark energy (Astronomy) Dunkle Energie (DE-588)7589166-9 gnd |
| topic_facet | Dark energy (Astronomy) Dunkle Energie |
| url | https://doi.org/10.1017/CBO9780511750823 |
| work_keys_str_mv | AT amendolaluca darkenergytheoryandobservations AT tsujikawashinji darkenergytheoryandobservations |