Titre : |
Dark energy |
Type de document : |
texte imprimé |
Auteurs : |
Wang, Yun, Auteur |
Editeur : |
New York : John Wiley & Sons |
Année de publication : |
2010 |
Importance : |
244 p. |
Présentation : |
ill. |
Format : |
25 cm |
ISBN/ISSN/EAN : |
978-3-527-40941-9 |
Note générale : |
Notes bibliogr. - Index. |
Langues : |
Anglais (eng) |
Mots-clés : |
Énergie sombre (astronomie) |
Index. décimale : |
52 Astronomie.Astrophysique.Recherche Spatial.Géodésie |
Résumé : |
A systematic, carefully authored review of our current observational and theoretical knowledge of dark energy. Providing a brief and concise overview, the book covers theory and experiment in equal detail, directly linking the two. A final section also looks at future developments. Indispensable for researchers entering this rapidly evolving field. |
Note de contenu : |
In summary :
1. The dark energy problem
2. The basic theoretical framework.
3. Models to explain cosmic Acceleration.
4. Observational method I: Type Ia supernovae as dark energy probe
5. Observational method II: Galaxy redshift survey as dark energy probe
6. Observational method III: Weak lensing as dark energy probe
7. Observational method IV: Clusters as dark energy probe
8. Other observational methods for probing dark energy
9. Framework for interpreting data
10. Basic Instrumentation for Dark Energy Experiments
11. Future Prospects for Probing Dark Energy |
Dark energy [texte imprimé] / Wang, Yun, Auteur . - New York : John Wiley & Sons, 2010 . - 244 p. : ill. ; 25 cm. ISBN : 978-3-527-40941-9 Notes bibliogr. - Index. Langues : Anglais ( eng)
Mots-clés : |
Énergie sombre (astronomie) |
Index. décimale : |
52 Astronomie.Astrophysique.Recherche Spatial.Géodésie |
Résumé : |
A systematic, carefully authored review of our current observational and theoretical knowledge of dark energy. Providing a brief and concise overview, the book covers theory and experiment in equal detail, directly linking the two. A final section also looks at future developments. Indispensable for researchers entering this rapidly evolving field. |
Note de contenu : |
In summary :
1. The dark energy problem
2. The basic theoretical framework.
3. Models to explain cosmic Acceleration.
4. Observational method I: Type Ia supernovae as dark energy probe
5. Observational method II: Galaxy redshift survey as dark energy probe
6. Observational method III: Weak lensing as dark energy probe
7. Observational method IV: Clusters as dark energy probe
8. Other observational methods for probing dark energy
9. Framework for interpreting data
10. Basic Instrumentation for Dark Energy Experiments
11. Future Prospects for Probing Dark Energy |
|  |