Cosmological Perturbations in Phantom Dark Energy Models
The ΛCDM paradigm, characterised by a constant equation of state w = − 1 for dark energy, is the model that better fits observations. However, the same observations strongly support the possibility of a dark energy content where the corresponding equation of state is close to but slightly sm...
Сохранить в:
| Главные авторы: | , , |
|---|---|
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
MDPI AG
2017-03-01
|
| Серии: | Universe |
| Предметы: | |
| Online-ссылка: | http://www.mdpi.com/2218-1997/3/1/22 |
| Метки: |
Нет меток, Требуется 1-ая метка записи!
|