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...
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| Автори: | , , |
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| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
MDPI AG
2017-03-01
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| Серія: | Universe |
| Предмети: | |
| Онлайн доступ: | http://www.mdpi.com/2218-1997/3/1/22 |
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