Large-scale galaxy correlations as a test for dark energy
We have shown earlier that, contrary to popular belief, Einstein--de Sitter (E--deS) models can still fit the {\sl WMAP} data on the cosmic microwave background provided one adopts a low Hubble constant and relaxes the usual assumption that the primordial density perturbation is scale-free. The rece...
| المؤلفون الرئيسيون: | , , , |
|---|---|
| التنسيق: | Journal article |
| اللغة: | English |
| منشور في: |
2005
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