Clustering dark energy and halo abundances
Within the standard paradigm, dark energy is taken as a homogeneous fluid that drives the accelerated expansion of the universe and does not contribute to the mass of collapsed objects such as galaxies and galaxy clusters. The abundance of galaxy clusters—measured through a variety of channels—has b...
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| Principais autores: | , |
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| Formato: | article |
| Idioma: | English |
| Publicado em: |
IOP Publishing
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| Endereço do item: | https://repositorio.ufrn.br/handle/123456789/30828 |
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