Effects of shear and rotation on the spherical collapse model for clustering dark energy
In the framework of the spherical collapse model, we study the influence of shear and rotation terms for dark matter fluid in clustering dark energy models. We evaluate, for different equations of state, the effects of these terms on the linear overdensity threshold parameter, δc, and on the virial...
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| Principais autores: | , , |
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| Formato: | article |
| Idioma: | English |
| Publicado em: |
Oxford University Press
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| Assuntos: | |
| Endereço do item: | https://repositorio.ufrn.br/handle/123456789/30830 |
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