Constraining H0 in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes
In accelerating dark energy models, the estimates of the Hubble constant, H0, from Sunyaev-Zel’dovich effect (SZE) and X-ray surface brightness of galaxy clusters may depend on the matter content (ΩM ), the curvature (ΩK) and the equation of state parameter (ω). In this article, by using a sample of...
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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/123456789/30943 |
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