Can a Chameleon Field Be Identified with Quintessence?
In the Einstein–Cartan gravitational theory with the chameleon field, while changing its mass independently of the density of its environment, we analyze the Friedmann–Einstein equations for the Universe’s evolution with the expansion parameter <i>a</i> being dependent on time only. We analyze the p...
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| Autors principals: | , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
MDPI AG
2020-11-01
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| Col·lecció: | Universe |
| Matèries: | |
| Accés en línia: | https://www.mdpi.com/2218-1997/6/12/221 |
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