Non-Canonical Dark Energy Parameter Evolution in a Canonical Quintessence Cosmology
This study considers the specific case of a flat, minimally coupled to gravity, quintessence cosmology with a dark energy quartic polynomial potential that has the same mathematical form as the Higgs potential. Previous work on this case determined that the scalar field is given by a simple expressi...
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| Format: | Artigo |
| Jezik: | Inglês |
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MDPI AG
2024-09-01
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| Serija: | Universe |
| Teme: | |
| Online dostop: | https://www.mdpi.com/2218-1997/10/9/356 |
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