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- W3080261121 abstract "In this paper we consider that dark energy could be described solely by a complex scalar field with a Bose-Einstein condensate-like potential (denoted as CSFDE), that is, with a self-interaction and a mass term. In particular, we analyse a solution which in a fast oscillation regime at late-times behaves as a Cosmological Constant. Our proposal adequately describes the standard homogeneous and flat Fridman dynamics, furthermore, in this quintessence--complex scalar field scenario it is possible to mimic the dynamics related to dark energy. However, when the precision cosmological tests are implemented in this landscape, the generic Equation-of-State derived for this model in a restricted regime of a_i (which corresponds to the scale factor at which the scalar field turns on), cannot be constrained by late-time current observations, since the analysis constraints solely the scalar field parameters within values ruled out by the theoretical model. This result is a clear hint to consider future CSFDE models with, for instance, two scalar fields in order to study the early-time dynamics of the Universe." @default.
- W3080261121 created "2020-09-01" @default.
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- W3080261121 date "2021-03-08" @default.
- W3080261121 modified "2023-10-03" @default.
- W3080261121 title "Observational constraints on complex quintessence with attractive self-interaction" @default.
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- W3080261121 doi "https://doi.org/10.1093/mnras/stab650" @default.
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