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Non minimally coupled condensate cosmologies: matching observational data with phase space
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We compare theoretical predictions with observations for a class of cosmological models in which the dark energy component is modeled as a fermionic condensate, non-minimally coupled with the gravitational field and characterized by some specific self-interaction potentials. Our analysis is based on the Markov Chain Monte Carlo Method (MCMC) and employs different data sets. It turns out that with an appropriate choice of parameters our models are fully compatible with several observed data. We combine these parameter values with phase space analysis to deduce the features of the entire cosmic history of the considered models.
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Cited by 2 Pith papers
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Non-minimally coupled nonlinear spinor field in FRW cosmology
In FRW cosmology, non-minimal spinor-gravity coupling strongly accelerates expansion for matter-like spinor fields, but has little effect for dark-energy-like nonlinearities.
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