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- W2047322411 abstract "Continuing with previous works, we present a cosmological model in which dark matter and dark energy are modeled by scalar fields $Phi $ and $Psi$, respectively, endowed with the scalar potentials $V(Phi)=V_{o}[ cosh {(lambda sqrt{kappa_{o}}Phi)}-1] $ and $tilde{V}(Psi)=tilde{V_{o}}[ sinh {(alpha sqrt{kappa_{o}}Psi)}] ^{beta}$. This model contains 95% of scalar field. We obtain that the scalar dark matter mass is $m_{Phi}sim 10^{-26}eV.$ The solution obtained allows us to recover the success of the standard CDM. The implications on the formation of structure are reviewed. We obtain that the minimal cutoff radio for this model is $r_{c}sim 1.2 kpc.$" @default.
- W2047322411 created "2016-06-24" @default.
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- W2047322411 date "2000-06-16" @default.
- W2047322411 modified "2023-10-18" @default.
- W2047322411 title "Quintessence and scalar dark matter in the Universe" @default.
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- W2047322411 doi "https://doi.org/10.1088/0264-9381/17/13/101" @default.
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