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- W3099308051 endingPage "2050057" @default.
- W3099308051 startingPage "2050057" @default.
- W3099308051 abstract "We derive two field theory models of interacting dark energy, one in which dark energy is associated with the quintessence and another in which it is associated with the tachyon. In both, instead of choosing arbitrarily the potential of scalar fields, these are specified implicitly by imposing that the dark energy fields must behave as the new agegraphic dark energy. The resulting models are compared with the Pantheon supernovae sample, CMB distance information from Planck 2015 data, baryonic acoustic oscillations (BAO) and Hubble parameter data. For comparison, the noninteracting case and the [Formula: see text] model also are considered. By use of the AIC and BIC criteria, we have obtained strong evidence in favor of the two interacting models, and the coupling constants are nonvanishing at more than [Formula: see text] confidence level." @default.
- W3099308051 created "2020-11-23" @default.
- W3099308051 creator A5053432898 @default.
- W3099308051 date "2020-06-01" @default.
- W3099308051 modified "2023-09-27" @default.
- W3099308051 title "Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection" @default.
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- W3099308051 doi "https://doi.org/10.1142/s0218271820500571" @default.
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