عنوان مجله
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ASTROPHYSICS AND SPACE SCIENCE
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چکیده
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We study the entropy-corrected version of the
new agegraphic dark energy (NADE) model and dark matter
in a spatially non-flat Universe and in the framework
of Hoˇrava-Lifshitz cosmology. For the two cases containing
noninteracting and interacting entropy-corrected NADE
(ECNADE) models, we derive the exact differential equation
that determines the evolution of the ECNADE density
parameter. Also the deceleration parameter is obtained. Furthermore,
using a parametrization of the equation of state
parameter of the ECNADE model as ω(z) = ω0 +ω1z, we
obtain both ω0 and ω1. We find that in the presence of interaction,
the equation of state parameter ω0 of this model can
cross the phantom divide line which is compatible with the
observation.
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