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Abstract
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In the Brans–Dicke cosmology framework, we study holographic dark energy models with interaction and
with power-law and logarithmic entropy corrections for different cutoffs. We consider conditions on the
Brans–Dicke parameter compared with the conditions for the acceleration and phantom phases to show
which entropy-corrected models can have acceleration and a phantom phase in the early Universe and at
the present. Moreover, we determine which of the considered models are classically stable and which are
unstable in early times and at the present.
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