Holographic dark energy models are formally rewritten as k-essence scalar fields, but the central reconstruction equation contains an apparent algebraic error and the 'most generalized' cutoff is not actually implemented.
Thus, in the present consideration L = H − 1
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Holographic reconstruction of k-essence model with Tsallis and the most generalized Nojiri-Odintsov version of holographic dark energy
Holographic dark energy models are formally rewritten as k-essence scalar fields, but the central reconstruction equation contains an apparent algebraic error and the 'most generalized' cutoff is not actually implemented.