Cosmological Implications of the Generalized Entropy Based Holographic Dark Energy Models in Dynamical Chern-Simons Modified Gravity

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colspan="4"><hr/></td></tr><tr><td class="align_left">RHDE</td><td class="align_center">quintessence-to-vacuum</td><td class="align_center">stability</td><td class="align_center">thawing region</td></tr><tr><td class="align_left" colspan="4"><hr/></td></tr><tr><td class="align_left">SMHDE</td><td class="align_center">quintessence</td><td class="align_center">un-stable</td><td class="align_center">thawing region</td></tr><tr class="table-tr"><td colspan="4"><hr class="tbody-hr"/></td></tr></table></td></tr></table>

<div>Summary of the cosmological parameters and plane.</div>

Advances in High Energy Physics

tab1

Table 1

Table 1: Cosmological Implications of the Generalized Entropy Based Holographic Dark Energy Models in Dynamical Chern-Simons Modified Gravity 