Barrow holographic dark energy model with different infrared cutoffs in dynamical Chern–Simons modified gravity


Altaibayeva A. Ualikhanova U. Shegebayeva U. Chattopadhyay S.
31 March 2026World Scientific

International Journal of Geometric Methods in Modern Physics
2026#23Issue 4

Barrow Holographic Dark Energy (BHDE), that modifies the standard holographic dark energy framework by incorporating quantum-gravity-induced deformation through a Barrow entropy measure, demonstrated in [E. N. Saridakis, Barrow holographic dark energy, Phys. Rev. D 102(12) (2020) 123525], is investigated and studied in the framework of the Chern–Simons modified gravity framework. We bring into focus the BHDE with two different IR cutoffs. The BHDE density is reconstructed in the Chern–Simons modified gravity framework and accordingly the equation of state parameter is reconstructed and studied for different ranges of Δ, which is the deformation parameter indicating the amount of the quantum gravitational deformation effects to the horizon structure associated with BHDE. The relevant expressions of the Hubble parameter H and reconstructed BHDE density are also studied. Finally, the four energy conditions are analyzed for the reconstruction models.

Barrow holographic dark energy , Chern–Simons modified gravity , deformation parameter , energy conditions , equation of state parameter

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Department of General and Theoretical Physics, L.N. Gumilyov Eurasian National University, Satpayev St. 2, Astana, 010008, Kazakhstan
Department of Mathematics, Amity University Kolkata, Major Arterial Road, Action Area II, Rajarhat, Newtown, Kolkata, 700135, India

Department of General and Theoretical Physics
Department of Mathematics

10 лет помогаем публиковать статьи Международный издатель

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