Barrow holographic dark energy in deformed Hořava-Lifshitz gravity

DOI10.1142/S0219887822501122WikidataQ114072318 ScholiaQ114072318MaRDI QIDQ6496018

Abdul Jawad, Nadeem Azhar, Shamaila Rani, Sameen Ashraf

Publication date: 2 May 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

thermodynamicscosmological parametersbarrow holographic dark energydeformed Hořava-Lifshitz gravity

Mathematics Subject Classification ID

Differential geometry (53-XX) Relativity and gravitational theory (83-XX)

Cites Work

• A dark energy model characterized by the age of the Universe
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• \(f(R)\) theories
• Instability of holographic dark energy models
• The area of a rough black hole
• Implications of the generalized entropy formalisms on the Newtonian gravity and dynamics
• Mach's Principle and a Relativistic Theory of Gravitation
• Effective Field Theory, Black Holes, and the Cosmological Constant
• The world as a hologram
• Rényi holographic dark energy in the Brans–Dicke cosmology

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