LRS Bianchi Type-II modified holographic Ricci dark energy models in a scalar-tensor theory of gravitation

DOI10.1080/1726037X.2017.1327163zbMath1499.83017OpenAlexW2626084665MaRDI QIDQ5069617

G. Ananda Rao, D. R. K. Reddy, T. Kanakavalli

Publication date: 19 April 2022

Published in: Journal of Dynamical Systems and Geometric Theories (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/1726037x.2017.1327163

zbMATH Keywords

scalar-tensor theorymodified holographic dark energyBianchi type-II universeRicci dark energyhybrid expansion law

Mathematics Subject Classification ID

General relativity (83C99) Space-time singularities, cosmic censorship, etc. (83C75) Dark matter and dark energy (83C56)

Cites Work

• Some simple predictions from \(E_{11}\) symmetry
• Anisotropic generalized ghost pilgrim dark energy model in general relativity
• Bulk-brane interaction and holographic dark energy
• The holographic dark energy in non-flat Brans-Dicke cosmology
• Exact spatially homogeneous cosmologies
• Holography Stabilizes the Vacuum Energy
• The cosmological constant and dark energy
• Mach's Principle and a Relativistic Theory of Gravitation
• RECONSTRUCTING DARK ENERGY
• THE COSMOLOGICAL DYNAMICS OF INTERACTING HOLOGRAPHIC DARK ENERGY MODEL
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Probable Values of the Cosmological Constant in a Holographic Theory

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