Analysis of Bianchi type V holographic dark energy models in general relativity and Lyra's geometry

DOI10.1155/2021/8818590zbMath1457.83084OpenAlexW3124473387MaRDI QIDQ2660118

Daba Meshesha Gusu, M. Vijaya Santhi

Publication date: 29 March 2021

Published in: Advances in High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1155/2021/8818590

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Dark matter and dark energy (83C56)

Cites Work

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• Holographic dark energy interacting with two fluids and validity of generalized second law of thermodynamics
• Exact spatially homogeneous cosmologies
• Stability analysis of agegraphic dark energy in Brans-Dicke cosmology
• Tilted Bianchi type-III cosmological models in Lyra geometry
• Holographic dark energy model with quintessence in Bianchi type-I space-time
• ACCELERATING DARK ENERGY MODELS IN BIANCHI TYPE-V SPACETIME
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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