Anisotropic cosmological models with two fluids

DOI10.1155/2018/6306848zbMath1396.83068arXiv1706.07661OpenAlexW3098558271MaRDI QIDQ1791267

S. K. J. Pacif, B. Mishra, Pratik P. Ray

Publication date: 4 October 2018

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

Full work available at URL: https://arxiv.org/abs/1706.07661

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (6)

Bianchi type-\(I\) bulk viscosity with a DE cosmological model ⋮ Modeling of Accelerating Universe with Bulk Viscous Fluid in Bianchi V Space‐Time ⋮ Probing kinematics and fate of Bianchi type V Universe ⋮ Axially magnetized dark energy cosmological model ⋮ Gravitational baryogenesis of cosmological constant dominated universe ⋮ Axially Symmetric Bulk Viscous Cosmological Model in F(R, T) Theory of Gravity

Cites Work

• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• Bianchi type III models with anisotropic dark energy
• Dark energy models with variable equation of state parameter
• Anisotropic dark energy model with a hybrid scale factor
• THERMODYNAMICAL DESCRIPTION OF THE INTERACTING NEW AGEGRAPHIC DARK ENERGY
• Dark Energy
• SOME BIANCHI TYPE-V MODELS OF ACCELERATING UNIVERSE WITH DARK ENERGY
• DYNAMICS OF DARK ENERGY
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Accelerating dark energy cosmological model in two fluids with hybrid scale factor
• General Relativity

This page was built for publication: Anisotropic cosmological models with two fluids