Bulk Viscous Bianchi Type-III Cosmological Model with Modified Takabayasi String in the Presence of Varying Λ

DOI10.1080/1726037X.2021.1978195zbMath1503.83021OpenAlexW3202868772MaRDI QIDQ5029646

G. S. Khadekar, Shoma Sen, Shilpa Samdurkar

Publication date: 14 February 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.2021.1978195

zbMATH Keywords

bulk viscosityBianchi type III spacetimecosmological term \(\Lambda \)Takabayasi's ring

Mathematics Subject Classification ID

Navier-Stokes equations for incompressible viscous fluids (76D05) Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Geometrodynamics and the holographic principle (83E05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• Unnamed Item
• Cosmological model with viscosity media (dark fluid) described by an effective equation of state
• Modified equation of state, scalar field, and bulk viscosity in Friedmann universe
• Interacting dark energy with inhomogeneous equation of state
• Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
• Quantum de Sitter cosmology and phantom matter
• Some Bianchi type III string cosmological models with bulk viscosity
• Dark energy and viscous cosmology
• DYNAMICS OF DARK ENERGY
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Topology of cosmic domains and strings
• FRW viscous fluid cosmological model with time-dependent inhomogeneous equation of state

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