Anisotropic cosmological models with quintessence

DOI10.1007/s10773-013-1829-3zbMath1284.83037OpenAlexW2024086523MaRDI QIDQ2444017

Yanyan Li

Publication date: 8 April 2014

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10773-013-1829-3

zbMATH Keywords

bulk viscosityquintessenceBianchi type I

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)

Related Items (4)

Bianchi type-I universe with cosmological constant and quadratic equation of state in \(f(R, T)\) modified gravity ⋮ Bianchi type-V domain walls and quark matter cosmological model with cosmological constant \(\Lambda\) in \(f\left(R, T\right)\) gravity ⋮ Interacting holographic dark energy in Bianchi type-V and IX universes with variable deceleration parameter ⋮ Scalar field and time varying cosmological constant in \(f(R, T)\) gravity for Bianchi type-I universe

Cites Work

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• Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant
• Bulk viscosity driving the acceleration of the universe
• A quintessence scalar field in Brans-Dicke theory
• The cosmological constant and dark energy
• A Quintessence Problem in Self-Interacting Brans–Dicke Theory
• Dissipative cosmology
• Bianchi Type III String Cosmological Model with Bulk Viscosity
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• BIANCHI TYPE I UNIVERSE WITH VISCOUS FLUID
• Quintessence model with double exponential potential

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