Interactions in the dark sector within the scope of Bianchi type-V model

DOI10.1142/S0217732320502260zbMath1443.83070MaRDI QIDQ4971762

Tatiana N. Pankratyeva, Ruslan K. Muharlyamov

Publication date: 12 October 2020

Published in: Modern Physics Letters A (Search for Journal in Brave)

zbMATH Keywords

dark energyBianchi type-Vcoincidence problemanisotropic dark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05) Dark matter and dark energy (83C56)

Related Items (1)

Final fate of Kantowski–Sachs gravitational collapse

Cites Work

• LRS Bianchi-I anisotropic cosmological model with dominance of dark energy
• Dynamics of Bianchi \(I\) universe with magnetized anisotropic dark energy
• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• Cosmological model with interactions in the dark sector
• Exact spatially homogeneous cosmologies
• Bianchi type-V dark energy model with varying EoS parameter
• Dark energy models with variable equation of state parameter
• Bianchi type III anisotropic dark energy models with constant deceleration parameter
• Model for a universe described by a non-minimally coupled scalar field and interacting dark matter
• The Bianchi models: then and now
• Cosmological models with a hybrid scale factor in an extended gravity theory
• The late cosmic acceleration and the coincidence problem in Bianchi type I Universe
• Accelerating dark energy cosmological model in two fluids with hybrid scale factor
• The cosmological constant problem

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