The late cosmic acceleration and the coincidence problem in Bianchi type I Universe

DOI10.1142/S0217732319502390zbMath1422.83021OpenAlexW2955954442WikidataQ127675035 ScholiaQ127675035MaRDI QIDQ5234602

Ruslan K. Muharlyamov, Tatiana N. Pankratyeva

Publication date: 27 September 2019

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

Full work available at URL: https://doi.org/10.1142/s0217732319502390

zbMATH Keywords

dark energyBianchi type I modelanisotropic dark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (1)

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

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
• Dark energy models with variable equation of state parameter
• Bianchi type III anisotropic dark energy models with constant deceleration parameter
• The Bianchi models: then and now
• Anisotropic dark energy model with a hybrid scale factor
• Cosmological models with a hybrid scale factor in an extended gravity theory
• New inflation from old
• Accelerating dark energy cosmological model in two fluids with hybrid scale factor
• The cosmological constant problem

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