Cosmological model with \({\Omega}_M\)-dependent cosmological constant

DOI10.1023/A:1024012816760zbMath1031.83030arXivastro-ph/0310609MaRDI QIDQ1398089

Vladimir Majernik

Publication date: 6 August 2003

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0310609

zbMATH Keywords

expansionuniversequintessencedark energystress-energy tensorobservationscosmological scenario

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Astrophysical cosmology (85A40)

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Kaluza-Klein Type Cosmological Model with Ω–Dependent Cosmological Constant and Big Rip Singularity ⋮ Null Fluid Collapse in Rastall Theory of Gravity ⋮ The commutator algebra of covariant derivative as general framework for extended gravity. The Rastall theory case and the role of the torsion ⋮ Einstein equations with fluctuating volume ⋮ 4-Index theory of gravity and its relation with the violation of the energy–momentum conservation law ⋮ Quasinormal Modes of the Schwarzschild Black Hole Surrounded by the Quintessence Field in Rastall Gravity

Cites Work

• Cosmology of general relativity without energy-momentum conservation
• Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
• The cosmological constant is back
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• The cosmic acceleration due to an alternative interpretation of the cosmological constant

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