Study of entropy-corrected models using dark energy in the framework of a complementary gravitational field

DOI10.1134/S0202289319030034zbMath1437.83159OpenAlexW2970454058WikidataQ127280444 ScholiaQ127280444MaRDI QIDQ2297676

Mustafa M. Selim, Ayman A. Aly

Publication date: 20 February 2020

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0202289319030034

zbMATH Keywords

Hubble parameterdark energyobservationsstatefinder parameterscomplementary gravitational fieldentropy-corrected models

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40) Quantum entropies (81P17) Dark matter and dark energy (83C56)

Cites Work

• Unnamed Item
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• On the \(\Lambda \)CDM universe in \(f(G)\) gravity
• Hořava-Lifshitz cosmology
• Cosmological evolution of pilgrim dark energy in \(f(G)\) gravity
• Energy conditions in generalized teleparallel gravity models
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• DYNAMICS OF DARK ENERGY

This page was built for publication: Study of entropy-corrected models using dark energy in the framework of a complementary gravitational field