Quintessence and holographic dark energy in \(f(T)\) gravity

DOI10.1155/2015/292767zbMath1433.83037OpenAlexW2007357883WikidataQ59102215 ScholiaQ59102215MaRDI QIDQ889046

N. E. Zubov

Publication date: 6 November 2015

Published in: Advances in High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1155/2015/292767

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)

Cites Work

• Unnamed Item
• Dynamical wormhole solutions in \(f(T)\) gravity
• Cosmological constraints on polytropic gas model
• Holographic Chaplygin gas model
• Cosmological reconstruction and stability in \(f(R,T)\) gravity
• Analysis of \(f(R)\) theory corresponding to NADE and NHDE
• Cosmology in scalar-tensor gravity.
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Evolution of the universe in inverse and \(\ln f(R)\) gravity
• ΛCDM epoch reconstruction from F ( R , G ) and modified Gauss–Bonnet gravities
• Cosmological evolution, future singularities, Little Rip and Pseudo-Rip in viable f(R) theories and their scalar–tensor counterpart
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The cosmological constant problem
• New Agegraphic Dark Energy in Brans–Dicke Theory

This page was built for publication: Quintessence and holographic dark energy in \(f(T)\) gravity