Inflation and dark energy in f(R, X, ϕ) gravity

DOI10.1142/S0217732318502152zbMath1402.83079OpenAlexW2898536800MaRDI QIDQ4558778

A. I. Keskin

Publication date: 30 November 2018

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

Full work available at URL: https://doi.org/10.1142/s0217732318502152

zbMATH Keywords

inflationscalar fieldsdark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (2)

Traversable phantom wormholes via conformal symmetry in f(R,φ,χ) gravity ⋮ Galileon inflation field with three dark eras of the universe

Cites Work

• \(f(R)\) theories
• A new type of isotropic cosmological models without singularity
• Extended theories of gravity and their cosmological and astrophysical applications
• Extended scalar–tensor theory and thermodynamics in teleparallel framework
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• Matter bounce cosmology with the f ( T ) gravity
• A unified picture of cosmological entropy on apparent horizon in F(R, G) gravity
• CURVATURE QUINTESSENCE
• Super inflation mechanism with oscillating scalar fields in F(R,T) gravity
• Connecting early and late universe by f(R) gravity
• Inflationary universe: A possible solution to the horizon and flatness problems
• Inflationary cosmology in unimodular F(T) gravity

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