Phantom energy-dominated universe as a transient stage in f(R) cosmology
From MaRDI portal
Publication:4972834
DOI10.1142/S0218271819501244zbMath1425.83093arXiv1812.03873OpenAlexW3105390886WikidataQ128038307 ScholiaQ128038307MaRDI QIDQ4972834
Barkha Taori, P. K. Sahoo, P. H. R. S. Moraes, Parbati Sahoo
Publication date: 27 November 2019
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1812.03873
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (3)
Cyclic anisotropic universe in modified gravity with variable deceleration parameter of third degree ⋮ Energy conditions of the f(T, B) gravity dark energy model with the validity of thermodynamics ⋮ Observational constraints in accelerated emergent f(Q) gravity model
Cites Work
- \(f(R)\) theories
- No ``big trips for the universe
- Early and late transient cosmic acceleration due to curvature inspired dark energy
- \(f(R)\) gravity constraints from gravitational waves
- Bouncing cosmologies: progress and problems
- A critical review of classical bouncing cosmologies
- Extended theories of gravity and their cosmological and astrophysical applications
- <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
- A Cyclic Model of the Universe
- Loop quantum cosmology: a status report
- F(R)-gravity and inflation
- Constant-roll inflation in F( R ) gravity
- Loop quantum cosmology-corrected Gauss–Bonnet singular cosmology
- Cosmological perfect-fluids in f(R) gravity
- Loop quantum cosmology scalar field models
- Loop quantum cosmology
This page was built for publication: Phantom energy-dominated universe as a transient stage in f(R) cosmology