The inflationary scenario in the f(R) gravity model with a R 4 term
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Publication:5164343
DOI10.1088/1361-6382/AC2DD0zbMath1479.83233OpenAlexW3207077873MaRDI QIDQ5164343
Sohan Kumar Jha, Sahazada Aziz, Anisur Rahaman
Publication date: 11 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/1361-6382/ac2dd0
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
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An exact solution of the higher-order gravity in standard radiation-dominated era ⋮ Effect of electric field on string-oriented perfect fluid collapse in f (R) gravity ⋮ A class of traversable wormholes in the Starobinsky-like \(f(R)\) gravity with anisotropic dark matter
Cites Work
- \(f(R)\) theories
- \(R + \alpha R^n\) inflation in higher-dimensional space-times
- Superconformal inflationary \(\alpha\)-attractors
- Beyond the Starobinsky model for inflation
- Unitary inflaton as decaying dark matter
- Starobinsky-like inflation from induced gravity
- A new type of isotropic cosmological models without singularity
- A new approach to reconstruction methods in f ( R ) gravity
- <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
- Slow-roll inflation in the ( R + R 4 ) gravity
- MODELS OF CHAOTIC INFLATION
- Inflationary universe: A possible solution to the horizon and flatness problems
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