f(R) dual theories of quintessence: expansion-collapse duality

DOI10.1088/1475-7516/2021/12/016zbMath1487.83070arXiv2105.10521OpenAlexW3164698278MaRDI QIDQ5064654

H. K. Jassal, Dipayan Mukherjee, Kinjalk Lochan

Publication date: 16 March 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2105.10521

zbMATH Keywords

modified gravitydark energy theory

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Geometrodynamics and the holographic principle (83E05) Rings with involution; Lie, Jordan and other nonassociative structures (16W10) Special Riemannian manifolds (Einstein, Sasakian, etc.) (53C25) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Dark matter and dark energy (83C56) Effective quantum field theories (81T12)

Related Items (1)

Transitioning from a bounce to R ² inflation

Cites Work

• Unnamed Item
• Unnamed Item
• \(f(R)\) theories
• \( F (R)\) gravity with an axion-like particle: dynamics, gravity waves, late and early-time phenomenology
• Collapse models and cosmology
• A new duality transformation for fourth-order gravity
• Can modified gravity explain accelerated cosmic expansion?
• The \(f(R)\) gravity function of the linde quintessence
• Correspondence of \(F(R)\) gravity singularities in Jordan and Einstein frames
• Deceleration versus acceleration universe in different frames of \(F(R)\) gravity
• Cosmological constant -- the weight of the vacuum
• Analyzing the \(H_0\) tension in \(F(R)\) gravity models
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
• A new type of isotropic cosmological models without singularity
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Naked Singularities in the Vaidya Spacetime
• Quintessence: a review
• FOURTH-ORDER GRAVITY AS THE INFLATIONARY MODEL REVISITED
• <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
• Are<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Dark Energy Models Cosmologically Viable?
• DYNAMICS OF DARK ENERGY
• Gravitation
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• Spacetime and Geometry
• Structural aspects of asymptotically safe black holes
• The Four-Dimensionality of Space and the Einstein Tensor
• Quasilocal energy in modified gravity
• Is de Sitter space always excluded in semiclassical f(R) gravity?
• General Relativity
• The cosmological constant

This page was built for publication: f(R) dual theories of quintessence: expansion-collapse duality