Late-time constraints on modified Gauss-Bonnet cosmology

DOI10.1007/s10714-023-03092-wzbMath1528.83122arXiv2208.02677OpenAlexW4324141832MaRDI QIDQ6174854

Francesco Bajardi, Rocco D'Agostino

Publication date: 15 July 2023

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2208.02677

zbMATH Keywords

cosmologyNoether symmetriesdark energymodified theories of gravity

Mathematics Subject Classification ID

Monte Carlo methods (65C05) Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Constrained dynamics, Dirac's theory of constraints (70H45) Symmetries and conservation laws, reverse symmetries, invariant manifolds and their bifurcations, reduction for problems in Hamiltonian and Lagrangian mechanics (70H33) Dark matter and dark energy (83C56)

Cites Work

• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• \(f(R)\) theories
• On non-abelian generalisation of the Born-Infeld action in string theory
• Can modified gravity explain accelerated cosmic expansion?
• Cosmological constant -- the weight of the vacuum
• The geometry of gauge fields
• Non-local curvature gravity cosmology via Noether symmetries
• Cosmological viability of a double field unified model from warm inflation
• Extended matter bounce scenario in ghost free \(f(R, \mathcal{G})\) gravity compatible with GW170817
• \(F(R,G)\) cosmology through Noether symmetry approach
• Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
• From Big to Little Rip in modified \(F(R,G)\) gravity
• Cosmography: Cosmology without the Einstein equations
• Noether symmetry approach in Gauss–Bonnet cosmology
• <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
• The cosmological constant and dark energy
• 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?
• Lovelock-Cartan theory of gravity
• DYNAMICS OF DARK ENERGY
• Newtonian, Post-Newtonian and Parametrized Post-Newtonian limits of f(R, 𝒢) gravity
• Modified Gauss–Bonnet gravity with the Lagrange multiplier constraint as mimetic theory
• ΛCDM epoch reconstruction from F ( R , G ) and modified Gauss–Bonnet gravities
• Dynamical analysis on $f(R, \mathcal{G})$ cosmology
• Noether symmetries as a geometric criterion to select theories of gravity
• Equivalence of nonminimally coupled cosmologies by Noether symmetries
• Extended gravity cosmography
• Exact solutions in higher-dimensional Lovelock and AdS ₅ Chern-Simons gravity
• Bottom-up reconstruction of viable GW170817 compatible Einstein–Gauss–Bonnet theories
• A refined Einstein–Gauss–Bonnet inflationary theoretical framework
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• The Einstein Tensor and Its Generalizations
• Monte Carlo sampling methods using Markov chains and their applications
• Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field
• The cosmological constant
• Noether symmetries and quantum cosmology in extended teleparallel gravity
• The Noether–Bessel-Hagen symmetry approach for dynamical systems