Dynamics of inflation and dark energy from \(F(R, \mathcal{G})\) gravity

DOI10.1016/j.nuclphysb.2018.07.013zbMath1405.83083arXiv1807.00335OpenAlexW2810389460MaRDI QIDQ1710216

Peng Zhang

Publication date: 15 January 2019

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1807.00335

Mathematics Subject Classification ID

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

Related Items (24)

The interplay between the dark matter axion and primordial black holes ⋮ Late time cosmology in f(R,G) -gravity with interacting fluids ⋮ The gravitational field outside a spatially compact stationary source in a generic fourth-order theory of gravity ⋮ Observational constrained gravity cosmological model and the dynamical system analysis ⋮ How a Conformally Flat Impacts Gauss‐Bonnet Gravity? ⋮ Finite-time cosmological singularities and the possible fate of the universe ⋮ Noether symmetries and quantum cosmology in extended teleparallel gravity ⋮ The fate of the universe evolution in the quadratic form of Ricci-Gauss-Bonnet cosmology ⋮ Observational constraints on a transit cosmological model in f(R,G) gravity ⋮ Anisotropic compact stars in \(f(\mathcal{R}, \mathcal{A})\) gravity including charge with exterior Reissner-Nordstrom spacetime ⋮ The inflationary era of the universe via Tsallis cosmology ⋮ Unnamed Item ⋮ Gravitational waves in modified Gauss–Bonnet gravity ⋮ De Sitter and power-law solutions in non-local Gauss–Bonnet gravity ⋮ Bouncing cosmology in \(f(R,\mathcal{G})\) gravity by order reduction ⋮ Cosmological viable models in f ( T , B ) theory as solutions to the H ₀ tension ⋮ Scalaron tunneling and the fate of antisymmetric tensor fields in F(R) gravity ⋮ Inflationary cosmology in \(f(R,T)\) modified gravity ⋮ Progress eras of the universe with spacetime dimensions ⋮ Cosmological perturbations in f(G) gravity ⋮ New cosmological solutions in hybrid metric-Palatini gravity from dynamical symmetries ⋮ \(F(R,G)\) cosmology through Noether symmetry approach ⋮ Inflationary magnetogenesis with reheating phase from higher curvature coupling ⋮ Effective theory of inflationary magnetogenesis and constraints on reheating

Cites Work

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