Noether symmetry for Gauss-Bonnet dilatonic gravity
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Publication:648103
DOI10.1007/s10714-011-1207-5zbMath1228.83100arXiv1107.0560OpenAlexW3100086246MaRDI QIDQ648103
Ester Piedipalumbo, Claudio Rubano, Abhik Kumar Sanyal
Publication date: 22 November 2011
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1107.0560
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
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Why Noether symmetry of \(F(R)\) theory yields three-half power law? ⋮ Noether symmetry approach in Gauss–Bonnet cosmology ⋮ Analyzing conserved currents in F(R) theory of gravity ⋮ Noether symmetry in \(f(T)\) teleparallel gravity ⋮ Viability of Noether symmetry of \(F(R)\) theory of gravity ⋮ The role of cosmological constant in f(R, G) gravity ⋮ Early Universe in view of a modified theory of gravity ⋮ Topological invariant quintessence ⋮ Reconstruction of \(F(T)\) gravity in homogeneous backgrounds and a general prescription for reconstructing through scalar field ⋮ Exact cosmological solutions of \(f(R)\) theories via Hojman symmetry
Cites Work
- Dynamical relaxation of dark energy: a solution to early inflation, late-time acceleration and the cosmological constant problem
- Dark energy from modified \(F(R)\)-scalar-Gauss-Bonnet gravity
- Emergent universe scenario in the Einstein-Gauss-Bonnet gravity with dilaton
- Transient crossing of phantom divide line \(w_{\Lambda} = - 1\) under Gauss-Bonnet interaction
- On some exponential potentials for a cosmological scalar field as quintessence
- Noether symmetry in the higher order gravity theory
- On compatibility of string effective action with an accelerating universe
- Symmetric vacuum scalar - tensor cosmology
- Cosmological models in scalar tensor theories of gravity and observations: a class of general solutions
- Dark energy and cosmological solutions in second-order string gravity