Non-Local Curvature Gravity Cosmology via Noether Symmetries
arXiv:2111.07285 · doi:10.1016/j.physletb.2022.136907
Abstract
We consider extensions of General Relativity based on the non-local function , where is the Ricci curvature scalar and the non-locality is due to the term . We focus on cosmological minisuperspaces and select viable models by the Noether Symmetry Approach. Then we find viable exact solutions pointing out the role of non-locality in cosmology.
arXiv comment13 pages
References in corpus (41)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- The Cosmological Constant and Dark Energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Modified Gravity and Cosmology
- f(R) theories
- Extended Theories of Gravity
- Cosmological Constant - the Weight of the Vacuum
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Towards singularity and ghost free theories of gravity
- Super-renormalizable Quantum Gravity
- Nonlocal Cosmology
- Spherically symmetric solutions in f(R)-gravity via Noether Symmetry Approach
- Modified non-local-F(R) gravity as the key for the inflation and dark energy
- Bouncing Cosmology in f(Q) Symmetric Teleparallel Gravity
- Hamiltonian dynamics and Noether symmetries in Extended Gravity Cosmology
- Accelerating cosmologies from non-local higher-derivative gravity
- Phantom and non-phantom dark energy: The cosmological relevance of non-locally corrected gravity
- Classical properties of non-local, ghost- and singularity-free gravity
- Early modified gravity in light of the tension and LSS data
- Ghost-free infinite derivative quantum field theory
- Consistent Higher Derivative Gravitational theories with stable de Sitter and Anti-de Sitter Backgrounds
- Inflation in (Super-)renormalizable Gravity
- New Spherically Symmetric Solutions in f(R)-gravity by Noether Symmetries
- Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
- Super-renormalizable or finite completion of the Starobinsky theory
- Addressing tension by means of VCDM
- f(G) Noether cosmology
- Noether Symmetries as a geometric criterion to select theories of gravity
- Addressing the cosmological tension by the Heisenberg uncertainty
- Constraining Generalized Non-local Cosmology from Noether Symmetries
- Aspects of Nonlocality in Quantum Field Theory, Quantum Gravity and Cosmology
- Considerations on gravitational waves in higher-order local and non-local gravity
- Noether Symmetries and Quantum Cosmology in Extended Teleparallel Gravity
- Constraining Non-local Gravity by S2 star orbits
- Gravitational waves in non-local gravity
- Equivalence of non-minimally coupled cosmologies by Noether symmetries
- Non-Local Curvature and Gauss-Bonnet Cosmologies by Noether Symmetries
- De Sitter and Power-law Solutions in Non-local Gauss-Bonnet Gravity
- The Noether Bessel Hagen Symmetry Approach for Dynamical Systems
- Logarithmic corrections to Newtonian gravity and Large Scale Structure
- Flat, radiation universes with quadratic corrections and asymptotic analysis
Cited by in corpus (13)
- Late-time constraints on modified Gauss-Bonnet cosmology
- The phase-space view of non-local gravity cosmology
- A Review of Stable, Traversable Wormholes in f (R) Gravity Theories
- Testing non-local gravity by clusters of galaxies
- Minisuperspace Quantum Cosmology in Metric and Affine Theories of Gravity
- Lagrangian reconstruction of Barrow holographic dark energy in interacting tachyon model
- Exploring departures from Schwarzschild black hole in gravity
- The energy-momentum complex in non-local gravity
- Velocity distribution of elliptical galaxies in the framework of Non-local Gravity model
- Testing non-local gravity through Ultra-Diffuse Galaxies kinematics
- Analytical CDM dynamics
- Nonlocal Lagrangian fields and the second Noether theorem. Non-commutative gauge theory
- Generic autonomous system approach to interacting dark energy models