Nonlocal cosmology II. Cosmic acceleration without fine tuning or dark energy

DOI10.1088/1475-7516/2019/06/034OpenAlexW3106130123WikidataQ127664807 ScholiaQ127664807MaRDI QIDQ5031377

Stanley Deser, Richard Woodard

Publication date: 18 February 2022

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

Full work available at URL: https://arxiv.org/abs/1902.08075

zbMATH Keywords

quantum cosmologymodified gravitydark energy theory

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (8)

Ricci-inverse gravity: a novel alternative gravity, its flaws, and how to cure them ⋮ Structure formation in the new Deser-Woodard nonlocal gravity model ⋮ Gravity in the infrared and effective nonlocal models ⋮ Non-local gravity in bouncing cosmology scenarios ⋮ The energy–momentum complex in non-local gravity ⋮ Structure formation in non-local bouncing models ⋮ Field-theoretic derivation of bubble-wall force ⋮ Testing modified gravity at cosmological distances with LISA standard sirens

Cites Work

• Modified non-local-\(F(R)\) gravity as the key for the inflation and dark energy
• Nonlocal models of cosmic acceleration
• Nonperturbative models for the quantum gravitational back-reaction on inflation
• Quantum scalar corrections to the gravitational potentials on de Sitter background
• Quantum gravity slows inflation
• Nonlocal Cosmology
• Quantum Gravity and Inflation
• Structure formation in the Deser-Woodard nonlocal gravity model: a reappraisal
• The cosmological constant problem
• Testing nonlocal gravity with Lunar Laser Ranging
• Observational constraints in nonlocal gravity: the Deser-Woodard case
• The cosmological constant

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