Observational constraints in nonlocal gravity: the Deser-Woodard case

DOI10.1088/1475-7516/2019/03/045OpenAlexW3105026661WikidataQ128140703 ScholiaQ128140703MaRDI QIDQ5862137

Henrik Nersisyan, Yves Dirian, Sohyun Park, Luca Amendola

Publication date: 4 March 2022

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

Full work available at URL: https://arxiv.org/abs/1901.07832

zbMATH Keywords

gravitymodified gravitydark energy theory

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (4)

Nonlocal cosmology II. Cosmic acceleration without fine tuning or dark energy ⋮ Probing alternative cosmologies through the inverse distance ladder ⋮ Limited modified gravity ⋮ Constraints on non-local gravity from binary pulsars gravitational emission

Uses Software

• Monte Python
• CLASS

Cites Work

• Unnamed Item
• Nonlocal models of cosmic acceleration
• Cosmological constant -- the weight of the vacuum
• Challenges to self-acceleration in modified gravity from gravitational waves and large-scale structure
• Quintessence: a review
• Cosmography with the Einstein Telescope
• Nonlocal Cosmology
• Nonlocal gravity. Conceptual aspects and cosmological predictions
• No slip gravity
• On nonlocally interacting metrics, and a simple proposal for cosmic acceleration
• Doppelgänger dark energy: modified gravity with non-universal couplings after GW170817
• Structure formation in the Deser-Woodard nonlocal gravity model: a reappraisal
• A unifying description of dark energy
• Ghosts in the self-accelerating universe
• The cosmological constant problem
• The Einstein Tensor and Its Generalizations
• The Four-Dimensionality of Space and the Einstein Tensor
• Testing nonlocal gravity with Lunar Laser Ranging
• 4D gravity on a brane in 5D Minkowski space

This page was built for publication: Observational constraints in nonlocal gravity: the Deser-Woodard case