Parameterised post-Newtonian formalism for the effective field theory of dark energy via screened reconstructed Horndeski theories

DOI10.1088/1475-7516/2020/12/032zbMath1484.83050arXiv2006.09910OpenAlexW3036076788WikidataQ125061672 ScholiaQ125061672MaRDI QIDQ5027095

Lucas Lombriser, Joe Kennedy, Cyril Renevey

Publication date: 3 February 2022

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

Full work available at URL: https://arxiv.org/abs/2006.09910

zbMATH Keywords

modified gravitydark energy theory

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Gravitational waves (83C35) Dark matter and dark energy (83C56) Effective quantum field theories (81T12)

Related Items

Scalar fields near compact objects: resummation versus UV completion ⋮ Constraining Horndeski theory with gravitational waves from coalescing binaries ⋮ Robustness of the cosmological constant damping mechanism through matter eras

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