Nonlinear effective theory of dark energy

DOI10.1088/1475-7516/2018/04/061OpenAlexW2772278655WikidataQ125680916 ScholiaQ125680916MaRDI QIDQ5022328

Matthew Lewandowski, Filippo Vernizzi, Giulia Cusin

Publication date: 18 January 2022

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

Full work available at URL: https://arxiv.org/abs/1712.02782

zbMATH Keywords

power spectrummodified gravitydark energy theorycosmological parameters from LSS

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (15)

Shift-symmetric Horndeski gravity in the asymptotic-safety paradigm ⋮ Effective field theory of dark energy: a review ⋮ The large scale structure bootstrap: perturbation theory and bias expansion from symmetries ⋮ k-evolution: a relativistic N-body code for clustering dark energy ⋮ Resonant decay of gravitational waves into dark energy ⋮ hi_class background evolution, initial conditions and approximation schemes ⋮ Dark-energy instabilities induced by gravitational waves ⋮ Constraints on modified gravity from the BOSS galaxy survey ⋮ Parity violation in the scalar trispectrum: no-go theorems and yes-go examples ⋮ Effective field theory of black hole perturbations with timelike scalar profile: formulation ⋮ Hi-COLA: fast, approximate simulations of structure formation in Horndeski gravity ⋮ Instabilities appearing in cosmological effective field theories: when and how? ⋮ Revisiting Vainshtein screening for fast N-body simulations ⋮ Gravitational wave decay into dark energy ⋮ Parameterised post-Newtonian formalism for the effective field theory of dark energy via screened reconstructed Horndeski theories

Uses Software

• gevolution

Cites Work

• Starting the universe: stable violation of the null energy condition and non-standard cosmologies
• Large-scale structure of the universe and cosmological perturbation theory
• The effective field theory of cosmological large scale structures
• An introduction to the Vainshtein mechanism
• Effective field theory of cosmological perturbations
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• Tackling non-linearities with the effective field theory of dark energy and modified gravity
• Weakening gravity on redshift-survey scales with kinetic matter mixing
• A unifying description of dark energy

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