Dark energy loopholes some time after GW170817

DOI10.1088/1475-7516/2020/11/063zbMath1486.83065arXiv2006.06652OpenAlexW3035113871MaRDI QIDQ5035313

Edmund J. Copeland, Lorenzo Bordin, Antonio Padilla

Publication date: 21 February 2022

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

Full work available at URL: https://arxiv.org/abs/2006.06652

zbMATH Keywords

modified gravitydark energy theorygravitational waves/theory

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35) Dark matter and dark energy (83C56) Effective quantum field theories (81T12)

Related Items (5)

Horndeski stars ⋮ Generalised scalar-tensor theories and self-tuning ⋮ Dynamical dark energy models in the light of gravitational-wave transient catalogues ⋮ Horndeski fermion–boson stars ⋮ Scalar-tensor cosmologies without screening

Cites Work

• Challenges to self-acceleration in modified gravity from gravitational waves and large-scale structure
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• DYNAMICS OF DARK ENERGY
• Simplifying the EFT of Inflation: generalized disformal transformations and redundant couplings
• Doppelgänger dark energy: modified gravity with non-universal couplings after GW170817
• Gravitational wave decay into dark energy
• The Super-Stückelberg procedure and dS in pure supergravity
• Dark energy in Horndeski theories after GW170817: A review
• Quintessence and supergravity

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