The phenomenology of beyond Horndeski gravity
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Publication:5025558
DOI10.1088/1475-7516/2019/08/035OpenAlexW2948528836MaRDI QIDQ5025558
Pedro G. Ferreira, Dina Traykova, Emilio Bellini
Publication date: 2 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1902.10687
modified gravitycosmological perturbation theorycosmological parameters from LSScosmological parameters from CMBR
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Uses Software
Cites Work
- Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
- Inference from iterative simulation using multiple sequences
- Helicity decomposition of ghost-free massive gravity
- Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
- Mach's Principle and a Relativistic Theory of Gravitation
- A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
- Gravitational wave decay into dark energy
- The sound of DHOST
- Diagnostic of Horndeski theories
- Weakening gravity on redshift-survey scales with kinetic matter mixing
- A unifying description of dark energy
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae