Dark sector evolution in Horndeski models

DOI10.1088/1475-7516/2019/09/018OpenAlexW3104116693MaRDI QIDQ5861833

Boris Bolliet, Francesco Pace, Damien Trinh, Battye, Richard A.

Publication date: 2 March 2022

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

Full work available at URL: https://arxiv.org/abs/1905.06795

zbMATH Keywords

gravitymodified gravitydark energy theory

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (5)

Fully relativistic predictions in Horndeski gravity from standard Newtonian N-body simulations ⋮ hi_class background evolution, initial conditions and approximation schemes ⋮ An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations ⋮ Relativistic corrections to the growth of structure in modified gravity ⋮ Comparison of different approaches to the quasi-static approximation in Horndeski models

Uses Software

• CMBEASY
• CAMB
• CLASS

Cites Work

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