Emergent cosmological expansion in scalar-tensor theories of gravity
From MaRDI portal
Publication:6657363
DOI10.1088/1361-6382/ad9880MaRDI QIDQ6657363
Chad Briddon, Timothy Clifton, Pierre Fleury
Publication date: 6 January 2025
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Unnamed Item
- Unnamed Item
- Tests of chameleon gravity
- Cosmology without averaging
- Ray tracing and Hubble diagrams in post-Newtonian cosmology
- SELCIE: a tool for investigating the chameleon field of arbitrary sources
- Multi-scale perturbation theory. Part I. Methodology and leading-order bispectrum corrections in the matter-dominated era
- Multi-scale perturbation theory II: Solutions and leading-order bispectrum in the ΛCDM universe
- The momentum constraint equation in parameterised post-Newtonian cosmology
- Chameleon screening depends on the shape and structure of NFW halos
- Junction conditions in scalar–tensor theories
- Gravity
- k-MOUFLAGE GRAVITY
- Parameterized post-Newtonian cosmology
- Mach's Principle and Invariance under Transformation of Units
- Riemannian geometry.
- Scale-dependent gravitational couplings in Parameterised Post-Newtonian Cosmology
- Hi-COLA: fast, approximate simulations of structure formation in Horndeski gravity
- Inconsistency of modified gravity in cosmology
This page was built for publication: Emergent cosmological expansion in scalar-tensor theories of gravity