Phantom scalar-tensor models and cosmological tensions

DOI10.1088/1475-7516/2023/04/029zbMath1522.83406arXiv2302.05291OpenAlexW4364381965MaRDI QIDQ6044351

Unnamed Author, Fabio Finelli, Unnamed Author

Publication date: 17 May 2023

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

Full work available at URL: https://arxiv.org/abs/2302.05291

zbMATH Keywords

modified gravitydark energy theorycosmological parameters from CMBRcosmological perturbation theory in GR and beyond

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Diffraction, scattering (78A45) Quantum optics (81V80) Hydro- and aero-acoustics (76Q05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Formal methods and deformations in algebraic geometry (14D15) Applications of Jordan algebras to physics, etc. (17C90) Matrix models and tensor models for quantum field theory (81T32) Dark matter and dark energy (83C56)

Cites Work

• Cosmology and broken scale invariance
• Brans–Dicke cosmology with a Λ-term: a possible solution to ΛCDM tensions*
• Variations of the gravitational constant from lunar laser ranging data
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Testing nonlocal gravity with Lunar Laser Ranging
• Testing extended Jordan-Brans-Dicke theories with future cosmological observations
• Perturbations in \(k\)-inflation

This page was built for publication: Phantom scalar-tensor models and cosmological tensions