Brans–Dicke cosmology with a Λ-term: a possible solution to ΛCDM tensions*

DOI10.1088/1361-6382/abbc43OpenAlexW3100368830MaRDI QIDQ5162434

Joan Solà Peracaula, Adrià Gómez-Valent, Cristian Moreno-Pulido, Javier de Cruz Pérez

Publication date: 2 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2006.04273

zbMATH Keywords

cosmological constantdark energyquantum field theory in curved spacetimescalar-tensor theories of gravitation

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Oscillation, zeros of solutions, mean value theorems, etc. in context of PDEs (35B05) Quantum field theory on curved space or space-time backgrounds (81T20) Quantum optics (81V80) Atomic physics (81V45) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Galactic and stellar structure (85A15) Matrix models and tensor models for quantum field theory (81T32) Dark matter and dark energy (83C56)

Related Items (8)

Landau damping for gravitational waves in parity-violating theories ⋮ Stability of scalar perturbations in scalar-torsion f(T,ϕ) gravity theories in the presence of a matter fluid ⋮ Difficulties in reconciling non-negligible differences between the local and cosmological values of the gravitational coupling in extended Brans-Dicke theories ⋮ Phantom scalar-tensor models and cosmological tensions ⋮ Cosmological distances and Hubble tension in Einstein-Cartan theory ⋮ Stringy running vacuum model and current tensions in cosmology ⋮ Long range interactions in cosmology: implications for neutrinos ⋮ Can scale-dependent cosmology alleviate the H₀ tension?

Uses Software

• GetDist
• CLASS

Cites Work

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