Analyzing the \(H_0\) tension in \(F(R)\) gravity models

DOI10.1016/J.NUCLPHYSB.2021.115377OpenAlexW3099767851MaRDI QIDQ2232536

Sergei D. Odintsov, G. S. Sharov, Diego Sáez-Chillón Gómez

Publication date: 6 October 2021

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2011.03957

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Nuclear physics (81V35) Geometrodynamics and the holographic principle (83E05) Quantum optics (81V80) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Galactic and stellar structure (85A15) Dark matter and dark energy (83C56) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (8)

Is there evidence for CIDER in the Universe? ⋮ Integral \(F(R)\) gravity and saddle point condition as a remedy for the \(H_0\)-tension ⋮ f(R) dual theories of quintessence: expansion-collapse duality ⋮ Can the Hubble tension be resolved by bulk viscosity? ⋮ Cosmological distances and Hubble tension in Einstein-Cartan theory ⋮ Early dark energy with power-law \(F(R)\) gravity ⋮ Lagrangian formulation and implications of barotropic fluid cosmologies ⋮ An axially symmetric transitioning models with observational constraints

Cites Work

• A new look at the statistical model identification

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