Can the Hubble tension be resolved by bulk viscosity?

DOI10.1142/S0217732321501984zbMath1489.83023arXiv2107.13533OpenAlexW3200289230MaRDI QIDQ5067298

Iver Brevik, Ben David Normann

Publication date: 1 April 2022

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2107.13533

zbMATH Keywords

Hubble tensionbulk-viscous cosmology

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Viscous-inviscid interaction for compressible fluids and gas dynamics (76N17)

Cites Work

• Phase space analysis of bulk viscous matter dominated universe
• Analyzing the \(H_0\) tension in \(F(R)\) gravity models
• Bulk viscosity driving the acceleration of the universe
• Characteristic properties of two different viscous cosmology models for the future universe
• On the viability of the truncated Israel–Stewart theory in cosmology
• Viscous self interacting dark matter cosmology for small redshift

This page was built for publication: Can the Hubble tension be resolved by bulk viscosity?