Cosmological background solutions and cosmological backreactions

DOI10.1007/s10714-009-0913-8zbMath1195.85015arXiv0901.4566OpenAlexW2048111466WikidataQ60872036 ScholiaQ60872036MaRDI QIDQ982251

Valerio Marra, Sabino Matarrese, Edward W. Kolb

Publication date: 6 July 2010

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0901.4566

zbMATH Keywords

dark energybackreactionobservational cosmologyinhomogeneous universe models

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

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Cites Work

• Dark energy from structure: a status report
• The 'fitting problem' in cosmology
• Can the acceleration of our universe be explained by the effects of inhomogeneities?
• Effect of Inhomogeneity on Cosmological Models
• Regional averaging and scaling in relativistic cosmology
• Is Dark Energy the Only Solution to the Apparent Acceleration of the Present Universe?
• Cosmological Solutions in Macroscopic Gravity
• Can Inhomogeneities Accelerate the Cosmic Volume Expansion?