Toward physical cosmology: focus on inhomogeneous geometry and its non-perturbative effects

DOI10.1088/0264-9381/28/16/164007zbMath1225.83087arXiv1103.2016OpenAlexW3101226085WikidataQ125130925 ScholiaQ125130925MaRDI QIDQ3173064

Thomas Buchert

Publication date: 10 October 2011

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

Full work available at URL: https://arxiv.org/abs/1103.2016

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Philosophical and critical aspects of logic and foundations (03A05) Geometrodynamics and the holographic principle (83E05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)

Related Items (14)

Inhomogeneous universe in \(f(T)\) theory ⋮ Cosmic bulk viscosity through backreaction ⋮ General relativistic cosmological N-body simulations. Part I. Time integration ⋮ On average properties of inhomogeneous fluids in general relativity. III: General fluid cosmologies ⋮ The averaging problem on the past null cone in inhomogeneous dust cosmologies ⋮ Backreaction in cosmic screening approach ⋮ Averaged Lemaître–Tolman–Bondi dynamics ⋮ Dark matter from backreaction? Collapse models on galaxy cluster scales ⋮ Lie sphere geometry in lattice cosmology ⋮ Gauss–Bonnet–Chern approach to the averaged Universe ⋮ Editorial note to: On the Newtonian limit of Einstein's theory of gravitation (by Jürgen Ehlers) ⋮ Relative entropy as a measure of inhomogeneity in general relativity ⋮ PECULIAR ANISOTROPIC STATIONARY SPHERICALLY SYMMETRIC SOLUTION OF EINSTEIN EQUATIONS ⋮ Disappearance and emergence of space and time in quantum gravity

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