The Weyl tensor in spatially homogeneous cosmological models

DOI10.1088/0264-9381/19/20/311zbMath1020.83034arXivgr-qc/0206061OpenAlexW2127832373MaRDI QIDQ4786841

John D. Barrow, Sigbjørn Hervik

Publication date: 13 May 2003

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0206061

zbMATH Keywords

attractorsEinstein field equationsgravitational entropycompact topologyplane-wave spacetimesasymptotic evolutionBianchi and Thurston typehyperbolic space sectionslate-time behaviourspatially homogeneous universeWeyl curvature invariant

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)

Related Items (10)

Perfect fluid Bianchi I model with variable \(G\) and \(\Lambda \) ⋮ An exploration of the black hole entropy in Gauss–Bonnet gravity via the Weyl tensor ⋮ BIANCHI I WITH VARIABLE G AND Λ: SELF-SIMILAR APPROACH ⋮ Indefinite information processing in ever-expanding universes ⋮ A note on the arrow of time in nonminimally coupled scalar field FRW cosmology ⋮ About Bianchi I with VSL ⋮ Fine structure constant, domain walls, and generalized uncertainty principle in the universe ⋮ Bianchi II with time varying constants. Self-similar approach ⋮ Massive cosmic strings in Bianchi type II ⋮ Weyl Curvature Hypothesis in Terms of Spacetime Thermodynamics

This page was built for publication: The Weyl tensor in spatially homogeneous cosmological models