On curvature decay in expanding cosmological models

DOI10.1007/s00220-005-1470-yzbMath1117.83014OpenAlexW2158203915MaRDI QIDQ865058

Hans Ringström

Publication date: 13 February 2007

Published in: Communications in Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s00220-005-1470-y

Mathematics Subject Classification ID

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

Related Items (5)

Collapsing in the Einstein flow ⋮ Backreaction in the future behavior of an expanding vacuum spacetime ⋮ Future stability of the Einstein-non-linear scalar field system ⋮ Instability of spatially homogeneous solutions in the class of \(\mathbb T^2\)-symmetric solutions to Einstein's vacuum equations ⋮ On the asymptotic spectrum of the reduced volume in cosmological solutions of the Einstein equations

Cites Work

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• Data at the moment of infinite expansion for polarized Gowdy
• On a wave map equation arising in general relativity
• The Geometries of 3-Manifolds
• Dynamical Systems in Cosmology
• The Bianchi IX attractor
• On long-time evolution in general relativity and geometrization of 3-manifolds

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