The reduced Einstein equations and the conformal volume collapse of 3-manifolds
From MaRDI portal
Publication:2769503
DOI10.1088/0264-9381/18/21/308zbMath0998.83008OpenAlexW1968409818MaRDI QIDQ2769503
Arthur E. Fischer, Vincent E. Moncrief
Publication date: 21 November 2002
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0264-9381/18/21/308
Bianchi modelsEinstein equationsreduced Hamiltonianconstraint equationsgauge conditionsvolume collapse
Lua error in Module:PublicationMSCList at line 37: attempt to index local 'msc_result' (a nil value).
Related Items (11)
Stable big bang formation in near-FLRW solutions to the Einstein-scalar field and Einstein-stiff fluid systems ⋮ Optical knots and contact geometry. I: From Arnol'd inequality to Ranada's dyons ⋮ On curvature decay in expanding cosmological models ⋮ A regime of linear stability for the Einstein-scalar field system with applications to nonlinear Big Bang formation ⋮ Optical knots and contact geometry. II: From Ranada dyons to transverse and cosmetic knots ⋮ Future stability of the Einstein-non-linear scalar field system ⋮ Harmonic analysis of linear fields on the nilgeometric cosmological model ⋮ Instability of spatially homogeneous solutions in the class of \(\mathbb T^2\)-symmetric solutions to Einstein's vacuum equations ⋮ Stability within \(T^2\)-symmetric expanding spacetimes ⋮ On the asymptotic spectrum of the reduced volume in cosmological solutions of the Einstein equations ⋮ On the CMC-Einstein-Λ flow
This page was built for publication: The reduced Einstein equations and the conformal volume collapse of 3-manifolds
