Hamiltonian reduction and perturbations of continuously self-similar ( n 1)-dimensional Einstein vacuum spacetimes
From MaRDI portal
Publication:4786829
DOI10.1088/0264-9381/19/21/318zbMath1028.83009OpenAlexW2076779840MaRDI QIDQ4786829
Arthur E. Fischer, Vincent E. Moncrief
Publication date: 19 January 2004
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0264-9381/19/21/318
dynamical systemsvacuum Einstein equationsself-similar spacetimesreduced Hamiltoniansnegative Einstein constant
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20)
Related Items
Stable big bang formation in near-FLRW solutions to the Einstein-scalar field and Einstein-stiff fluid systems ⋮ Collapsing in the Einstein flow ⋮ A regime of linear stability for the Einstein-scalar field system with applications to nonlinear Big Bang formation ⋮ Reflections on the U(1) problem in general relativity ⋮ Asymptotic behavior of a matter filled universe with exotic topology ⋮ On the initial geometry of a vacuum cosmological spacetime ⋮ Attractors of the ‘n + 1’ dimensional Einstein-Λ flow ⋮ Kasner-like regions near crushing singularities * ⋮ The linear stability of the n + 1 dimensional FLRW spacetimes ⋮ On the CMC-Einstein-Λ flow
