Linearization stability of the Einstein equation for Robertson–Walker models. I

DOI10.1063/1.533019zbMath0982.83008OpenAlexW2079658133MaRDI QIDQ4498422

Lluís Bruna, Joan Girbau

Publication date: 16 August 2000

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

Full work available at URL: https://doi.org/10.1063/1.533019

zbMATH Keywords

Einstein equationspacelike hypersurfaceperfect fluidRobertson-Walker modelsstress-energy tensorlinearization stability

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (4)

Linearization stability of the Einstein constraint equations on an asymptotically hyperbolic manifold ⋮ Linearization stability of the Einstein equation for Robertson–Walker models. II ⋮ Cosmology with curvature-saturated gravitational Lagrangian \(R/\sqrt{1 + l^4 R^2}\) ⋮ Laplacian in the hyperbolic space Hn and linearization stability of the Einstein equation for Robertson-Walker models

Cites Work

• Unnamed Item
• On the existence of perturbed Robertson-Walker universes
• The Einstein evolution equations as a first-order quasi-linear symmetric hyperbolic system. I
• On the stability of flat space
• Spacetime symmetries and linearization stability of the Einstein equations. I
• The Einstein Equations of Evolution-A Geometric Approach

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