Anisotropic homogeneous cosmologies in the post-Newtonian approximation

DOI10.1023/A:1010280332043zbMath0989.83074arXivgr-qc/0007061OpenAlexW1814453540MaRDI QIDQ5947444

Tamath Rainsford

Publication date: 2001

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0007061

zbMATH Keywords

cosmologyBianchi typespost-Newtonian approximationwell posed

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (2)

Adding twist to anisotropic fluids ⋮ More problems for Newtonian cosmology

Cites Work

• Newtonian and post-Newtonian approximations of the \(k=0\) Friedmann-Robertson-Walker cosmology
• Relativistic Cosmology. I
• Homogeneous Newtonian cosmologies and their perturbations
• Empty space-times admitting a three parameter group of motions

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