Rotating Bianchi type V dust models generalizing the k=−1 Friedmann model

DOI10.1063/1.1330197zbMath1063.83522arXivgr-qc/0005109OpenAlexW3103053756MaRDI QIDQ2774664

Andrzej Krasiński

Publication date: 26 February 2002

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0005109

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (4)

Observational assessment of the viability of De Sitter Gödel De Sitter phase transition ⋮ Closed timelike loops in homogeneous rotating \(\varLambda\)-dust cosmologies ⋮ GLOBAL AND LOCAL EFFECTS OF ROTATION: OBSERVATIONAL ASPECTS ⋮ Friedmann limits of rotating hypersurface–homogeneous dust models

Cites Work

• The program ORTOCARTAN for algebraic calculations in relativity
• Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. I. Two Killing fields spanned on uα and wα
• Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. II. One Killing field spanned on uα and wα
• Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα

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