Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. II. One Killing field spanned on uα and wα

DOI10.1063/1.532336zbMath0907.53056arXivgr-qc/9705078OpenAlexW2295365223MaRDI QIDQ4212636

Andrzej Krasiński

Publication date: 4 March 1999

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9705078

zbMATH Keywords

exact solutionsEinstein equationsrotating dust matter

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)

Related Items (5)

Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα ⋮ Closed timelike loops in homogeneous rotating \(\varLambda\)-dust cosmologies ⋮ GLOBAL AND LOCAL EFFECTS OF ROTATION: OBSERVATIONAL ASPECTS ⋮ Rotating Bianchi type V dust models generalizing the k=−1 Friedmann model ⋮ Friedmann limits of rotating hypersurface–homogeneous dust models

Cites Work

• A relativistically rotating fluid cylinder
• The program ORTOCARTAN for algebraic calculations in relativity
• On the thermodynamical interpretation of perfect fluid solutions of the Einstein equations with no symmetry
• New Homogeneous Solutions of Einstein's Field Equations with Incoherent Matter Obtained by a Spinor Technique
• An Example of a New Type of Cosmological Solutions of Einstein's Field Equations of Gravitation

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