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Автор Nazeem Mustapha
Автор George F R Ellis
Автор Henk van Elst
Автор Mattias Marklund
Дата выпуска 2000-08-21
dc.description We show that there are no new consistent cosmological perfect fluid solutions when in an open neighbourhood U of an event the fluid kinematical variables and the electric and magnetic Weyl curvature are all assumed to be rotationally symmetric about a common spatial axis, specializing the Weyl curvature tensor to algebraic Petrov type D. The consistent solutions of this kind are either locally rotationally symmetric, or are subcases of the Szekeres dust models. Parts of our results require the assumption of a barotropic equation of state. Additionally we demonstrate that local rotational symmetry of perfect fluid cosmologies follows from rotational symmetry of the Riemann curvature tensor and of its covariant derivatives only up to second order, thus strengthening a previous result.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Partially locally rotationally symmetric perfect fluid cosmologies
Тип paper
DOI 10.1088/0264-9381/17/16/304
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 17
Первая страница 3135
Последняя страница 3156
Аффилиация Nazeem Mustapha; Cosmology Group, Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701, Cape Town, South Africa
Аффилиация George F R Ellis; Cosmology Group, Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701, Cape Town, South Africa
Аффилиация Henk van Elst; Cosmology Group, Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701, Cape Town, South Africa
Аффилиация Mattias Marklund; Cosmology Group, Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701, Cape Town, South Africa
Выпуск 16

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