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1996
DOI: 10.1088/0264-9381/13/5/032
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Perfect-fluid cylinders and walls - sources for the Levi-Civita spacetime

Abstract: The diagonal metric tensor whose components are functions of one spatial coordinate is considered. Einstein's field equations for a perfect-fluid source are reduced to quadratures once a generating function, equal to the product of two of the metric components, is chosen. The solutions are either static fluid cylinders or walls depending on whether or not one of the spatial coordinates is periodic. Cylinder and wall sources are generated and matched to the vacuum (LeviCivita) space-time. A match to a cylinder … Show more

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Cited by 41 publications
(41 citation statements)
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“…Thus for example one could assume µ = constant, P z = P φ = P r , then we can integrate (11) to obtain…”
Section: Discussionmentioning
confidence: 99%
“…Thus for example one could assume µ = constant, P z = P φ = P r , then we can integrate (11) to obtain…”
Section: Discussionmentioning
confidence: 99%
“…which is not bounded from above-solutions with unbounded m T have also been found analytically [18]. We can use mass per unit coordinate length, M 1 (6.12), with no upper bound (see figure 4).…”
Section: Cylinders Of Incompressible Fluid: Analytic Approach and Nummentioning
confidence: 92%
“…On the other hand, it is clear that in the case of a plane source we should not expect φ to behave like an angle coordinate (see also [12] on this point). Therefore , on the basis of all comments above, we are inclined to think (as in [18]) that the σ = 1/2 case corresponds to an infinite plane.…”
Section: Discussionmentioning
confidence: 99%
“…However, as it has been recently emphasized [12], [18], Kretschmann scalar may not be a good measure of the strength of the gravitational field. Instead, those authors suggest that the acceleration of the test particle represents more suitably the intensity of the field.…”
Section: Introductionmentioning
confidence: 97%