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
We present the whole set of equations with regularity and matching conditions required for the description of physically meaningful static cylindrically symmmetric distributions of matter, smoothly matched to Levi-Civita vacuum spacetime. It is shown that the conformally flat solution with equal principal stresses represents an incompressible fluid. It is also proved that any conformally flat cylindrically symmetric static source cannot be matched through Darmois conditions to the Levi-Civita spacetime. Further evidence is given that when the Newtonian mass per unit length reaches 1/2 the spacetime has plane
We present the whole set of equations with regularity and matching conditions required for the description of physically meaningful static cylindrically symmmetric distributions of matter, smoothly matched to Levi-Civita vacuum spacetime. It is shown that the conformally flat solution with equal principal stresses represents an incompressible fluid. It is also proved that any conformally flat cylindrically symmetric static source cannot be matched through Darmois conditions to the Levi-Civita spacetime. Further evidence is given that when the Newtonian mass per unit length reaches 1/2 the spacetime has plane
“…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
Abstract. The global properties of static perfect-fluid cylinders and their external Levi-Civita fields are studied both analytically and numerically. The existence and uniqueness of global solutions is demonstrated for a fairly general equation of state of the fluid. In the case of a fluid admitting a non-vanishing density for zero pressure, it is shown that the cylinder's radius has to be finite. For incompressible fluid, the field equations are solved analytically for nearly Newtonian cylinders and numerically in fully relativistic situations. Various physical quantities such as proper and circumferential radii, external conicity parameter and masses per unit proper/coordinate length are exhibited graphically.
“…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.…”
The physical meaning of the Levi-Civita spacetime, for some "critical" values of the parameter σ, is discussed in the light of gedanken experiments performed with gyroscopes circumventing the axis of symmetry. The fact that σ = 1/2 corresponds to flat space described from the point of view of an accelerated frame of reference, led us to incorporate the C-metric into discussion. The interpretation of φ as an angle coordinate for any value of σ, appears to be at the origin of difficulties.
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