Abstract:Zipoy used spheroidal coordinates to construct a family of static axisymmetric gravitational fields included in Weyl's class. We calculate the mass moment source for the dipole solution using techniques previously developed for magnetic and angular momentum densities and compare it with the Newtonian analog studied by Bonnor and Sackfield.
“…Let us consider the ZV solution [9] in Weyl coordinates (for a discussion on Zipoy-Voorhees solution see [10]), with the line element (2) and the metric functions given by:…”
Starting with a Zipoy-Voorhees line element we construct and study the three parameter family of solutions describing a deformed black string with arbitrary tension.
“…Let us consider the ZV solution [9] in Weyl coordinates (for a discussion on Zipoy-Voorhees solution see [10]), with the line element (2) and the metric functions given by:…”
Starting with a Zipoy-Voorhees line element we construct and study the three parameter family of solutions describing a deformed black string with arbitrary tension.
“…After the fashion of [3], [6], [7], an asymptotically cartesian function Z will be introduced and will be taken to satisfy the same differential equation as V :…”
In this lecture a new formalism for constructing electromagnetic surface sources for static axisymmetric electrovacs is presented. The electrostatic and magnetostatic sources are derived from the discontinuities of the scalar potentials. This formalism allows the inclusion of two kinds of dipole sources: Sheets of dipoles and the dipole moment of a distribution of monopoles. It is a generalization of a previous formalism in order to cope with asymptotically monopolar electric fields.
“…Since all known diagonal cylindrical perfect fluid models ( [11], [12], [13], [14]) with regular curvature invariants have already been shown to be geodesically complete [4], we shall only concern about nondiagonal ones. To our knowledge there are just two and both can be derived from Einstein spacetimes using the Wainwright-Ince-Marshman generation algorithm for stiff perfect fluids [15].…”
Section: Completeness Of Several Cylindrical Modelsmentioning
confidence: 99%
“…[1], [2] and references therein) in order to determine whether a spacetime is singular. But on the contrary theorems that provide large families of nonsingular spacetimes are not very usual [3], [4] and in principle the proof of geodesic completeness involves cumbersome calculations [5].…”
Section: Introductionmentioning
confidence: 99%
“…Our aim will be the generalization of the theorem on diagonal orthogonally transitive cylindrical spacetimes in [4] to nondiagonal models and thereby comprise all known nonsingular cylindrical perfect fluid spacetimes in the literature.…”
In this paper a theorem is derived in order to provide a wide sufficient condition for an orthogonally transitive cylindrical spacetime to be singularity-free. The applicability of the theorem is tested on examples provided by the literature that are known to have regular curvature invariants.
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