Conformastationary disk-haloes in Einstein-Maxwell gravity

Abstract

An exact solution of the Einstein-Maxwell field equations for a conformastationary metric with magnetized disk-haloes sources is worked out in full. The characterization of the nature of the energy momentum tensor of the source is discussed. All the expressions are presented in terms of a solution of the Laplace's equation. A "generalization" of the Kuzmin solution of the Laplace's equations is used as a particular example. The solution obtained is asymptotically flat in general and turns out to be free of singularities. All the relevant quantities show a reasonable physical behaviour.

References in corpus (5)

• Dissipative collapse of axially symmetric, general relativistic, sources: A general framework and some applications
• Disc sources for Conformastationary metrics
• Conformastatic disk-haloes in Einstein-Maxwell gravity
• Possible features of galactic halo with electric field and observational constraints
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Cited by in corpus (5)

• Models of spherical shells as sources of Majumdar-Papapetrou type spacetimes
• Self-gravitating razor-thin disks around black holes via multi-hole seeds
• General Relativistic Razor-Thin Disks with Magnetically Polarized Matter
• Test particles in a magnetized conformastatic spacetime
• Analytical models of finite thin disks in a magnetic field