Some Properties of a New Solution of the Ernst Equation

Details Some Properties of a New Solution of the Ernst Equation Some Properties of a New Solution of the Ernst Equation

2001-09-25

arxiv.org/abs/gr-qc/0109086v1

Class.Quant.Grav.19:2157-2170,2002

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

17 pages, LaTeX, 10 EPS figures, uses graficx.sty

Scientific paper

10.1088/0264-9381/19/8/307

From a particularly simple solution of the Ernst equation, we build a solution of the vacuum stationary axisymmetric Einstein equations depending on three parameters. The parameters are associated to the total mass of the source and its angular momentum. The third parameter produces a topological deformation of the ergosphere making it a two-sheet surface, and for some of its values forbids the Penrose process.

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