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- W2022956811 abstract "In a stationary axisymmetric vacuum gravitational field, the conformal structure of the 3-space is determined by the symmetric, trace free and divergence-less tensor Yir. Using the Killing vector Ki of the axisymmetry, the conformal potential U can be defined by U,i = eijkKjYkrKr. Conversely, the tensor Yik is given algebraically in terms of the gradient U,i of the conformal potential. An attempt is made here to re-formulate the field equations Rλμ = 0 in terms of the conformal potential. Introducing the Ernst potential as a complex coordinate, the cylindrical radius can be eliminated from the field equations." @default.
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- W2022956811 date "1986-01-01" @default.
- W2022956811 modified "2023-09-25" @default.
- W2022956811 title "The conformal potential of the stationary axisymmetric vacuum" @default.
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- W2022956811 doi "https://doi.org/10.1002/asna.2113070522" @default.
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