In the Carter-projective sector of stationary axisymmetric spacetimes, the diagonal Einstein equations reduce to a single sourced master equation for structure functions Delta and Y, with algebraic compatibility conditions on sources.
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A master equation for Carter-separable stationary axisymmetric spacetimes and compatible sources
In the Carter-projective sector of stationary axisymmetric spacetimes, the diagonal Einstein equations reduce to a single sourced master equation for structure functions Delta and Y, with algebraic compatibility conditions on sources.