Exact rotating charged Kerr-Levi-Civita solutions are constructed by Ernst inversion and by Hassan-Sen charging, with no exterior Ernst zeros or azimuthal closed timelike curves in the Einstein-Maxwell case and a Lambda=0 curvature wall in the heterotic case.
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Charged Kerr--Levi-Civita geometries in Einstein--Maxwell and low-energy heterotic string theory
Exact rotating charged Kerr-Levi-Civita solutions are constructed by Ernst inversion and by Hassan-Sen charging, with no exterior Ernst zeros or azimuthal closed timelike curves in the Einstein-Maxwell case and a Lambda=0 curvature wall in the heterotic case.