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Abstract
We consider the rotating non-extremal black hole of N=2 D=4 STU supergravity carrying three magnetic charges and one electric charge. We show that its subtracted geometry is obtained by applying a specific SO(4,4) Harrison transformation on the black hole. As previously noted, the resulting subtracted geometry is a solution of the N=2 S=T=U supergravity.
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1 Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Golm, Germany (GRID:grid.450243.4) (ISNI:0000000107904262)




