Rotating BPS black holes in matter-coupled AdS(4) supergravity

Understand

Using the general recipe given in arXiv:0804.0009, where all timelike supersymmetric solutions of N=2, D=4 gauged supergravity coupled to abelian vector multiplets were classified, we construct genuine rotating supersymmetric black holes in AdS(4) with nonconstant scalar fields.

• This is done for the SU(1,1)/U(1) model with prepotential F=-iX^0X^1.
• In the static case, the black holes are uplifted to eleven dimensions, and generalize the solution found in hep-th/0105250 corresponding to membranes wrapping holomorphic curves in a Calabi-Yau five-fold.
• The constructed rotating black holes preserve one quarter of the supersymmetry, whereas their near-horizon geometry is one half BPS.