Selfdual backgrounds in N=2 five-dimensional Chern-Simons Supergravity
arXiv:hep-th/0009066 · doi:10.1016/S0370-2693(01)00098-3
Abstract
We consider five-dimensional S(2,2|N) Chern-Simons supergravity on M_4 * R . By fine-tuning the Kaluza-Klein reduction to make the 4d cosmological constant equal zero, it is shown that selfdual curvatures on M_4 provide exact solutions to the equations of motion if N=2.
Added comments on the Eguchi-Hanson metric as a solution to 5d Chern-Simons supergravity on M4*S1