Rotating BPS black holes in matter-coupled AdS4 supergravity
Abstrak
Using the general recipe given in arXiv:0804.0009, where all timelike super-symmetric solutions of $ \mathcal{N} = 2 $, D = 4 gauged supergravity coupled to abelian vector multiplets were classified, we construct genuine rotating supersymmetric black holes in AdS4 with nonconstant scalar fields. This is done for the SU(1, 1)/U(1) model with prepotential F = −iX0X1. 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. Moreover, for constant scalars, we generalize (a supersymmetric subclass of) the Plebanski-Demianski solution of cosmological Einstein-Maxwell theory to an arbitrary number of vector multiplets. Remarkably, the latter turns out to be related to the dimensionally reduced gravitational Chern-Simons action.
Topik & Kata Kunci
Penulis (1)
D. Klemm
Akses Cepat
- Tahun Terbit
- 2011
- Bahasa
- en
- Total Sitasi
- 39×
- Sumber Database
- Semantic Scholar
- DOI
- 10.1007/JHEP07(2011)019
- Akses
- Open Access ✓