Abstract
We present BPS black hole solutions in a four-dimensional mathcal{N} = 2 supergravity with an abelian dyonic gauging of the universal hypermultiplet moduli space. This supergravity arises as the SU(3)-invariant subsector in the reduction of massive IIA supergravity on a six-sphere. The solutions are supported by non-constant scalar, vector and tensor fields and interpolate between a unique AdS2 × H2 geometry in the near-horizon region and the domain-wall DW4 (four-dimensional) description of the D2-brane at the boundary. Some special solutions with charged AdS4 or non-relativistic scaling behaviours in the ultraviolet are also presented.
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