# BPS black holes from massive IIA on S$^6$

## TL;DR

This paper constructs BPS black hole solutions within a specific four-dimensional supergravity model derived from massive IIA supergravity on a six-sphere, revealing their near-horizon and boundary behaviors.

## Contribution

It introduces new BPS black hole solutions in a gauged supergravity model from massive IIA reduction, including special cases with charged AdS4 and non-relativistic UV behaviors.

## Key findings

- Solutions interpolate between AdS2×H2 and domain-wall geometries.
- Some solutions exhibit charged AdS4 or non-relativistic scaling in the UV.
- Supports non-constant scalar, vector, and tensor fields in black hole configurations.

## 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 $\textrm{AdS}_{2} \,\times\, \textrm{H}^2$ geometry in the near-horizon region and the domain-wall DW$_{4}$ (four-dimensional) description of the D2-brane at the boundary. Some special solutions with charged AdS$_{4}$ or non-relativistic scaling behaviours in the ultraviolet are also presented.