Symplectically invariant flow equations for N=2, D=4 gauged supergravity with hypermultiplets

TL;DR

This paper derives symplectically invariant flow equations for N=2, D=4 gauged supergravity with hypermultiplets, providing a unified framework for BPS and non-BPS black hole solutions and their attractor behavior.

Contribution

It introduces a symplectically covariant formulation of flow equations in gauged supergravity, extending previous work to include magnetic gaugings and non-BPS solutions.

Findings

Derived first-order flow equations from Hamilton-Jacobi formalism.

Extended flow equations to include magnetic gaugings.

Obtained attractor equations for extremal black holes.

Abstract

We consider N=2 supergravity in four dimensions, coupled to an arbitrary number of vector- and hypermultiplets, where abelian isometries of the quaternionic hyperscalar target manifold are gauged. Using a static and spherically or hyperbolically symmetric ansatz for the fields, a one-dimensional effective action is derived whose variation yields all the equations of motion. By imposing a sort of Dirac charge quantization condition, one can express the complete scalar potential in terms of a superpotential and write the action as a sum of squares. This leads to first-order flow equations, that imply the second-order equations of motion. The first-order flow turns out to be driven by Hamilton's characteristic function in the Hamilton-Jacobi formalism, and contains among other contributions the superpotential of the scalars. We then include also magnetic gaugings and generalize the flow equations to a symplectically covariant form. Moreover, by rotating the charges in an appropriate way, an alternative set of non-BPS first-order equations is obtained that corresponds to a different squaring of the action. Finally, we use our results to derive the attractor equations for near-horizon geometries of extremal black holes.