Stable de Sitter Vacua from N=2 Supergravity

Abstract

We find extrema of the potential of matter couplings to N=2 supergravity that define de Sitter vacua and no tachyonic modes. There are three essential ingredients in our construction: namely non-abelian non-compact gaugings, de Roo-Wagemans rotation angles, and Fayet-Iliopoulos terms.

30 pages, 1 figure; v2: Added reference, and typos corrected. Version to be published in CQG

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