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Stable de Sitter Vacua from N=2 Supergravity

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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.

fields

hep-th 1

years

2026 1

verdicts

UNVERDICTED 1

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