Non-supersymmetric Extremal RN-AdS Black Holes in N=2 Gauged Supergravity
Tetsuji Kimura

TL;DR
This paper explores new non-supersymmetric extremal RN-AdS black hole solutions in N=2 gauged supergravity, revealing a novel attractor equation and solutions in specific charge configurations, with implications for understanding AdS black holes.
Contribution
It introduces a new attractor equation for extremal RN-AdS black holes in N=2 gauged supergravity and constructs explicit non-supersymmetric solutions in specific models.
Findings
Derived a new attractor equation for AdS black holes.
Constructed explicit non-supersymmetric solutions in T^3 and STU models.
Showed negative cosmological constant can arise without Fayet-Iliopoulos terms.
Abstract
We investigate extremal Reissner-Nordstrom-AdS black holes in four-dimensional N=2 abelian gauged supergravity. We find a new attractor equation which is not reduced to the one in the asymptotically flat spacetime. Focusing on so-called the T^3-model with a single neutral vector multiplet, we obtain non-supersymmetric extremal Reissner-Nordstrom-AdS black hole solutions with regular event horizon in the D0-D4 and the D2-D6 charge configurations. The negative cosmological constant emerges even without the Fayet-Iliopoulos parameters. Furthermore, we also argue the formal description of the non-supersymmetric black hole solutions of the T^3-model and the STU-model in generic configurations.
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