2019
DOI: 10.1007/jhep01(2019)199
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Rotating attractors and BPS black holes in AdS4

Abstract: We analyze stationary BPS black hole solutions to 4d N = 2 abelian gauged supergravity. Using an appropriate near horizon ansatz, we construct rotating attractors with magnetic flux realizing a topological twist along the horizon surface, for any theory with a symmetric scalar manifold. An analytic flow to asymptotically locally AdS 4 is presented for a subclass of these near-horizon geometries, and an explicit new example of supersymmetric AdS 4 rotating black hole is discussed in detail. We further note that… Show more

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Cited by 58 publications
(151 citation statements)
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References 127 publications
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“…The first constraint of (4.29) comes from the index-like condition for the partition function without (−1) F while the second constraint implies the topological twist by the magnetic flux for the R-symmetry on S 2 . The above large N Cardy free energy (4.27) statistically accounts for the microstates of magnetically charged or dyonic rotating BPS black holes in mAdS 4 × S 7 [45,74]. As before, this large N free energy gives the correct entropy of the BPS black holes at arbitrary β.…”
Section: The Refined Topologically Twisted Indexmentioning
confidence: 72%
See 1 more Smart Citation
“…The first constraint of (4.29) comes from the index-like condition for the partition function without (−1) F while the second constraint implies the topological twist by the magnetic flux for the R-symmetry on S 2 . The above large N Cardy free energy (4.27) statistically accounts for the microstates of magnetically charged or dyonic rotating BPS black holes in mAdS 4 × S 7 [45,74]. As before, this large N free energy gives the correct entropy of the BPS black holes at arbitrary β.…”
Section: The Refined Topologically Twisted Indexmentioning
confidence: 72%
“…In this subsection, we construct the large N Cardy limit of the refined topologically twisted index from (4.18). This index should statistically account for the microstates of the magnetically charged or dyonic, static [71][72][73] or rotating [74] BPS black holes with the nonvanishing magnetic flux for the gauged R-symmetry in mAdS 4 ×S 7 [14], which is a particular asymptotically locally AdS spacetime [38]. For these black holes, one can freely turn off the electric charges, angular momentum, and magnetic charges for the (non-R) flavor symmetries.…”
Section: The Refined Topologically Twisted Indexmentioning
confidence: 99%
“…There have been many studies regarding rotating magnetically charged black holes that are the natural candidates for the refined topologically twisted index. In particular, there is one recent publication that discusses these issues in detail and contains a comprehensive list of references [64]. A common theme, since the very beginning of the explorations of rotating magnetically charged black holes, is that within the confines of the universal sector described by the action in equation (4.12) spherically symmetric black holes do not exist [59].…”
Section: Rotating Magnetically Charged Ads 4 Black Holesmentioning
confidence: 99%
“…We conclude with discussion and outlook in section 7. Appendix A contains some technical aspects of the relevant N = 2 gauged supergravity and the black hole solutions of [17,21]. Appendix B contains an example of our techniques applied to asymptotically flat black holes in four dimensions.…”
Section: Figure 1 Gluing Gravitational Blocksmentioning
confidence: 99%
“…In order to give a unifying picture it is convenient to use a four-dimensional point of view. All the above mentioned black objects can be dimensionally reduced to give four-dimensional rotating black hole solutions of an N = 2 gauged supergravity coupled to vector multiplets that can be studied using the methods in [17,21]. The relevant gauged supergravity arises as a consistent truncation of type IIB or M-theory and it is completely specified by a prepotential F(X Λ ) and a set of gauging, or Fayet-Iliopoulos parameters, {g Λ , g Λ }.…”
mentioning
confidence: 99%