2021
DOI: 10.1007/jhep04(2021)053
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Exact holographic RG flows in extended SUGRA

Abstract: We present a family of exact planar hairy neutral black hole solutions in extended supergravity with Fayet-Iliopoulos (FI) terms. We consider a model where the magnetic part of FI sector vanishes and obtain the superpotential at finite temperature in analytic form. Then, we discuss the thermodynamics and some holographic properties of these solutions. We regularize the action by two different methods, one with gravitational and scalar counterterms and the other using the thermal superpotential as a counterterm… Show more

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Cited by 12 publications
(14 citation statements)
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References 91 publications
(121 reference statements)
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“…The simplicity of the susy AdS soliton make us conjecture that these 1/2 BPS solutions can be generalized to have different charges by the introduction of running scalars in D = 4 and D = 5 gauged supergravity [23,[37][38][39]. Furthermore, we believe that this susy AdS soliton should also be part of the spectrum of any gauged supergravity in any dimension that contains a consistent supersymmetric truncation with a U(1) gauge field.…”
Section: Discussionmentioning
confidence: 89%
“…The simplicity of the susy AdS soliton make us conjecture that these 1/2 BPS solutions can be generalized to have different charges by the introduction of running scalars in D = 4 and D = 5 gauged supergravity [23,[37][38][39]. Furthermore, we believe that this susy AdS soliton should also be part of the spectrum of any gauged supergravity in any dimension that contains a consistent supersymmetric truncation with a U(1) gauge field.…”
Section: Discussionmentioning
confidence: 89%
“…In this case, we set ϕ 1 = ϕ 3 = 0. The STU model then reduces to the n = 1 model, coinciding with our (57). The Duff-Liu configuration can be recovered from our solution provided either the magnetic or the electric charges are set to zero.…”
Section: Duff-liumentioning
confidence: 55%
“…Scalar self-interactions could be relevant for dynamic and thermodynamic stability of the configuration: naively, we can imagine the condition for the existence of hairy solutions as if the self-interaction of the scalar and the gravitational interaction were to combine such that the near-horizon hair did not collapse into the black hole, while the far-region hair did not escape to infinity 3. These new solutions generalize the uncharged configurations of[47,51,56,57].…”
mentioning
confidence: 99%
“…which corresponds to AdS invariant boundary conditions [4,41], namely a triple trace deformation in the boundary theory. Hence, the boundary conformal symmetry is preserved and the black hole mass can be extracted from the asymptotic expansion of the spacetime [4,11,32,38,42,43]. The expansion of metric (4.1) explicitly reads:…”
Section: Jhep11(2021)116mentioning
confidence: 99%
“…1 Static hairy single-scalar black holes within these models were recently constructed and studied in [4,11,17]. In the BPS limit [4], such solutions are related to the class of black holes considered in [18][19][20][21][22][23][24][25][26][27][28][29][30][31][32]. Hairy black hole solutions in higher dimensions were considered in [33], generalizing those found in [34].…”
Section: Introductionmentioning
confidence: 99%