2021
DOI: 10.48550/arxiv.2111.03069
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The joy of factorization at large $N$: five-dimensional indices and AdS black holes

Seyed Morteza Hosseini,
Itamar Yaakov,
Alberto Zaffaroni

Abstract: We discuss the large N factorization properties of five-dimensional supersymmetric partition functions for CFT with a holographic dual. We consider partition functions on manifolds of the form M = M 3 × S 2 , where is an equivariant parameter for rotation. We show that, when M 3 is a squashed three-sphere, the large N partition functions can be obtained by gluing elementary blocks associated with simple physical quantities. The same is true for various observables of the theories on M 3 = Σ g × S 1 , where Σ g… Show more

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Cited by 3 publications
(5 citation statements)
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“…The holographic prediction was verified at large N for certain classes of theories, including Seiberg theories [1] and related quiver theories [2], by explicit field theoretical computation of S 3 b × Σ g partition function in [3]. Similar results for different 5d manifolds have been obtained in the large N limit [4,5] and in Cardy limit [6].…”
Section: Introductionsupporting
confidence: 61%
See 1 more Smart Citation
“…The holographic prediction was verified at large N for certain classes of theories, including Seiberg theories [1] and related quiver theories [2], by explicit field theoretical computation of S 3 b × Σ g partition function in [3]. Similar results for different 5d manifolds have been obtained in the large N limit [4,5] and in Cardy limit [6].…”
Section: Introductionsupporting
confidence: 61%
“…We can follow the approach of extremizing the twisted superpotential first and then evaluating the free energy on those solutions but for the purposes of swiftness, we follow the approach of extremizing the free energy with respect to both the gauge variable ũ and gauge flux m following [6]. From past experiences, we expect the extremum values for ũ to be imaginary so we substitute ũi → iσ i .…”
Section: Su (N ) K + N Fmentioning
confidence: 99%
“…A More details on the AdS 4 × Σ g solutions A.1 Relation with the Lagrangian of [1] Here we make contact between the D = 6 Lagrangian (2.1), that we use in the paper, and the Lagrangian used in [1], given explicitly in [51]. In order to minimise confusion we have relabelled some of the quantities in [51] as follows ϕ 1,2 → φ1,2 , F 3,6 → 1 2 F 3,6 , m → m 1 , (A.1) 16 Again, the recent paper [41] discusses related setups, for compactifications of d = 5 and d = 6 SCFTs on various smooth manifolds, including S 2 ǫ × Σ g and S 2 ǫ1 × S 2 ǫ2 .…”
Section: Discussionmentioning
confidence: 99%
“…For g = 0,(5.38) can also be viewed as the off-shell free energy on S 3 × S 2 ǫ of N = 2 SYM in d = 5. Using this, the form (5.38) has been recently proved in[41] for S 3 b × S 2 ǫ .…”
mentioning
confidence: 87%
“…• The holographic duals of holomorphic blocks were dubbed gravitational blocks [91] and have played a role in a number of follow-ups [92][93][94]. It will be interesting to see how if our modular family of holomorphic blocks can add to their analysis.…”
Section: Summary and Future Directionsmentioning
confidence: 99%