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On the planar limit of 3d T ρ σ SU N $$ {\mathrm{T}}_{\rho}^{\sigma}\left[\mathrm{SU}\left(\mathrm{N}\right)\right] $$

dc.contributor.authorCoccia, Lorenzo
dc.contributor.authorUhlemann, Christoph F.
dc.date.accessioned2022-08-10T17:41:05Z
dc.date.available2022-08-10T17:41:05Z
dc.date.issued2021-06-07
dc.identifier.citationJournal of High Energy Physics. 2021 Jun 07;2021(6):38
dc.identifier.urihttps://doi.org/10.1007/JHEP06(2021)038
dc.identifier.urihttps://hdl.handle.net/2027.42/173343en
dc.description.abstractAbstract We discuss a limit of 3d T ρ σ SU N $$ {T}_{\rho}^{\sigma}\left[\mathrm{SU}(N)\right] $$ quiver gauge theories in which the number of nodes is large and the ranks scale quadratically with the length of the quiver. The sphere free energies and topologically twisted indices are obtained using supersymmetric localization. Both scale quartically with the length of the quiver and quadratically with N, with trilogarithm functions depending on the quiver data as coefficients. The IR SCFTs have well-behaved supergravity duals in Type IIB, and the free energies match precisely with holographic results. Previously discussed theories with N2 ln N scaling arise as limiting cases. Each balanced 3d quiver theory is linked to a 5d parent, whose matrix model is related and dominated by the same saddle point, leading to close relations between BPS observables.
dc.titleOn the planar limit of 3d T ρ σ SU N $$ {\mathrm{T}}_{\rho}^{\sigma}\left[\mathrm{SU}\left(\mathrm{N}\right)\right] $$
dc.typeJournal Article
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/173343/1/13130_2021_Article_15893.pdf
dc.identifier.doihttps://dx.doi.org/10.7302/5074
dc.language.rfc3066en
dc.rights.holderThe Author(s)
dc.date.updated2022-08-10T17:41:04Z
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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