Following Black Hole States

Abstract

We study N=4\mathcal{N}=4 SYM at non-integer number of colours. By varying NN we can continuously follow states all the way from N=∞N=\infty where integrability reigns to finite NN where quantum gravity effects dominate. As an application we consider classically 1/161/16 BPS states. Quantum mechanically, these states are generically non-supersymmetric but some special states -- at special values of NN -- become super-symmetric at the quantum level as well. They are the so-called quantum black hole states studied recently using cohomology. We write down the form of the lightest BH state at N=2N=2 -- and follow it in NN, both at weak coupling and -- more speculatively -- at strong coupling as well. At weak coupling this state has protected dimension Ξ”=19/2\Delta=19/2 at N=2N=2 and becomes a triple trace made out of Konishi and two light BPS operators at infinite NN with Ξ”=19/2+12Ξ»+…\Delta=19/2+12\lambda+\dots. At strong coupling we suspect it becomes a quadruple trace with dimension Δ≃19/2+integer\Delta \simeq 19/2+\text{integer}.Comment: 7+8 pages, 20 footnote

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