Supersymmetric phases of 4d N = 4 SYM at large N

TY - JOUR

T1 - Supersymmetric phases of 4d N = 4 SYM at large N

AU - Cabo-Bizet, Alejandro

AU - Murthy, Sameer

PY - 2020/9/29

Y1 - 2020/9/29

N2 - We find a family of complex saddle-points at large N of the matrix model for the superconformal index of SU(N) N = 4 super Yang-Mills theory on S3× S1 with one chemical potential τ. The saddle-point configurations are labelled by points (m, n) on the lattice Λτ = ℤτ + ℤ with gcd(m, n) = 1. The eigenvalues at a given saddle are uniformly distributed along a string winding (m, n) times along the (A, B) cycles of the torus ℂ/Λτ. The action of the matrix model extended to the torus is closely related to the Bloch-Wigner elliptic dilogarithm, and the related Bloch formula allows us to calculate the action at the saddle-points in terms of real-analytic Eisenstein series. The actions of (0, 1) and (1, 0) agree with that of pure AdS5 and the supersymmetric AdS5 black hole, respectively. The black hole saddle dominates the canonical ensemble when τ is close to the origin, and there are new saddles that dominate when τ approaches rational points. The extension of the action in terms of modular forms leads to a simple treatment of the Cardy-like limit τ → 0.

AB - We find a family of complex saddle-points at large N of the matrix model for the superconformal index of SU(N) N = 4 super Yang-Mills theory on S3× S1 with one chemical potential τ. The saddle-point configurations are labelled by points (m, n) on the lattice Λτ = ℤτ + ℤ with gcd(m, n) = 1. The eigenvalues at a given saddle are uniformly distributed along a string winding (m, n) times along the (A, B) cycles of the torus ℂ/Λτ. The action of the matrix model extended to the torus is closely related to the Bloch-Wigner elliptic dilogarithm, and the related Bloch formula allows us to calculate the action at the saddle-points in terms of real-analytic Eisenstein series. The actions of (0, 1) and (1, 0) agree with that of pure AdS5 and the supersymmetric AdS5 black hole, respectively. The black hole saddle dominates the canonical ensemble when τ is close to the origin, and there are new saddles that dominate when τ approaches rational points. The extension of the action in terms of modular forms leads to a simple treatment of the Cardy-like limit τ → 0.

KW - AdS-CFT Correspondence

KW - Black Holes in String Theory

KW - Supersymmetric Gauge Theory

UR - http://www.scopus.com/inward/record.url?scp=85091733995&partnerID=8YFLogxK

U2 - 10.1007/JHEP09(2020)184

DO - 10.1007/JHEP09(2020)184

M3 - Article

AN - SCOPUS:85091733995

SN - 1126-6708

VL - 2020

SP - 1

EP - 55

JO - Journal of High Energy Physics

JF - Journal of High Energy Physics

IS - 9

M1 - 184

ER -