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Renyi Entropies, the Analytic Bootstrap, and 3D Quantum Gravity at Higher Genus

Matthew Headrick, Alexander Maloney, Eric Perlmutter, Ida G. Zadeh

Abstract

We compute the contribution of the vacuum Virasoro representation to the genus-two partition function of an arbitrary CFT with central charge $c>1$. This is the perturbative pure gravity partition function in three dimensions. We employ a sewing construction, in which the partition function is expressed as a sum of sphere four-point functions of Virasoro vacuum descendants. For this purpose, we develop techniques to efficiently compute correlation functions of holomorphic operators, which by crossing symmetry are determined exactly by a finite number of OPE coefficients; this is an analytic implementation of the conformal bootstrap. Expanding the results in $1/c$, corresponding to the semiclassical bulk gravity expansion, we find that---unlike at genus one---the result does not truncate at finite loop order. Our results also allow us to extend earlier work on multiple-interval Renyi entropies and on the partition function in the separating degeneration limit.

Renyi Entropies, the Analytic Bootstrap, and 3D Quantum Gravity at Higher Genus

Abstract

We compute the contribution of the vacuum Virasoro representation to the genus-two partition function of an arbitrary CFT with central charge . This is the perturbative pure gravity partition function in three dimensions. We employ a sewing construction, in which the partition function is expressed as a sum of sphere four-point functions of Virasoro vacuum descendants. For this purpose, we develop techniques to efficiently compute correlation functions of holomorphic operators, which by crossing symmetry are determined exactly by a finite number of OPE coefficients; this is an analytic implementation of the conformal bootstrap. Expanding the results in , corresponding to the semiclassical bulk gravity expansion, we find that---unlike at genus one---the result does not truncate at finite loop order. Our results also allow us to extend earlier work on multiple-interval Renyi entropies and on the partition function in the separating degeneration limit.

Paper Structure

This paper contains 34 sections, 181 equations, 4 figures.

Figures (4)

  • Figure 1: A depiction of the sewing construction as applied to $Z_{\rm vac}$, the contribution of the Virasoro vacuum representation to a genus-two CFT partition function. The coordinates $p_1$ and $p_2$ represent the widths of the two handles in a Schottky uniformization of the Riemann surface. The handles are replaced by a sum over pairwise operator insertions, where we include all Virasoro descendants of the identity, ${\cal O} \in {\cal H}_{\rm vac}$. This recasts $Z_{\rm vac}$ as a sum of sphere four-point functions, weighted by powers of $p_1$ and $p_2$. The operators ${\cal O}_i$ and ${\cal O}_j$ have holomorphic conformal weights $h_i$ and $h_j$, respectively. A detailed description of the sewing construction is presented in section \ref{['iv']} (see equations \ref{['Z2']} and \ref{['Ch1h2']}).
  • Figure 2: The $n$-sheeted replica surface ${\mathscr R}_{2,n}$, which is the branched covering surface of the plane with two intervals and has genus $n-1$. On each sheet, there is a cycle separating the two intervals called the $A$-cycle, and another cycle encircling the two points $v_1$ and $u_2$, called the $B$-cycle. There are $n-1$ independent cycles of each type.
  • Figure 3: An alternate depiction of the surface ${\mathscr R}_{2,n}$ in figure \ref{['fig-R2n']}. ${\mathscr R}_{2,n}$ can be visualized as two spheres connected by $n$ tubes. The two spheres, one for each interval, are made by cutting small holes around each pair of intervals on all $n$ sheets. The tubes connecting the holes on the two spheres represent the sheets. In this picture, the $A$-cycles wrap the $n$ tubes and the $B$-cycles run through two different tubes.
  • Figure 4: A picture of the sewing approach to computing a genus-two partition function, $Z$. The mechanism was explained in figure \ref{['fig-sewing-vac']}. To compute $Z$ rather than $Z_{\rm vac}$, one simply lets the sum run over all operators in the CFT Hilbert space.