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Exact Virasoro Blocks from Wilson Lines and Background-Independent Operators

A. Liam Fitzpatrick, Jared Kaplan, Daliang Li, Junpu Wang

TL;DR

This work provides an exact, bulk-reconstruction-friendly framework in which sl$(2)$ Chern-Simons Wilson lines reproduce Virasoro blocks and OPE blocks in CFT$_2$, enabling background-independent descriptions of AdS$_3$ physics. By formulating Wilson lines as boundary-anchored objects in an infinite-dimensional sl$(2)$ representation, the authors construct Virasoro OPE blocks from Wilson line networks and derive a path-integral representation that automatically yields uniformizing coordinates in arbitrary backgrounds. They perform concrete checks in the large-$c$ and $1/c$ regimes: the vacuum block is computed up to order $1/c^2$, and general Virasoro blocks are obtained at order $1/c$, with explicit kernels $f_a$, $f_b$ and partial $f_c$ that agree with known results and Zamolodchikov recursion. The approach offers a background-independent, non-perturbative handle on bulk gravity in AdS$_3$, with potential implications for black hole information, bulk reconstruction, and the non-perturbative structure of Virasoro blocks, while also highlighting regulatory and computational challenges for higher-order corrections.

Abstract

Aspects of black hole thermodynamics and information loss can be derived as a consequence of Virasoro symmetry. To bolster the connection between Virasoro conformal blocks and AdS$_3$ quantum gravity, we study sl$(2)$ Chern-Simons Wilson line networks and revisit the idea that they compute a variety of CFT$_2$ observables, including Virasoro OPE blocks, exactly. We verify this in the semiclassical large central charge limit and to low orders in a perturbative $1/c$ expansion. Wilson lines connecting the boundary to points in the bulk play a natural role in bulk reconstruction. Because quantum gravity in AdS$_3$ is rigidly fixed by Virasoro symmetry, we argue that sl$(2)$ Wilson lines provide building blocks for background independent bulk reconstruction. In particular, we show explicitly that they automatically compute the uniformizing coordinates appropriate to any background state.

Exact Virasoro Blocks from Wilson Lines and Background-Independent Operators

TL;DR

This work provides an exact, bulk-reconstruction-friendly framework in which sl Chern-Simons Wilson lines reproduce Virasoro blocks and OPE blocks in CFT, enabling background-independent descriptions of AdS physics. By formulating Wilson lines as boundary-anchored objects in an infinite-dimensional sl representation, the authors construct Virasoro OPE blocks from Wilson line networks and derive a path-integral representation that automatically yields uniformizing coordinates in arbitrary backgrounds. They perform concrete checks in the large- and regimes: the vacuum block is computed up to order , and general Virasoro blocks are obtained at order , with explicit kernels , and partial that agree with known results and Zamolodchikov recursion. The approach offers a background-independent, non-perturbative handle on bulk gravity in AdS, with potential implications for black hole information, bulk reconstruction, and the non-perturbative structure of Virasoro blocks, while also highlighting regulatory and computational challenges for higher-order corrections.

Abstract

Aspects of black hole thermodynamics and information loss can be derived as a consequence of Virasoro symmetry. To bolster the connection between Virasoro conformal blocks and AdS quantum gravity, we study sl Chern-Simons Wilson line networks and revisit the idea that they compute a variety of CFT observables, including Virasoro OPE blocks, exactly. We verify this in the semiclassical large central charge limit and to low orders in a perturbative expansion. Wilson lines connecting the boundary to points in the bulk play a natural role in bulk reconstruction. Because quantum gravity in AdS is rigidly fixed by Virasoro symmetry, we argue that sl Wilson lines provide building blocks for background independent bulk reconstruction. In particular, we show explicitly that they automatically compute the uniformizing coordinates appropriate to any background state.

Paper Structure

This paper contains 31 sections, 193 equations, 6 figures.

Figures (6)

  • Figure 1: Left: A sketch of Wilson lines computing a Virasoro OPE block. Middle: By putting together two such OPE blocks, one obtains a Wilson line network computing a Virasoro conformal block. The blue line indicates the non-trivial vacuum expectation value of the product of the OPE blocks. Right: The Virasoro conformal blocks can also be computed by putting the OPE blocks in the appropriate background bra and ket states.
  • Figure 2: This figure shows a single Wilson line $W_h$ ending at two points on the boundary, and a network of three Wilson lines emanating from three boundary points and meeting at a bulk vertex. The vertex must be invariant under the bulk sl$(2)$ gauge group, and so as a function of the internal sl$(2)$ variables $x_i$ it must take the functional form of a conformally invariant 3-point correlator.
  • Figure 3: This figure shows some Wilson lines anchored near the boundary at $y=0$ at various points $z_i$ and pointing into the bulk. The Wilson lines are labelled by an $x_i$ variable transforming in the infinite dimensional representation of sl$(2)$ with primary dimension $h_i$. From the near-boundary behavior we deduce that this obeys the Virasoro Ward identity for a correlator of primary operators with dimensions $h_i$ located at $z_i$.
  • Figure 4: The Hilbert space associated with an empty cylinder consists of the vacuum and its Virasoro descendants. When we include a Wilson line $W_h$, the space of states includes all Virasoro descendants of a dimension $h$ primary state.
  • Figure 5: This figure indicates the contributions to the Virasoro vacuum block at order $\frac{1}{c}$ and $\frac{1}{c^2}$. The Wilson lines appear in black, while the wavy blue lines indicate contractions of stress energy tensors $\langle TT \rangle = \frac{c}{2 z_{ij}^4}$. "Connected" stress tensor correlators begin to contribute at order $\frac{1}{c^3}$.
  • ...and 1 more figures