Abstract

We show that for three dimensional gravity with higher genus boundary conditions, if the theory possesses a sufficiently light scalar, there is a second order phase transition where the scalar field condenses. This three dimensional version of the holographic superconducting phase transition occurs even though the pure gravity solutions are locally AdS3. This is in addition to the first order Hawking-Page-like phase transitions between different locally AdS3 handlebodies. This implies that the Rényi entropies of holographic CFTs will undergo phase transitions as the Rényi parameter is varied, as long as the theory possesses a scalar operator which is lighter than a certain critical dimension. We show that this critical dimension has an elegant mathematical interpretation as the Hausdorff dimension of the limit set of a quotient group of AdS3, and use this to compute it, analytically near the boundary of moduli space and numerically in the interior of moduli space. We compare this to a CFT computation generalizing recent work of Belin, Keller and Zadeh, bounding the critical dimension using higher genus conformal blocks, and find a surprisingly good match.

Highlights

  • Take the boundary of (Euclidean) space-time to be any smooth, two dimensional Riemann surface B

  • We show that for three dimensional gravity with higher genus boundary conditions, if the theory possesses a sufficiently light scalar, there is a second order phase transition where the scalar field condenses

  • This three dimensional version of the holographic superconducting phase transition occurs even though the pure gravity solutions are locally AdS3. This is in addition to the first order Hawking-Page-like phase transitions between different locally AdS3 handlebodies. This implies that the Renyi entropies of holographic CFTs will undergo phase transitions as the Renyi parameter is varied, as long as the theory possesses a scalar operator which is lighter than a certain critical dimension

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Summary

Review of higher genus partition functions in 3D gravity and 2D CFT

We will review the description of higher genus Riemann surfaces, and the construction of solutions to three-dimensional gravity with such boundaries, which can be interpreted as saddle points for the higher genus partition function of a holographic CFT. We describe a class of symmetric surfaces that we will use as examples. We will review the interpretation of these partition functions in terms of Renyi entropies

Moduli spaces and handlebodies
Relationship with Renyi entropies
The phase transition from CFT
The partition function and conformal blocks
Semiclassical global limit of higher genus blocks
Applying the blocks to generalized free fields
The bulk instability
The zero mode and spectral theory
Locally hyperbolic spaces
Divergence of the partition function
When Γ is Fuchsian
McMullen’s algorithm
Analytic results
Numerical results
Full Text
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