pith. sign in

arxiv: 1807.06200 · v1 · pith:OYZTOK7Knew · submitted 2018-07-17 · ✦ hep-th

Monstrous Product CFTs in the Grand Canonical Ensemble

classification ✦ hep-th
keywords canonicalformulagrandensemblemodularparameterproducttransition
0
0 comments X
read the original abstract

We study symmetric products of the chiral 'Monster' conformal field theory with c=24 in the grand canonical ensemble by introducing a complex parameter \rho, whose imaginary part represents the chemical potential \mu conjugate to the number of copies of the CFT. The grand canonical partition function is given by the DMVV product formula in terms of the multiplicities of the seed CFT. It possesses an O(2,2;\ZZ) symmetry that enhances the familiar SL(2,\ZZ) modular invariance of the canonical ensemble and mixes the modular parameter \tau with the parameter \rho. By exploiting this enhanced modular symmetry and the pole structure of the DMVV product formula we are able to extend the region of validity of Cardy's formula, and explain why it matches the semi-classical Bekenstein-Hawking formula for black holes all the way down to the AdS-scale. We prove that for large c the spectrum contains a universal perturbative sector whose degeneracies obey Hagedorn growth. The transition from Cardy to Hagedorn growth is found to be due to the formation of a Bose-Einstein condensate of ground state CFTs at low temperatures. The grand canonical partition function has an interesting phase structure, which in addition to the standard Hawking-Page transition between low and high temperature, exhibits a wall-crossing transition that exchanges the roles of \tau and \rho.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Holographic pressure and volume for black holes

    hep-th 2026-02 unverdicted novelty 5.0

    Introduces a holographic pressure and volume for static spherically symmetric black holes via quasi-local thermodynamics, showing large black holes become extensive in the large-system limit while small ones do not.