Universal sectors of two-dimensional Carrollian CFTs
Ankit Aggarwal, Arjun Bagchi, Stephane Detournay, Daniel Grumiller, Max Riegler, Joan Simon
TL;DR
The paper analyzes modular invariance in two-dimensional Carrollian CFTs (CCFT$_2$) by expressing the partition function as a sum over Carrollian characters for induced and highest-weight representations. It identifies six sectors in which the vacuum character dominates in the dual ($S$-dual) channel, revealing universal, gravity-like thermodynamics including a negative specific heat in all vacuum-dominated sectors. A central result is the Schwarzian sector, which mirrors near-extremal dynamics and is holographically realized as an $O$-plane orbifold in flat space, with its microstates and density of states computable via the Carrollian modular S-matrix. The work also contrasts induced vs. highest-weight representations, connects the Schwarzian sector to flat space cosmologies, and situates CCFT$_2$ results within broader contexts such as 3d gravity and Warped CFTs. Overall, it provides a comprehensive framework for universal Carrollian thermodynamics and a holographic dictionary for flat-space holography through six vacuum-dominated sectors and their associated density-of-states structures.
Abstract
We revisit modular invariance in two-dimensional Carrollian conformal field theories from a geometric perspective. Focusing on the characters of the induced and highest-weight representations of the theory, we show that there are regions of parameter space where the vacuum character dominates in the dual channel. We use this property to zoom into different subsectors of the Carrollian theory. One of them is reminiscent of the Schwarzian sector of a relativistic CFT2 and has a flat space holographic interpretation as O-plane orbifold. It exists only for the highest-weight representation. We prove that for all sectors with vacuum dominance in the dual channel, the specific heat is negative, concurrent with the holographic interpretation of the negative specific heat of asymptotically flat spacetimes with horizons.
