Modular Constraints on Superconformal Field Theories
Jin-Beom Bae, Sungjay Lee, Jaewon Song
TL;DR
The authors constrain the spectra of ${\mathcal N}=(1,1)$ and ${\mathcal N}=(2,2)$ 2D SCFTs by enforcing NS-sector modular invariance under ${\Gamma}_{\theta}$ and solving a modular bootstrap via semi-definite programming. They obtain both charge-independent and charge-dependent bounds, uncovering pronounced twist-gap features (kinks and plateaus) that align with candidate RCFTs and reveal holomorphic factorization at special central charges ${c}$, all while connecting to AdS$_3$/CFT$_2$ via the weak gravity conjecture. Notably, they identify single-character RCFTs at ${c=9}$ and ${c=33/2}$, relate plateau spectra to free fermion theories, and derive a bound ${\Delta} \le {c}/{8}+O(1)$ for charged non-BPS states, along with charge bounds that imply the existence of light charged states. Their WGC analysis disfavors a ${\Delta}/{Q} \lesssim \sqrt{c}$ scaling and supports a linear ${\Delta}$–${c}$ bound for charged sectors in ${\mathcal N}=(2,2)$ theories, offering quantitative tests of holographic gravity in AdS$_3$.
Abstract
We constrain the spectrum of $\mathcal{N}=(1, 1)$ and $\mathcal{N}=(2, 2)$ superconformal field theories in two-dimensions by requiring the NS-NS sector partition function to be invariant under the $Γ_θ$ congruence subgroup of the full modular group $SL(2, \mathbb{Z})$. We employ semi-definite programming to find constraints on the allowed spectrum of operators with or without $U(1)$ charges. Especially, the upper bounds on the twist gap for the non-current primaries exhibit interesting peaks, kinks, and plateau. We identify a number of candidate rational (S)CFTs realized at the numerical boundaries and find that they are realized as the solutions to modular differential equations associated to $Γ_θ$. Some of the candidate theories have been discussed by Höhn in the context of self-dual extremal vertex operator (super)algebra. We also obtain bounds for the charged operators and study their implications to the weak gravity conjecture in AdS$_3$.
