Duncan--Frenkel twisted chiral gravity conjecture

Let Γg\Gamma_g be the group associated to gMg\in\mathbb{M}, and let TΓg(1)T^{(-1)}_{\Gamma_g} denote the normalized Rademacher sum attached to Γg\Gamma_g. Duncan--Frenkel conjecture. There exists a monster-indexed family of twisted chiral three-dimensional gravity theories whose genus-one partition functions at

μ=Λ=1/16G\mu=\sqrt{-\Lambda}=1/16G

are given by TΓg(1)(1/τ)T^{(-1)}_{\Gamma_g}(-1/\tau). The conjecture seeks a physical realization of the principal-modulus properties of monstrous moonshine through a family of twisted gravity theories; the specific non-trivial modular fact about these functions is proven by Carnahan, but the existence of the physical theories is not thereby established.

Sources & referencesView supporting material

Primary source

John F. R. Duncan, Michael J. Griffin and Ken Ono, “Moonshine”, arXiv:1411.6571 (2015).

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