Duncan--Frenkel twisted chiral gravity conjecture

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Let Γg\Gamma_g be the group associated to g∈Mg\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.

References

Primary source

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

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