The N=1* Theories on R^{1+2} X S^1 with Twisted Boundary Conditions
Seok Kim, Ki-Myeong Lee, Ho-Ung Yee, Piljin Yi
TL;DR
The paper studies ${\rm N}=1^{*}$ theories compactified on ${\bf R}^{1+2}\times S^1$ with twisted boundary conditions, classifying the twists by twisted affine Lie algebras ${\frak G}^{(L)}$ and showing that the low-energy dynamics are governed by a holomorphic superpotential linked to elliptic Calogero-Moser models. By combining monopole-instanton sums, Weyl symmetry, 3D reductions, and a crucial ${\rm SL}(2,\mathbb{Z})$ modular constraint (supported by M-theory realizations), the authors derive exact twisted superpotentials. They further demonstrate universality of the glueball sector via a dual transformation, showing the Veneziano–Yankielowicz glueball potential is twist-independent to several orders and that twist-induced differences reside only in the irreducible ${\cal W}({\boldsymbol{X}})$, not in ${\cal W}(S)$. The results establish a deep link between nonperturbative dynamics in twisted compactifications and integrable models, with implications for dualities and for generalizations to other dimensions and representations.
Abstract
We explore the N=1* theories compactified on a circle with twisted boundary conditions. The gauge algebra of these theories are the so-called twisted affine Lie algebra. We propose the exact superpotentials by guessing the sum of all monopole-instanton contributions and also by requiring SL(2,Z) modular properties. The latter is inherited from the N=4 theory, which will be justified in the M theory setting. Interestingly all twisted theories possess full SL(2,Z) invariance, even though none of them are simply-laced. We further notice that these superpotentials are associated with certain integrable models widely known as elliptic Calogero-Moser models. Finally, we argue that the glueball superpotential must be independent of the compactification radius, and thus of the twisting, and confirm this by expanding it in terms of glueball superfield in weak coupling expansion.
