论具有扭曲质量的红外线代数

Ahsan Z. Khan, Gregory W. Moore
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引用次数: 0

摘要

红外代数(Algebra of the Infrared \cite{Gaiotto:2015aoa})是一个框架,用于仅利用BPS部门的信息来构建二维中大质量$\mathcal{N}=(2,2)$理论的局部观测值、界面和超对称边界条件类别。由此产生的框架被称为 "基于网络的形式主义"。在本文中,我们开始对基于网络的形式主义进行概括,以包括比(cite{Gaiotto:2015aoa}中讨论的更广泛的一类$\mathcal{N}=(2,2)$量子场论:具有非三维扭曲质量的理论。新的基本要素是在一个固定的真空扇区中存在BPS粒子。在本文中,我们针对允许存在这种BPS粒子的最简单理论类别:具有单一真空和单一扭曲质量的理论,建立了基于网络的形式主义。我们的研究表明,即使在这种简单的环境中,也会出现一些有趣的新现象,包括封闭玻色子的福克空间的出现,以及科斯祖尔对偶代数的自然出现。在数学上,研究具有扭曲质量的理论包括研究由封闭全形一形式定义的朗道-金兹堡模型的 A 型边界条件的 Fukaya-Seidelcategory 。本文勾画了一个基于网络的A型边界条件类别的构造,该类别适用于具有单个莫尔兹零点和单个非三维周期的单形式。我们在一个特别有启发性的例子中明确演示了我们的形式主义。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On the Algebra of the Infrared with Twisted Masses
The Algebra of the Infrared \cite{Gaiotto:2015aoa} is a framework to construct local observables, interfaces, and categories of supersymmetric boundary conditions of massive $\mathcal{N}=(2,2)$ theories in two dimensions by using information only about the BPS sector. The resulting framework is known as the ``web-based formalism.'' In this paper we initiate the generalization of the web-based formalism to include a much wider class of $\mathcal{N}=(2,2)$ quantum field theories than was discussed in \cite{Gaiotto:2015aoa}: theories with non-trivial twisted masses. The essential new ingredient is the presence of BPS particles within a fixed vacuum sector. In this paper we work out the web-based formalism for the simplest class of theories that allow for such BPS particles: theories with a single vacuum and a single twisted mass. We show that even in this simple setting there are interesting new phenomenon including the emergence of Fock spaces of closed solitons and a natural appearance of Koszul dual algebras. Mathematically, studying theories with twisted masses includes studying the Fukaya-Seidel category of A-type boundary conditions for Landau-Ginzburg models defined by a closed holomorphic one-form. This paper sketches a web-based construction for the category of A-type boundary conditions for one-forms with a single Morse zero and a single non-trivial period. We demonstrate our formalism explicitly in a particularly instructive example.
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