{"title":"Wilson Lines in the Abelian Lattice Higgs Model","authors":"Malin P. Forsström","doi":"10.1007/s00220-024-05128-x","DOIUrl":null,"url":null,"abstract":"<div><p>Lattice gauge theories are lattice approximations of the Yang–Mills theory in physics. The abelian lattice Higgs model is one of the simplest examples of a lattice gauge theory interacting with an external field. In a previous paper (Forsström et al. in Math Phys 4(2):257–329, 2023), we calculated the leading order term of the expected value of Wilson loop observables in the low-temperature regime of the abelian lattice Higgs model on <span>\\({\\mathbb {Z}}^4,\\)</span> with structure group <span>\\(G = {\\mathbb {Z}}_n\\)</span> for some <span>\\(n \\ge 2.\\)</span> In the absence of a Higgs field, these are important observables since they exhibit a phase transition which can be interpreted as distinguishing between regions with and without quark confinement. However, in the presence of a Higgs field, this is no longer the case, and a more relevant family of observables are so-called open Wilson lines. In this paper, we extend and refine the ideas introduced in Forsström et al. (Math Phys 4(2):257–329, 2023) to calculate the leading order term of the expected value of the more general Wilson line observables. Using our main result, we then calculate the leading order term of several natural ratios of expected values and confirm the behavior predicted by physicists.</p></div>","PeriodicalId":522,"journal":{"name":"Communications in Mathematical Physics","volume":"405 11","pages":""},"PeriodicalIF":2.2000,"publicationDate":"2024-11-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00220-024-05128-x.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Communications in Mathematical Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s00220-024-05128-x","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MATHEMATICAL","Score":null,"Total":0}
引用次数: 0
Abstract
Lattice gauge theories are lattice approximations of the Yang–Mills theory in physics. The abelian lattice Higgs model is one of the simplest examples of a lattice gauge theory interacting with an external field. In a previous paper (Forsström et al. in Math Phys 4(2):257–329, 2023), we calculated the leading order term of the expected value of Wilson loop observables in the low-temperature regime of the abelian lattice Higgs model on \({\mathbb {Z}}^4,\) with structure group \(G = {\mathbb {Z}}_n\) for some \(n \ge 2.\) In the absence of a Higgs field, these are important observables since they exhibit a phase transition which can be interpreted as distinguishing between regions with and without quark confinement. However, in the presence of a Higgs field, this is no longer the case, and a more relevant family of observables are so-called open Wilson lines. In this paper, we extend and refine the ideas introduced in Forsström et al. (Math Phys 4(2):257–329, 2023) to calculate the leading order term of the expected value of the more general Wilson line observables. Using our main result, we then calculate the leading order term of several natural ratios of expected values and confirm the behavior predicted by physicists.
格规理论是物理学中杨-米尔斯理论的格近似。无邻晶格希格斯模型是晶格规理论与外部场相互作用的最简单例子之一。在之前的一篇论文(Forsström et al. in Math Phys 4(2):257-329, 2023)中,我们计算了非等边晶格希格斯模型低温机制下威尔逊环观测值的前导阶项,该模型的结构组为\({\mathbb {Z}}^4,\) with structure group \(G = {\mathbb {Z}_n\) for some \(n \ge 2.\在没有希格斯场的情况下,这些都是重要的观测指标,因为它们表现出一种相变,可以被解释为区分有夸克约束和没有夸克约束的区域。然而,在存在希格斯场的情况下,情况就不再是这样了,与之更相关的观测指标系列是所谓的开放式威尔逊线。在本文中,我们扩展并完善了 Forsström 等人(《数学物理》4(2):257-329, 2023)中提出的观点,计算了更一般的威尔逊线观测值的期望值的前导阶项。利用我们的主要结果,我们随后计算了几个预期值自然比率的前导阶项,并证实了物理学家预测的行为。
期刊介绍:
The mission of Communications in Mathematical Physics is to offer a high forum for works which are motivated by the vision and the challenges of modern physics and which at the same time meet the highest mathematical standards.