Orbit space curvature as a source of mass in quantum gauge theory

IF 0.4 Q4 MATHEMATICS, INTERDISCIPLINARY APPLICATIONS Annals of Mathematical Sciences and Applications Pub Date : 2018-09-17 DOI:10.4310/amsa.2019.v4.n2.a3
V. Moncrief, A. Marini, R. Maitra
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引用次数: 4

Abstract

It has long been realized that the natural orbit space for non-abelian Yang-Mills dynamics is a positively curved (infinite dimensional) Riemannian manifold. Expanding on this result I.M. Singer proposed that strict positivity of the corresponding Ricci tensor (computable through zeta function regularization) could play a fundamental role in establishing that the associated Schroedinger operator admits a spectral gap. His argument was based on representing the (regularized) kinetic term in the Schroedinger operator as a Laplace-Beltrami operator on this positively curved orbit space. We revisit Singer's proposal and show how, when the contribution of the Yang-Mills potential energy is taken into account, the role of the original orbit space Ricci tensor is instead played by a Bakry-Emery Ricci tensor computable from the ground state wave functional of the quantum theory. We next review our ongoing Euclidean-signature-semi-classical program for deriving asymptotic expansions for such wave functionals and discuss how, by keeping the dynamical nonlinearities and non-abelian gauge invariances intact at each level of the analysis, our approach surpasses that of conventional perturbation theory for the generation of approximate wave functionals. Though our main focus is on Yang-Mills theory we derive the orbit space curvature for scalar electrodynamics and prove that, whereas the Maxwell factor remains flat, the interaction naturally induces positive curvature in the (charged) scalar factor of the resulting orbit space. This has led us to the conjecture that such orbit space curvature effects could furnish a source of mass for ordinary Klein-Gordon type fields provided the latter are (minimally) coupled to gauge fields, even in the abelian case. Finally we discuss the potential applicability of our Euclidean-signature program to the Wheeler-DeWitt equation of canonical quantum gravity.
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轨道空间曲率在量子规范理论中的质量来源
人们早就认识到,非阿贝尔杨-米尔斯动力学的自然轨道空间是一个正弯曲(无限维)黎曼流形。在此结果的基础上,I.M. Singer提出相应Ricci张量的严格正性(可通过zeta函数正则化计算)可以在确定相关薛定谔算子允许谱间隙方面发挥基本作用。他的论证是基于将薛定谔算符中的(正则化的)动力学项表示为这个正弯曲轨道空间上的拉普拉斯-贝尔特拉米算符。我们重新审视辛格的提议,并展示了当考虑到杨-米尔斯势能的贡献时,原始轨道空间里奇张量的作用是如何由量子理论的基态波泛函可计算的Bakry-Emery里奇张量代替的。接下来,我们将回顾我们正在进行的欧几里得-签名-半经典程序,用于导出此类波泛函的渐近展开,并讨论如何通过在分析的每个层面保持动态非线性和非阿贝尔规范不变性的完整性,我们的方法超越了传统的摄动理论,用于生成近似波泛函。虽然我们的主要焦点是杨-米尔斯理论,但我们推导了标量电动力学的轨道空间曲率,并证明,尽管麦克斯韦因子保持平坦,但相互作用自然地在产生的轨道空间的(带电)标量因子中诱导出正曲率。这使我们猜想,这样的轨道空间曲率效应可以为普通克莱因-戈登型场提供质量来源,只要后者(最低限度地)与规范场耦合,即使在阿贝尔情况下也是如此。最后讨论了欧几里得签名程序对经典量子引力的Wheeler-DeWitt方程的潜在适用性。
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来源期刊
Annals of Mathematical Sciences and Applications
Annals of Mathematical Sciences and Applications MATHEMATICS, INTERDISCIPLINARY APPLICATIONS-
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