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Exact solutions of (n+1)-dimensional Yang-Mills equations in curved space-time

机译:弯曲时空中(n + 1)维Yang-Mills方程的精确解

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In the context of a semiclassical approach where vectorial gauge fields can be considered as classical fields, we obtain exact static solutions of the SU(N) Yang-Mills equations in an (n+. 1)-dimensional curved space-time, for the cases n=1, 2, 3. As an application of the results obtained for the case n=3, we consider the solutions for the anti-de Sitter and Schwarzschild metrics. We show that these solutions have a confining behavior and can be considered as a first step in the study of the corrections of the spectra of quarkonia in a curved background. Since the solutions that we find in this work are valid also for the group U(1), the case n=2 is a description of the (2. +. 1) electrodynamics in the presence of a point charge. For this case, the solution has a confining behavior and can be considered as an application of the planar electrodynamics in a curved space-time. Finally we find that the solution for the case n=1 is invariant under a parity transformation and has the form of a linear confining solution.
机译:在将矢量规范场视为经典场的半经典方法的情况下,对于这种情况,我们可以在(n + 1。)维弯曲时空中获得SU(N)Yang-Mills方程的精确静态解。 n = 1,2,3。作为在n = 3情况下获得的结果的应用,我们考虑了anti-de Sitter和Schwarzschild度量的解决方案。我们表明,这些解决方案具有局限性,可以被认为是弯曲背景中夸克尼亚光谱校正研究的第一步。由于我们在这项工作中找到的解对于U(1)组也有效,因此n = 2的情况是对存在点电荷的(2. +。1)电动力学的描述。对于这种情况,该解决方案具有约束行为,可以视为在弯曲时空中应用平面电动力学。最终,我们发现对于n = 1的情况,在奇偶校验变换下的解是不变的,并且具有线性约束解的形式。

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