2000
DOI: 10.1103/physrevd.62.025019
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Path integral representation for Wilson loops and the non-Abelian Stokes theorem

Abstract: We discuss the derivation of the path integral representation over gauge degrees of freedom for Wilson loops in SU (N ) gauge theory and 4-dimensional Euclidean space-time by using well-known properties of group characters. A discretized form of the path integral is naturally provided by the properties of group characters and does not need any artificial regularization. We show that the path integral over gauge degrees of freedom for Wilson loops derived by Diakonov and Petrov (Phys. Lett. B224 (1989) 131) by… Show more

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Cited by 26 publications
(50 citation statements)
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“…(6.117c) 57 For another choice of h 2 = − ν 2 , the same results are obtained if the following replacement is performed.…”
Section: Explicit Construction For Su(3)supporting
confidence: 66%
See 2 more Smart Citations
“…(6.117c) 57 For another choice of h 2 = − ν 2 , the same results are obtained if the following replacement is performed.…”
Section: Explicit Construction For Su(3)supporting
confidence: 66%
“…Rather, we claim that even in the SU(N) Yang-Mills theory a single magnetic monopole is sufficient to achieve confinement, when quarks belong to the fundamental representation of the color gauge group. In fact, this scenario was originally proposed in [59,60,61] based on a consideration from a non-Abelian Stokes theorem for the Wilson loop operator [55,56,57,58], which is more elaborated in [62,63,64,65] (See [66,67,68,69,70,71,72] for other versions of non-Abelian Stokes theorem). In order to consider confinement of quarks in the specified representation based on the Wilson loop operator, we adopt the color field n(x) taking the value in the Lie algebra of G/H, 14) whereH is a subgroup of G called the maximal stability subgroup which is determined once the highest-weight state of a given representation is chosen.…”
Section: 3)mentioning
confidence: 99%
See 1 more Smart Citation
“…This work was all done using a Newtonian or modified Newtonian approach (by including gravitational radiation reaction in different ways in the calculations), and we note that the thermodynamic details are of little importance for the emission of gravitational waves, since it is concernced primarily with the motion of bulk matter at high densities. More recently, there have been advances in making post-Newtonian calculations of initial conditions (Lombardi, Rasio & Shapiro 1997) and mergers (Faber & Rasio 2000;Faber, Rasio & Manor 2000;Ayal et al 2001), and also in including general relativity (Wilson, Mathews & Marronetti 1996;Baumgarte et al 1997;Oohara & Nakamura 1999;Shibata 1999;Shibata & Uryū 2000;Usui, Uryū & Eriguchi 2000;Gourgoulhon et al 2001).…”
Section: Introduction a N D M O T I Vat I O Nmentioning
confidence: 99%
“…This confirms fully the results obtained in Refs. [2,3] that the evolution operator Z Reg (R 2 , R 1 ) vanishes and the path integral representation of the Wilson loop suggested by Diakonov and Petrov in terms of the evolution operator Z Reg (R 2 , R 1 ) is erroneous. All of these statements are completely applicable to the results discussed by Diakonov and Petrov in their recent manuscript hep-lat/0008004 [4].…”
mentioning
confidence: 99%