Non-Abelian Strings and the Luscher Term

Details Non-Abelian Strings and the Luscher Term Non-Abelian Strings and the Luscher Term

2007-12-20

arxiv.org/abs/0712.3512v1

Phys.Rev.D77:066008,2008

Physics

High Energy Physics

High Energy Physics - Theory

7 pages, no figures

Scientific paper

10.1103/PhysRevD.77.066008

We calculate the Luscher term for recently suggested non-Abelian flux tubes (strings). The main feature of the non-Abelian strings is the presence of orientational zero modes associated with rotation of their color flux inside a non-Abelian subgroup. The Luscher term is determined by the number of light degrees of freedom on the string wordsheet. Unlike the standard \pi/12 we get N\pi/12 for non-Abelian strings in the U(N) gauge theories. Thus, the Luscher coefficient acquires a dependence on the rank of the gauge group. In the models with non-Abelian strings discussed in the literature there are two distinct scales: the string tension \xi (the string thickness \sim \xi^{-1/2}) and the dynamical scale of strong interactions \Lambda. At weak coupling \xi\gg\Lambda^2. The Luscher term for non-Abelian strings experiences a jump: at \xi^{-1/2}\ll L\ll \Lambda^{-1} it is N\pi/12 while at at L\gg \Lambda^{-1} the orientational moduli are frozen out and the Luscher coefficient approaches its "Luscher" value \pi/12. We raise the question of possible extra (i.e. non-translational) light moduli on the worldsheet of QCD strings at large N.

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