Closed flux tubes and their string description in D=2+1 SU(N) gauge theories

TL;DR

This study uses lattice calculations to analyze confining flux tubes in 2+1 dimensional SU(N) gauge theories, finding strong agreement with the free string Nambu-Goto model and supporting the universality of effective string corrections.

Contribution

It provides the first detailed comparison of flux tube spectra in 2+1 dimensions with the Nambu-Goto string model, confirming universality and identifying the dominant correction terms.

Findings

Energies closely match Nambu-Goto predictions even below critical length.

Supports universality of O(1/l) and O(1/l^3) corrections.

No evidence of non-stringy massive flux tube modes.

Abstract

We carry out lattice calculations of the spectrum of confining flux tubes that wind around a spatial torus of variable length l, in 2+1 dimensions. We compare the energies of the lowest c.30 states to the free string Nambu-Goto model and to recent results on the universal properties of effective string actions. Our most useful calculations are in SU(6) at a small lattice spacing, which we check is very close to the large-N continuum limit. We find that the energies, En(l), are remarkably close to the predictions of the free string Nambu-Goto model, even well below the critical length at which the expansion of the Nambu-Goto energy in powers of 1/l diverges and the series needs to be resummed. Our analysis of the ground state supports the universality of the O(1/l) and the O(1/l^3) corrections to l.sigma, and we find that the deviations from Nambu-Goto at small l prefer a leading correction that is O(1/l^7), consistent with theoretical expectations. We find that the low-lying states that contain a single phonon excitation are also consistent with the leading O(1/l^7) correction dominating down to the smallest values of l. By contrast our analysis of the other light excited states clearly shows that for these states the corrections at smaller l resum to a much smaller effective power. Finally, and in contrast to our recent calculations in D=3+1, we find no evidence for the presence of any non-stringy states that could indicate the excitation of massive flux tube modes.