Auxiliary fields and the flux tube model

Abstract

It is possible to eliminate exactly all the auxiliary fields (einbein fields) appearing in the rotating string Hamiltonian to obtain the classical equations of motion of the relativistic flux tube model. A clear interpretation can then be done for the characteristic variables of the rotating string model.

No table, No figure

References in corpus (2)

• Auxiliary fields and hadron dynamics
• Reduction of the QCD string to a time component vector potential

Cited by in corpus (12)

• On two- and three-body descriptions of hybrid mesons
• Bottomonium spectrum in the relativistic flux tube model
• Baryonic mass formula in large $N_c$ QCD versus quark model
• Meson and glueball spectra with the relativistic flux tube model
• Casimir scaling, glueballs and hybrid gluelumps
• Hybrid mesons and auxiliary fields
• Lagrange mesh, relativistic flux tube, and rotating string
• Semirelativistic potential model for three-gluon glueballs
• Semirelativistic potential model for low-lying three-gluon glueballs
• Quark self-energy and relativistic flux tube model
• Retardation effects in the rotating string model
• String deformations induced by retardation effects