Auxiliary fields and the flux tube model
High Energy Physics - Phenomenology
2010-11-19 v1
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.
Keywords
Cite
@article{arxiv.hep-ph/0406216,
title = {Auxiliary fields and the flux tube model},
author = {Fabien Buisseret and Claude Semay},
journal= {arXiv preprint arXiv:hep-ph/0406216},
year = {2010}
}
Comments
No table, No figure