Auxiliary fields and the flux tube model

[en] 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.

Disciplines :

Physics

Author, co-author :

Buisseret, Fabien

Semay, Claude

Language :

English

Title :

Auxiliary fields and the flux tube model

Publication date :

01 October 2004

Journal title :

Physical Review. D, Particles and Fields

ISSN :

0556-2821

Publisher :

American Physical Society, Lancaster, Panama

Volume :

Pages :

077501 (4 p.)

Peer reviewed :

Peer reviewed

Research unit :

S824 - Physique nucléaire et subnucléaire

Research institute :

R150 - Institut de Recherche sur les Systèmes Complexes

Available on ORBi UMONS :

since 21 December 2010

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Bibliography

D. LaCourse and M. G. Olsson, Phys. Rev. D 39, 2751 (1989).10.1103/PhysRevD.39.2751
C. Semay and B. Silvestre-Brac, Phys. Rev. D 52, 6553 (1995).10.1103/PhysRevD.52.6553
E. L. Gubankova and A. Yu. Dubin, Phys. Lett. B 334, 180 (1994).10.1016/0370-2693(94)90608-4
V. L. Morgunov, A. V. Nefediev, and Yu. A. Simonov, Phys. Lett. B 459, 653 (1999).10.1016/S0370-2693(99)00710-8
T. J. Allen and M. G. Olsson, Phys. Rev. D 68, 054022 (2003).10.1103/PhysRevD.68.054022
C. Semay, B. Silvestre-Brac, and I. M. Narodetskii, Phys. Rev. D 69, 014003 (2004).10.1103/PhysRevD.69.014003
M. G. Olsson and Siniša Veseli, Phys. Rev. D 51, 3578 (1995).10.1103/PhysRevD.51.3578
F. Buisseret and C. Semay, “Lagrange mesh, relativistic flux tube and rotating string” (to be published).