Relativistic corrections for two- and three-body flux tube model

dc.creatorBuisseret, F.
dc.creatorSemay, C.
dc.date2007-04-13
dc.date2007-07-09
dc.date.accessioned2026-07-07T10:59:34Z
dc.date.available2026-07-07T10:59:34Z
dc.descriptionWe generalize the relativistic flux tube model for arbitrary two- or three-body systems. The spin-independent and spin-dependent contributions of the flux tube to the total Hamiltonian are computed in perturbation. In particular, we show that the spin-dependent part exhibits a universal spin-orbit form: It does not depend on the nature of the confined particles. The general equations we present, being well-defined for light particles, can thus be applied to usual as well as exotic hadrons such as hybrid mesons and glueballs.
dc.description10 pages; v2 accepted for publication (minor changes)
dc.identifierhttps://arxiv.org/abs/0704.1753
dc.identifierhttp://arxiv.org/abs/0704.1753
dc.identifierPhys.Rev.D76:017501,2007
dc.identifierdoi:10.1103/PhysRevD.76.017501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187443
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRelativistic corrections for two- and three-body flux tube model
dc.typetext

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