Pole versus Breit-Wigner resonance description of the orbitally excited baryons

dc.contributorVirginia Techen
dc.contributor.authorWorkman, Ronald L.en
dc.contributor.departmentPhysicsen
dc.date.accessed2013-12-11en
dc.date.accessioned2013-12-18T19:26:51Zen
dc.date.available2013-12-18T19:26:51Zen
dc.date.issued1999-06en
dc.description.abstractWe consider the masses used in recent studies involving the nonstrange sector of the l = 1 baryons. The use of T-matrix and K-matrix poles versus the conventional Breit-Wigner masses is discussed within the context of a large-N-c fitting scheme. [S0556-2813(99)01206-6].en
dc.identifier.citationWorkman, R., Jun 1999. “Pole versus Breit-Wigner resonance description of the orbitally excited baryons,” PHYSICAL REVIEW C 59(6): 3441-3443. DOI: 10.1103/PhysRevC.59.3441en
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.59.3441en
dc.identifier.issn0556-2813en
dc.identifier.urihttp://hdl.handle.net/10919/24728en
dc.identifier.urlhttp://prc.aps.org/pdf/PRC/v59/i6/p3441_1en
dc.language.isoen_USen
dc.publisherAmerican Physical Societyen
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectlarge n-cen
dc.subjectl=1 baryonsen
dc.subjectquark-modelen
dc.subjectphotoproductionen
dc.subjectmassesen
dc.subjectbosonen
dc.subjectqcden
dc.subjectPhysicsen
dc.titlePole versus Breit-Wigner resonance description of the orbitally excited baryonsen
dc.title.serialPhysical Review Cen
dc.typeArticle - Refereeden

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