Distinguishing Hybrids from Radial Quarkonia

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dc.creatorClose, Frank E.
dc.creatorPage, Philip R.
dc.date1997-01-31
dc.date1997-04-09
dc.date.accessioned2026-07-07T10:33:28Z
dc.date.available2026-07-07T10:33:28Z
dc.descriptionWe present arguments that reinforce the hybrid interpretation of pi(1800) and we establish that the rho(1450) and the omega(1420) can be interpreted as radial-hybrid mixtures. Some questions for future experiments are raised.
dc.description11 pages, LaTeX, 3 eps figures, uses epsf. Title changed
dc.identifierhttps://arxiv.org/abs/hep-ph/9701425
dc.identifierhttp://arxiv.org/abs/hep-ph/9701425
dc.identifierPhys.Rev.D56:1584-1588,1997
dc.identifierdoi:10.1103/PhysRevD.56.1584
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179117
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDistinguishing Hybrids from Radial Quarkonia
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