Reconclining phi radiative decays with other data for a0(980), fo(980), pi-pi -> KK and pi-pi -> eta-eta

dc.creatorBugg, D. V.
dc.date2006-03-12
dc.date2006-08-27
dc.date.accessioned2026-07-07T10:28:37Z
dc.date.available2026-07-07T10:28:37Z
dc.descriptionData for phi -> gamma (eta-pizero) are analysed using the KK loop model and compared with parameters of a0(980) derived from Crystal Barrel data. The eta-pi mass spectrum agrees closely and the absolute normalisation lies just within errors. However, BES parameters for fo(980) predict a normalisation for phi -> gamma (pizero-pizero) at least a factor 2 lower than is observed. This discrepancy may be eliminated by including constructive interference between fo(980) and sigma. The magnitude required for sigma -> KK is consistent with data on pi-pi -> KK. A dispersion relation analysis by Buttiker, Descotes-Genon and Moussallam of pi-pi -> KK leads to a similar conclusion. Data on pi-pi -> eta-eta also require decays of sigma to eta-eta. Four sets of pi-pi -> KK data all require a small but definite fo(1370) signal.
dc.description21 pages, 11 figures, Small rearrangement of references
dc.identifierhttps://arxiv.org/abs/hep-ex/0603023
dc.identifierhttp://arxiv.org/abs/hep-ex/0603023
dc.identifierEur.Phys.J.C47:45-55,2006
dc.identifierdoi:10.1140/epjc/s2006-02562-2
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177507
dc.subjectHigh Energy Physics - Experiment
dc.titleReconclining phi radiative decays with other data for a0(980), fo(980), pi-pi -> KK and pi-pi -> eta-eta
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