2002
DOI: 10.1103/physrevc.65.044619
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Nucleon resonances with double polarization observables of pion photoproduction

Abstract: The role of the nucleon resonances in the double polarization observables of pion photoproduction is investigated by using the resonance parameters predicted by Capstick and Roberts. As an example, we show that the not-well-determined two-star resonance N 3/2 Ϫ (1960) can be examined by performing experiments on beam-recoil polarization at large angles.

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Cited by 10 publications
(10 citation statements)
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References 11 publications
(26 reference statements)
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“…To make progress, we follow the phenomenological procedure of Ref. [49] to define t γN,πN in terms of the empirical γN → πN amplitude and the resonant amplitude constructed from the quark model predictions of Ref. [27,28,29].…”
Section: A Coupled-channel Formalismmentioning
confidence: 99%
See 1 more Smart Citation
“…To make progress, we follow the phenomenological procedure of Ref. [49] to define t γN,πN in terms of the empirical γN → πN amplitude and the resonant amplitude constructed from the quark model predictions of Ref. [27,28,29].…”
Section: A Coupled-channel Formalismmentioning
confidence: 99%
“…where t QM,R πN,γN is the quark model amplitude given explicitly in Ref. [49] and T SAID πN,γN is obtained from the 1995 solution of the SAID [37] analysis. As an alternative, we can replace t QM,R πN,γN by t PDG,R πN,γN which is the γN → N * → πN amplitude defined by the resonance parameters listed by PDG.…”
Section: A Coupled-channel Formalismmentioning
confidence: 99%
“…[8,34,69]. The asymmetries are of great interest in the search of missing resonances which do not show up so clearly in other observables [70]. The formulae which relate the amplitudes with the asymmetries will be presented in forthcoming paragraphs.…”
Section: Differential Cross Sections and Asymmetriesmentioning
confidence: 99%
“…Whatever the origin is for the observed enhancement around 2.2 GeV, it is remarkable that the scaled differential cross section drops by a factor of 4 over a rather small centerof-mass energy range (∼ 0.3 GeV). More experimental work, such as polarization measurements [40], together with an extended SAID model might help to understand the exact nature of the observed enhancement.…”
mentioning
confidence: 99%