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1985
DOI: 10.1007/bf01556612
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Photoproduction of ϕ mesons by linearly polarized photons of energy 20–40 GeV and further evidence for a photoproduced high-massKK enhancement

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Cited by 28 publications
(10 citation statements)
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“…In Fig. 7, we compare our model to the data from the Omega-Photon collaboration [22]. Their data are taken in the energy range E γ = 20 − 40 GeV.…”
Section: Comparison With Datamentioning
confidence: 99%
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“…In Fig. 7, we compare our model to the data from the Omega-Photon collaboration [22]. Their data are taken in the energy range E γ = 20 − 40 GeV.…”
Section: Comparison With Datamentioning
confidence: 99%
“…The model is extrapolated to E γ = 2.8 GeV and 4.7 GeV and compared to the three natural components of the SLAC SDMEs at these energies. In Section IV, we compare the model to the nine ω and ρ 0 SDMEs obtained with a polarized beam at SLAC with E γ = 9.3 GeV, to the nine φ SDMEs from LEPS [21] and Omega-Photon [22], and to the three ω SDMEs obtained with a unpolarized beam from CLAS [23,24], LAMP2 [25] and Cornell [26]. Furthermore, we test the Pomeron normalization for the ω and ρ 0 differential cross sections at E γ > 50 GeV, and the Regge exchange normalization for the ω, ρ 0 and φ differential cross sections at E γ = 9.3 GeV from Ref.…”
Section: Introductionmentioning
confidence: 99%
“…the integrals of the dw ,⊥ /dy over the interval (2). In difference from the notations of [11] W, R and F calculated for the full interval (0,1) of y in this paper the pair production characteristics integrated over the interval (2) are denoted by small letters w, r and f for absorption coefficients, asymmetry and figure of merit, respectively.…”
Section: The Physics and Formulae Of The Methodsmentioning
confidence: 99%
“…with the numbers of pairs n ,⊥ produced in the interval (2). The degree of linear polarization is determined by the formula P=a/r where…”
Section: The Physics and Formulae Of The Methodsmentioning
confidence: 99%
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