2012
DOI: 10.1063/1.3701260
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ω photoproduction at the CBELSA/TAPS experiment

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Cited by 12 publications
(26 citation statements)
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“…The SAPHIR [30], CLAS [32] and A2 [35] Collaborations' data sets are in fairly good agreement overall with each other in the overlapping energy regions but there are some noticeable discrepancies, especially, close to threshold energies, where the SAPHIR and CLAS data are poorer than the A2 data. The CBELSA/TAPS cross section data [33] show a clear discrepancy (which increases with energy and becomes clear for energies above W ∼ 2 GeV or so) with both the SAPHIR and CLAS data. The SAPHIR data seem systematically lower than both the CLAS and CBELSA/TAPS data for backward ω production angles.…”
Section: Numerical Results and Discussionmentioning
confidence: 81%
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“…The SAPHIR [30], CLAS [32] and A2 [35] Collaborations' data sets are in fairly good agreement overall with each other in the overlapping energy regions but there are some noticeable discrepancies, especially, close to threshold energies, where the SAPHIR and CLAS data are poorer than the A2 data. The CBELSA/TAPS cross section data [33] show a clear discrepancy (which increases with energy and becomes clear for energies above W ∼ 2 GeV or so) with both the SAPHIR and CLAS data. The SAPHIR data seem systematically lower than both the CLAS and CBELSA/TAPS data for backward ω production angles.…”
Section: Numerical Results and Discussionmentioning
confidence: 81%
“…We now turn our attention to the analysis of the A2 [35] and CBELSA/TAPS [33] data to see how they influence the extracted resonance content compare to the CLAS data. Recall that there are some inconsistencies in the cross section of both the A2 and CBELSA/TAPS the CBELSA/TAPS data as explained above are shown in Fig.…”
Section: Numerical Results and Discussionmentioning
confidence: 99%
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“…Consequently, as shown in the present work, our rigorous theoretical analyses on the presently available highstatistics and wide-angle-coverage experimental data for the various physical observables will be valuable for a profound understanding for the light-flavor (ρ and ω) and hidden-flavor (J/ψ) vector meson photoproductions [64][65][66][67][68][69][70][71]. Related works will appear elsewhere.…”
Section: Discussionmentioning
confidence: 99%
“…This enables us to investigate meson exchanges of different parities independently, because they do not interfere with each other. More recently, experiments on ω photoproduction are extended to include the reaction at the deuteron target and the data on the reaction off a neutron target from the CBELSA/TAPS and GRAAL Collaborations [9,10] are available for photon energies up to 2 GeV. From the isospin symmetry, therefore, photoproduction of ω off the neutron target could provide further constraint on the different role of the π exchange in the isovector channel.…”
Section: Introductionmentioning
confidence: 99%