Some errors were discovered [1] in the computer code on which the calculations presented in this paper were based. This leads to changes in Figs. 2-7 and to modifications to some of the conclusions of the paper. The corrected figures are shown below; the captions are the same as for the original fig
Relativistic calculations for incoherent photoproduction of η mesons
✍ Scribed by I.R. Blokland; H.S. Sherif
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 165 KB
- Volume
- 694
- Category
- Article
- ISSN
- 0375-9474
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✦ Synopsis
We develop a relativistic model for incoherent η-photoproduction on nuclei. The elementary process is described using an effective Lagrangian containing photons, nucleons, the S 11 (1535) and D 13 (1520) nucleon resonances, and ρ, ω and η mesons. The nucleon and η wave functions are obtained from relativistic wave equations. Final-state interactions of the outgoing particles are included via optical potentials. The effects of these interactions are found to be large and lead to reduced cross sections.The incoherent cross sections for isovector transitions are much larger than those for isoscalar ones. The dominant contributions are those from the S 11 and D 13 resonances. We find important interference effects between the contributions of these two resonances. We give some detailed calculations for the cross sections for incoherent η-photoproduction on 12 C. We find that the incoherent cross section for a subset of states in the excitation energy region below 17 MeV are significantly larger than those of the coherent process. These cross sections may thus be accessible experimentally.
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