1997
DOI: 10.1016/s0375-9474(96)00408-3
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Photoabsorption on nuclei

Abstract: We calculate the total photoabsorption cross section on nuclei in the energy range from 300 MeV to 1 GeV within the framework of a semi-classical phase space model. Besides medium modifications like Fermi motion and Pauli blocking we focus on the collision broadening of the involved resonances. The resonance contributions to the elementary cross section are fixed by fits to partial wave amplitudes of pion photoproduction. The cross sections for $N \, R \to N \, N$, needed for the calculation of collision broad… Show more

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Cited by 61 publications
(86 citation statements)
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References 25 publications
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“…We do not expect any major change in our results due to these effects. As is pointed out in [47,48,49], the medium correction effects on widths of the s-and p-wave resonances, which make the dominant contribution to the cross sections being investigated here, are not substantial. On the other hand, any medium modification in the width of the d-wave resonance is unlikely to alter our results as their contributions to the cross sections are negligible [46].…”
Section: Calculations Of the Tnm Amplitudesmentioning
confidence: 70%
“…We do not expect any major change in our results due to these effects. As is pointed out in [47,48,49], the medium correction effects on widths of the s-and p-wave resonances, which make the dominant contribution to the cross sections being investigated here, are not substantial. On the other hand, any medium modification in the width of the d-wave resonance is unlikely to alter our results as their contributions to the cross sections are negligible [46].…”
Section: Calculations Of the Tnm Amplitudesmentioning
confidence: 70%
“…To obtain correction (3) at the resonance region (W 2 ≤ 4GeV 2 ) we use the Breit-Wigner parameterization for the photoabsorption cross sections in (12), (13), suggested in [20,21,22,23,24,25,26]. There are many baryon resonances that give contribution to photon absorption cross sections.…”
mentioning
confidence: 99%
“…We take into account only five important resonances: P 33 (1232), S 11 (1535), D 13 (1520), P 11 (1440), F 15 (1680). Considering the one-pion decay channel of the resonances, the absorption cross sections σ 1/2 and σ 3/2 may be written as follows [23,27]:…”
mentioning
confidence: 99%
“…To obtain correction (8) at the resonance region (W 2 ≤ 4GeV 2 ) we use the Breit-Wigner parameterization for the photoabsorption cross sections in (18), (19), suggested in [30][31][32][33][34][35][36]. There are many baryon resonances that give contribution to photon absorption cross sections.…”
Section: B Resonance Regionmentioning
confidence: 99%
“…We take into account only five most important resonances: P 33 (1232), S 11 (1535), D 13 (1520), P 11 (1440), F 15 (1680). Considering the one-pion decay channel of the resonances, the absorption cross sections σ 1/2 and σ 3/2 may be written as follows [33,37]:…”
Section: B Resonance Regionmentioning
confidence: 99%