1979
DOI: 10.1103/physrevc.19.455
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Photopion production in the Fermi-gas model

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Cited by 11 publications
(6 citation statements)
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“…[28,41] in the case of pion photoproduction, Fermi motion can be approximated by choosing κ = 1. This approximation can reproduce the exact cross section to within an accuracy of 7% [42]. Figure 7 compares the cross sections calculated in the two approximations with the exact calculation.…”
Section: Resultsmentioning
confidence: 87%
“…[28,41] in the case of pion photoproduction, Fermi motion can be approximated by choosing κ = 1. This approximation can reproduce the exact cross section to within an accuracy of 7% [42]. Figure 7 compares the cross sections calculated in the two approximations with the exact calculation.…”
Section: Resultsmentioning
confidence: 87%
“…From this study we have predicted the existence of a quenching of 17% of the nucleon polarizability in the nuclear medium due to the Pauli blocking effects. This has been investigated by McDonald et al [20]. It is nevertheless detectable using dispersion relations for the real part of the forward Compton amplitude.…”
Section: Resultsmentioning
confidence: 95%
“…The quantity ~u is given by the dispersive integral c~:v=~ ~ ~f-aco (20) where aN(co) is the total nucleon photoabsorption cross section. The isobar is expected to affect mostly the magnetic polarizability.…”
Section: The Photon Scattering Amplitudementioning
confidence: 99%
“…However this is not possible because the Pauli blocking itself is aected by the existence of the . It is indeed known that the modication of the pion propagation in the nuclear medium, due to the virtual -hole excitations, makes the Pauli blocking less eective [7]. It is thus not possible to disentangle the in the pion photoproduction region.…”
Section: Dispersion Relations and Compton Amplitudementioning
confidence: 99%