1985
DOI: 10.1016/0370-1573(85)90145-0
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Photonuclear reaction cross sections for 12C, 14N and 16O

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Cited by 69 publications
(32 citation statements)
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“…We used the following data to get charge changing photo cross sections av for 160: a) 10-30 MeV Photo cross sections for 160 for the emission of one proton and one neutron (7, np), for the emission of at least one proton and no neutron (?, p+ X) and for the emission of other charged particles (7, ~), (7, 4ct), (7,3He) and (7, d) are given in a review paper by Fuller [12]. b) 30-160 MeV Total photon absorption cross sections for (7, hadrons) for 160 were measured by Ahrens et al [13].…”
Section: A Theoretical Calculationsmentioning
confidence: 99%
See 1 more Smart Citation
“…We used the following data to get charge changing photo cross sections av for 160: a) 10-30 MeV Photo cross sections for 160 for the emission of one proton and one neutron (7, np), for the emission of at least one proton and no neutron (?, p+ X) and for the emission of other charged particles (7, ~), (7, 4ct), (7,3He) and (7, d) are given in a review paper by Fuller [12]. b) 30-160 MeV Total photon absorption cross sections for (7, hadrons) for 160 were measured by Ahrens et al [13].…”
Section: A Theoretical Calculationsmentioning
confidence: 99%
“…We checked the validity of a theoretical model by Bertulani and Baur [10] describing the process of ED using virtual photon spectra from [11] and the energy dependent photo cross sections for 160 nuclei from nucleon emission threshold ~ 10 MeV up to 5000 MeV [12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 99%
“…Most important in this respect is the collective giant dipole resonance, and the energy and angular distributions of the emerging photonuclear fragments therefore depend strongly on the photon energy and the target nuclei (Hayward 1970). For photon energies above 30 MeV, the dominant processes are photoneutron and photoproton production where the (γ , n ) and (γ , p) cross sections are rather similar in magnitude and shape (Fuller 1985). The photoneutron reaction is of main interest in this study since photoproton reactions do not generally generate positron-emitting radionuclides and hence do not contribute to the PET activity.…”
Section: Photonuclear Reactionsmentioning
confidence: 99%
“…The main photoneutron reactions resulting in the production of the positron-emitting radionuclides are 12 C(γ , n) 11 C, 14 N(γ , n) (Gudowska et al 1999). Positron emitters 11 C and 12 C(γ , 2n) 10 C. However, the integrated photonuclear cross sections for these reactions constitute, respectively, 0.5%, 0.8%, 3.5% and 0.2% of the respective integrated photoneutron cross section (Fuller 1985). As shown in figure 1, the peaks of the photoneutron cross sections, σ γ ,n (E), are often in the photon energy range 18-25 MeV.…”
Section: Photonuclear Reactionsmentioning
confidence: 99%
“…Since the photoproton cross section on 12C is large (and exceeds the photoneutron cross section), the Dietrich and Berman compilations of photoneutron data cannot be used to obtain the total photoabsorption cross section. Instead, these cross sections were taken from the Fuller evaluation [75], which is based upon absorption measurements by Ahrens et al [76].…”
Section: Level Densities and Discrete Levelsmentioning
confidence: 99%