Electromagnetic transitions in 11B and 14C

Bell, R.A.I.; Gill, R.D.; Robertson, B.C.; Lopes, José Sérgio Leite; Rose, H. J.

doi:10.1016/0375-9474(68)90434-x

Cited by 15 publications

(1 citation statement)

References 38 publications

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“…The values of the mixing ratio δ were taken from Refs. [50,51] and used in the phase convention of Krane and Steffen. The calculated photon flux, normalized to that deduced from 11 B, is presented in Fig.…”

Section: Resultsmentioning

confidence: 99%

Low-energy tail of the giant dipole resonance inMo98andMo100

et al. 2008

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Dipole-strength distributions in the nuclides 98 Mo and 100 Mo up to the neutron-separation energies have been studied in photon-scattering experiments at the bremsstrahlung facility of the Forschungszentrum Dresden-Rossendorf. To determine the dipole-strength distributions up to the neutron-emission thresholds, statistical methods were developed for the analysis of the measured spectra. The measured spectra of scattered photons were corrected for detector response and atomic background by simulations using the code GEANT3. Simulations of γ -ray cascades were performed to correct the intensities of the transitions to the ground state for feeding from higher-lying levels and to determine their branching ratios. The photoabsorption cross sections obtained for 98 Mo and 100 Mo from the present (γ, γ ) experiments are combined with (γ, n) data from literature, resulting in a photoabsorption cross section covering the range from 4 to about 15 MeV of interest for network calculations in nuclear astrophysics. Novel information about the low-energy tail of the giant dipole resonance and its energy dependence is derived. The photoabsorption cross sections deduced from the present photon-scattering experiments are compared with existing data from neutron capture and 3 He-induced reactions.

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Section: Resultsmentioning

confidence: 99%