Radiative capture reactions and α-elastic scattering on 106Cd for the astrophysical p-process

Details Radiative capture reactions and α-elastic scattering on 106Cd for the astrophysical p-process Radiative capture reactions and α-elastic scattering on 106Cd for the astrophysical p-process

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..819..201g&link_type=abstract

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS: 12th International Symposium. AIP Conference Proceedings, Volume 819, pp. 20

Astronomy and Astrophysics

Astrophysics

Radiative Capture, Elastic And Inelastic Scattering, 90<=A<=149, Fundamental Aspects Of Astrophysics

Scientific paper

In the present work both the (α,γ) and (p,γ) cross sections on the p-nucleus 106Cd have been measured in the energy range relevant to the astrophysical p-process. The results are compared with the predictions of the statistical model calculations implemented with the NON-SMOKER code using different input parameters. The proton capture cross section has also been measured for 108Cd.
The α + 106Cd optical potential, an important input parameter for the 106Cd(α,γ) reaction rate determination, can be determined directly by measuring the deviation from the Rutherford scattering in the 106Cd(α,α)106Cd elastic scattering experiment. This experiment has also been performed in a wide angular range and the results are compared with different global optical potentials.

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