W. Rapp

Alpha-induced cross-sections of Cd-106 for the astrophysical p-process

The {sup 106}Cd({alpha},{gamma}){sup 110}Sn reaction cross section has been measured in the energy range of the Gamow window for the astrophysical p-process scenario. The cross sections for {sup 106}Cd({alpha},n){sup 109}Sn and for {sup 106}Cd({alpha},p){sup 109}In below the ({alpha},n) threshold have also been determined. The results are compared with predictions of the statistical model code NON-SMOKER using different input parameters. The comparison shows that a discrepancy for {sup 106}Cd({alpha},{gamma}){sup 110}Sn when using the standard optical potentials can be removed with a different {alpha} + {sup 106}Cd potential. Some astrophysical implications are discussed.

Cross section measurements of α-induced reactions on Mo 92 , 94 and Sn 112 for p -process studies

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Cross section measurements of α-induced reactions on 92,94Mo and 112Sn for p-process studies

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Cross section measurements of alpha-induced reactions on Mo-92, Mo-94 and Sn-112 for p-process studies

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Astrophysical S factor for {alpha}-capture on {sup 112}Sn in the p-process energy range

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Α-induced cross sections of 106Cd for the astrophysical p process

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a-induced cross sections of Cd106 for the astrophysical p process

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CERN n_TOF facility: performance report

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Cross section measurements of a-induced reactions on Mo92,94 and Sn112 for p-process studies

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Cross section measurements of -induced reactions on {sup 92,94}Mo and Sn for p-process studies

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