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

Gyurky, Gy. and Kiss, G. G. and Elekes, Z. and Fulop, Zs. and Somorjai, E. and Palumbo, A. and Gorres, J. and Lee, H. Y. and Rapp, W. and Wiescher, M. and Ozkan, N. and Guray, R. T. and Efe, G. and Rauscher, T.. (2006) α-induced cross sections of ¹⁰⁶Cd for the astrophysical p process. Physical review. C, Nuclear physics, Vol. 74, H. 2 , 025805, 9 S..

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Official URL: http://edoc.unibas.ch/dok/A5253893

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Abstract

The Cd-106(alpha,gamma)Sn-110 reaction cross section has been measured in the energy range of the Gamow window for the astrophysical p-process scenario. The cross sections for Cd-106(alpha,n)Sn-109 and for Cd-106(alpha,p)In-109 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 Cd-106(alpha,gamma)Sn-110 when using the standard optical potentials can be removed with a different alpha + Cd-106 potential. Some astrophysical implications are discussed.
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Rauscher, Thomas
Item Type:Article, refereed
Article Subtype:Research Article
Publisher:American Institute of Physics
ISSN:0556-2813
Note:Variant title: alpha-induced cross sections of Cd-106 for the astrophysical p process -- Publication type according to Uni Basel Research Database: Journal article
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Last Modified:22 Mar 2012 14:25
Deposited On:22 Mar 2012 13:49

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