Mocelj, D. and Rauscher, T. and Martinez-Pinedo, G. and Alhassid, Y.. (2003) The importance of parity-dependence of the nuclear level density in the prediction of astrophysical reaction rates. In: Capture gamma-ray spectroscopy and related topics : proceedings of the 11th International Symposium on ... Pruhonice near Prague, 2-6 September 2002. New Jersey [u.a.], pp. 781-784.
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Official URL: http://edoc.unibas.ch/dok/A5839264
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Abstract
A simple description for obtaining the parity distribution of nuclear levels in the pf + g(9/2) shell as a function of excitation energy was recently derived. We implement this in a global nuclear level density model. In the framework of the statistical model, cross sections and astrophysical reaction rates are calculated in the Fe region and compared to rates obtained with the common assumption of an equal distribution of parities. We find considerable differences, especially for reactions involving particles in the exit channel.
| Faculties and Departments: | 05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann) |
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| UniBasel Contributors: | Rauscher, Thomas |
| Item Type: | Conference or Workshop Item, refereed |
| Conference or workshop item Subtype: | Conference Paper |
| Publisher: | World Scientific |
| Note: | Publication type according to Uni Basel Research Database: Conference paper |
| Identification Number: |
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| Last Modified: | 08 Jun 2012 06:54 |
| Deposited On: | 08 Jun 2012 06:33 |
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