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Phys. Rev. C 74, 025806 (2006) [6 pages]

Photoneutron cross section measurements on the N=82 nuclei 139La and 141Pr: Implications for p-process nucleosynthesis

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H. Utsunomiya1, A. Makinaga1, S. Goko1, T. Kaihori1, H. Akimune1, T. Yamagata1, M. Ohta1, H. Toyokawa2, S. Müller3, Y.-W. Lui4, and S. Goriely5
1Department of Physics, Konan University, Okamoto 8-9-1, Higashinada, Kobe 658-8501, Japan
2National Institute of Advanced Industrial Science and Technology, 1-1-1 Umezono, Tsukuba, Ibaraki 305-8568, Japan
3Institut fuer Kernphysik, TU Darmstadt, Schlossgartenstr 9, D-64289 Darmstadt, Germany
4Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA
5Institute d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Campus de la Plaine, CP-226, 1050 Brussels, Belgium

Received 23 September 2005; revised 5 January 2006; published 22 August 2006

Cross sections of the 139La(γ,n) and 141Pr(γ,n) reactions were measured using quasi-monochromatic γ-ray beams from laser Compton scattering. The results are compared to the predictions of Hauser-Feshbach statistical calculations using different models for the γ-ray strength function. The model parameters are constrained by the present experimental data and used to estimate the stellar photoneutron rates and their associated uncertainties and to study the implication for the production of the rare odd-odd nuclide 138La by the p process. No evidence for a large thermonuclear p-process contribution to the solar 138La is found. The need to further explore the photodestruction rate of 138La is emphasized.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.74.025806
DOI:
10.1103/PhysRevC.74.025806
PACS:
25.20.-x, 26.30.+k, 27.60.+j, 97.10.Tk