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Phys. Rev. C 79, 025801 (2009) [8 pages]

Photodisintegration of 80Se: Implications for the s-process branching at 79Se

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A. Makinaga1, H. Utsunomiya1, S. Goriely2, T. Kaihori1, S. Goko3, H. Akimune1, T. Yamagata1, H. Toyokawa4, T. Matsumoto4, H. Harano4, H. Harada3, F. Kitatani3, Y. K. Hara3, S. Hohara5, and Y.-W. Lui6
1Department of Physics, Konan University, Okamoto 8-9-1, Higashinada, Kobe 658-8501, Japan
2Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Campus de la Plaine, CP-226, 1050 Brussels, Belgium
3Japan Atomic Energy Agency, Tokai-mura, Naka, Ibaraki 319-1195, Japan
4National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan
5Atomic Energy Research Institute, Kinki University, Kowakae 3-4-1, Osaka 577-8502, Japan
6Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA

Received 19 May 2008; revised 24 November 2008; published 5 February 2009

Photoneutron cross sections were measured for 80Se immediately above the neutron separation energy with quasimonochromatic γ-ray beams to experimentally constrain the E1 γ strength function for 80Se. Two sets of the γ strength function and the level density that equally meet the experimental constraint predict largely different neutron capture cross sections for 79Se. Based on the Maxwellian-averaged cross sections of the latest compilation complemented with the predicted cross sections for 79Se, we calculated σN values of the main s-process component using a phenomenological model and deduced empirical abundances of the weak s-process component. An attempt is made of considering the implications of the abundance ratios of 80Kr and 82Kr within the framework of phenomenological models for the weak s process.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.79.025801
DOI:
10.1103/PhysRevC.79.025801
PACS:
26.50.+x, 25.20.Lj, 24.60.Dr, 27.50.+e