skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: THE {gamma}SF METHOD

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3628388· OSTI ID:21612060
; ; ; ; ;  [1];  [2]; ;  [3];  [3]; ;  [4];  [5];  [6];  [7]
  1. Department of Physics, Konan University, Okamoto 8-9-1, Higashinada, Kobe 658-8501 (Japan)
  2. Institut d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles, Campus de la Plaine, CP-226, 1050 Brussels (Belgium)
  3. Japan Atomic Energy Agency, Tokai-mura, Naka, Ibaraki 319-1195 (Japan)
  4. National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568 (Japan)
  5. Cyclotron Institute, Texas A and M University, College Station, Texas 77843 (United States)
  6. CEA, DAM, DIF, F-91297 Arpajon (France)
  7. Nuclear Research and Consultancy Group, P.O. Box 25, NL-1755 ZG Petten (Netherlands)

The {gamma}-ray strength function ({gamma}SF) interconnects radiative neutron capture and photoneutron emission as a common ingredient in the statistical model. Outlined here is an indirect method of determining radiative neutron-capture cross sections for unstable nuclei based on the {gamma}-ray strength function. Application examples of the {gamma}SF method are demonstrated.

OSTI ID:
21612060
Journal Information:
AIP Conference Proceedings, Vol. 1377, Issue 1; Conference: FINUSTAR 3 Conference on frontiers in nuclear structure, astrophysics, and reactions, Rhodes (Greece), 23-27 Aug 2010; Other Information: DOI: 10.1063/1.3628388; (c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English