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Gamma-ray strength functions and their relation to astrophysics

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3628386· OSTI ID:21612057
; ; ; ; ; ; ; ; ; ; ; ; ;  [1];  [2];  [3];  [4];  [5];  [6];  [7]
  1. Department of Physics/SAFE, University of Oslo, N-0316 Oslo (Norway)
  2. Institut d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles, CP 226, 1050 Brussels (Belgium)
  3. Department of Physics, Eskisehir Osmangazi University, Meselik 26480 (Turkey)
  4. Stanford University, Palo Alto, California 94305 (United States)
  5. Dapnia/SPhN, CEA-Saclay (France)
  6. Department of Physics/SAFE, Aabo Akademi, FIN-20500 Aabo (Finland)
  7. Department of Physics, North Carolina State University, Raleigh, NC 27695 (United States)
The nuclear {gamma}-ray strength function is one of the indispensable inputs needed for reaction-rate calculations, and is particularly important for the neutron-capture cross section. The nuclear physics group at the Oslo Cyclotron Laboratory has developed a method to extract simultaneously nuclear level density and {gamma}-ray strength function from particle-{gamma} coincidence measurements. Data on the strength functions of Sn nuclei as well as for lighter elements are presented. The Sn isotopes all display a resonance-like structure close to the neutron threshold, that could possibly be due to the neutron-skin oscillation mode. This so-called pygmy dipole resonance greatly influences the neutron-capture rates. In the lighter nuclei, an enhancement of the strength function at low {gamma} energies is observed. The possible impact of this increase on Maxwellian-averaged reaction rates has been investigated.
OSTI ID:
21612057
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1377; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English