Published June 1, 2010 | Version v1
Journal article

Extra γ-ray strength for 116,117Sn arising from pygmy dipole resonance

  • 1. Department of Physics, Konan University, Okamoto 8-9-1, Higashinada, Kobe 658-8501 (Japan)
  • 2. National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568 (Japan)
  • 3. Cyclotron Institute, Texas A and M University, College Station, Texas 77843 (United States)
  • 4. Institute d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles, Campus de la Plaine, CP-226, 1050 Brussels (Belgium)

Description

Photoneutron cross sections were measured for 117Sn and 116Sn near neutron thresholds with quasi-monochromatic laser Compton scattering γ-rays. The measured cross sections for 117Sn and 116Sn are strongly enhanced from the threshold behavior expected for L = 1 neutron emissions after E1 photoexcitation. This suggests the presence of extra γ-ray strength in the low-energy tail of the giant dipole resonance. The present cross sections were analyzed together with radiative neutron capture cross sections for 116Sn within the framework of the statistical model calculation. It is shown that the extra γ-ray strength can be interpreted as pygmy E1 resonance which was previously reported in the nuclear resonance fluorescence experiment for 116Sn and 124Sn.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1238
Journal Issue
1
Journal Page Range
p. 234-236
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
7. Tours symposium on nuclear physics and astrophysics
Dates
16-20 Nov 2009
Place
Kobe (Japan)

Optional Information

Notes
(c) 2010 American Institute of Physics