Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Cross section measurement on {sup 139}La (gamma,gamma') below neutron separation energy

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3455936· OSTI ID:21362109
 [1];  [2]; ; ; ; ; ; ; ; ;  [3];  [4];  [5]
  1. Hokkaido University VBL, Kita 10-jo, Nishi 8-chome, Kita-ku, Sapporo, Hokkaido (Japan)
  2. Department of Physics, Duke University, and Triangle Universities Nuclear Laboratory, Durham, North Carolina 27708 (United States)
  3. Institut fuer Strahlenphysik, Forschungszentrum Dresden-Rossendorf, D-01314 Dresden (Germany)
  4. LIP, Physics Department, University of Coimbra, 3004-516 Coimbra (Portugal)
  5. Vattenfall Power, S-16216 Stockholm (Sweden)
The gamma-ray strength function is an important input quantity for the determination of the photoreaction rate and the neutron capture rate for astrophysics as well as for nuclear technologies. Recent studies show that extra gamma-ray strength near the neutron separation energy S{sub n}(pygmy resonance) affects the stellar reaction rate strongly. In this work, the photoabsorption cross section for {sup 139}La below S{sub n} was measured using bremsstrahlung produced at the electron accelerator ELBE of Eorschungszentrum Dresden-Rossendorf with an electron beam of 11.5 MeV kinetic energy. Experimental result of {sup 139}La is presented.
OSTI ID:
21362109
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1238; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English