Published December 2009
| Version v1
Journal article
Predicted levels of 9Be based on a theoretical analysis of neutron double-differential cross sections at En=14.1 and 18 MeV
- 1. College of Physics and Technology, Guangxi Normal University, Guilin 541004 (China)
- 2. China Institute of Atomic Energy, P. O. Box 275(41), Beijing 102413 (China)
Description
By using the statistical theory for neutron-induced light nucleus reaction, the calculation of the neutron double-differential cross sections for n+9Be reactions is performed. The secondary outgoing neutrons only coming from the (n,2n)2α reaction channel through six different emission processes are illustrated in detail in this article. Based on the theoretical analysis of neutron double-differential cross sections at En=14.1 and 18 MeV, two predicted levels of 9Be, i.e., E(Jπ)Γ=9((5/2)+)1000 and 10((5/2)+)1000, have been recommended. The calculated results indicate that the fittings would be improved obviously while the predicted levels have been employed.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 80
- Journal Issue
- 6
- Journal Page Range
- p. 064612-064612.8
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41042909
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ALPHA PARTICLES; BERYLLIUM 9; DIFFERENTIAL CROSS SECTIONS; EMISSION; LIGHT NUCLEI; MEV RANGE 10-100; NEUTRON EMISSION; NEUTRON REACTIONS; NEUTRONS; SIMULATION; STATISTICAL MODELS
- Descriptors DEC
- ALKALINE EARTH ISOTOPES; BARYON REACTIONS; BARYONS; BERYLLIUM ISOTOPES; CHARGED PARTICLES; CROSS SECTIONS; ELEMENTARY PARTICLES; EMISSION; ENERGY RANGE; EVEN-ODD NUCLEI; FERMIONS; HADRON REACTIONS; HADRONS; IONIZING RADIATIONS; ISOTOPES; LIGHT NUCLEI; MATHEMATICAL MODELS; MEV RANGE; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; NUCLEONS; RADIATIONS; STABLE ISOTOPES
Optional Information
- Notes
- (c) 2009 The American Physical Society