Published September 2010
| Version v1
Journal article
Systematics of 21+ states in semimagic nuclei
Creators
- 1. Academy of Romanian Scientists, 54 Splaiul Independentei, Bucharest 050094 (Romania)
- 2. 'Horia Hulubei' National Institute of Physics and Nuclear Engineering, 407 Atomistilor, Bucharest-Magurele 077125 (Romania)
Description
We propose a simple systematics of low-lying 21+ energy levels and electromagnetic transitions in semimagic isotopic chains Z=28,50,82 and isotonic chains N=28,50,82,126. To this purpose we use a two-level pairing plus quadrupole Hamiltonian, within the spherical quasiparticle random phase approximation (QRPA). We derive a simple relation connecting the 21+ energy with the pairing gap and quadrupole-quadupole (QQ) interaction strength. It turns out that the systematics of energy levels and B(E2) values predicted by this simple model is fulfilled with a reasonable accuracy by all available experimental data. This systematics suggests that not only active nucleons but also those filling closed shells play an important role.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.82.031302;
- arXiv
- arXiv:1006.0059v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 82
- Journal Issue
- 3
- Journal Page Range
- p. 031302-031302.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42013644
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ACCURACY; CHAINS; E2-TRANSITIONS; ENERGY LEVELS; ENERGY-LEVEL TRANSITIONS; FASTENING; HAMILTONIANS; INTERACTIONS; MAGIC NUCLEI; NUCLEI; NUCLEONS; RANDOM PHASE APPROXIMATION; SPHERICAL CONFIGURATION
- Descriptors DEC
- APPROXIMATIONS; BARYONS; CALCULATION METHODS; CONFIGURATION; ELEMENTARY PARTICLES; ENERGY-LEVEL TRANSITIONS; FABRICATION; FERMIONS; HADRONS; JOINING; MATHEMATICAL OPERATORS; MULTIPOLE TRANSITIONS; NUCLEI; QUANTUM OPERATORS
Optional Information
- Notes
- (c) 2010 The American Physical Society