Published February 2010
| Version v1
Journal article
g factors of coexisting isomeric states in 188Pb
Creators
- 1. National Institute for Physics and Nuclear Engineering, Bucharest (Romania)
- 2. Dipartimento di Fisica dell' Universita and INFN, Sezione di Padova, Padova (Italy)
- 3. Laboratori Nazionali di Legnaro, Legnaro (Italy)
- 4. Helmholtz-Institut fuer Strahlen- und Kernphysik, Universitaet Bonn, D-53115 Bonn (Germany)
- 5. Instituto de Fisica, Universidade de Sao Paulo, Sao Paulo (Brazil)
Description
The g factors of the 12+, 11-, and 8- isomeric states in 188Pb were measured using the time-differential perturbed angular distribution method as g(12+)=-0.179(6), g(11-)=+1.03(3), and g(8-)=-0.037(7). The g factor of the 12+ state follows the observed slight down-sloping evolution of the g factors of the i13/22 neutron spherical states with decreasing N. The g factors of the 11- and 8- isomers proposed as oblate and prolate deformed states, respectively, were interpreted within the rotational model, using calculated and empirical g factor values for the involved single-particle orbitals.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 81
- Journal Issue
- 2
- Journal Page Range
- p. 024323-024323.5
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41115208
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ANGULAR DISTRIBUTION; EVOLUTION; ISOMERS; LANDE FACTOR; LEAD 188; NEUTRONS; SPHERICAL CONFIGURATION
- Descriptors DEC
- ALPHA DECAY RADIOISOTOPES; BARYONS; BETA DECAY RADIOISOTOPES; BETA-PLUS DECAY RADIOISOTOPES; CONFIGURATION; DIMENSIONLESS NUMBERS; DISTRIBUTION; ELECTRON CAPTURE RADIOISOTOPES; ELEMENTARY PARTICLES; EVEN-EVEN NUCLEI; FERMIONS; HADRONS; HEAVY NUCLEI; ISOTOPES; LEAD ISOTOPES; NUCLEI; NUCLEONS; RADIOISOTOPES; SECONDS LIVING RADIOISOTOPES
Optional Information
- Notes
- (c) 2010 The American Physical Society