Published January 24, 2008
| Version v1
Journal article
Mirror Nuclei: Symmetry Breaking and Nuclear Dynamics
Creators
- 1. Dipartimento di Fisica dell'Universita and INFN, I-35131 Padova (Italy)
Description
Differences in excitation energy between isobaric analogue states are measured to study the validity of isospin symmetry in medium-mass nuclei as a function of the angular momentum These differences are of the order of tens of keV and can be well reproduced by state-of-the-art shell model calculations. Several nuclear structure properties can be deduced from these data, such as the alignment of nucleons along rotational bands, the evolution of the nuclear radius and the appearance of pure single particle configurations across two main shells. In addition, the isospin breaking of the nuclear interaction is suggested by the systematic comparison with the data
Additional details
Identifiers
- DOI
- 10.1063/1.2870324;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 972
- Journal Issue
- 1
- Journal Page Range
- p. 31-39
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- Carpathian summer school of physics 2007 on exotic nuclei and nuclear/particle astrophysics (II)
- Dates
- 21-31 Aug 2007
- Place
- Sinaia (Romania)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39069730
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANGULAR MOMENTUM; COMPARATIVE EVALUATIONS; EXCITATION; GAMMA SPECTROSCOPY; INTERMEDIATE MASS NUCLEI; ISOBARIC ANALOGS; ISOSPIN; KEV RANGE; MIRROR NUCLEI; NUCLEAR STRUCTURE; NUCLEONS; ROTATIONAL STATES; SHELL MODELS; SYMMETRY; SYMMETRY BREAKING
- Descriptors DEC
- BARYONS; ELEMENTARY PARTICLES; ENERGY LEVELS; ENERGY RANGE; ENERGY-LEVEL TRANSITIONS; EVALUATION; EXCITED STATES; FERMIONS; HADRONS; MATHEMATICAL MODELS; NUCLEAR MODELS; NUCLEI; PARTICLE PROPERTIES; SPECTROSCOPY
Optional Information
- Notes
- (c) 2008 American Institute of Physics