Published May 21, 2008
| Version v1
Journal article
E0 transition strength and cluster structure in 13C
Creators
- 1. Meme Media Laboratory, Hokkaido University 060-8628 Sapporo (Japan)
- 2. Department of physics, University of Tokyo, Hongo, 113-0033 Tokyo (Japan)
Description
We study the structure of low-lying states of 13C with a microscopic cluster model. The second 0+ state of 12C, which is known as the Hoyle state and is important for astrophysical reactions, has been clarified to have dilute α-cluster structure. On the basis of the α-cluster model, we discuss the effect of one valence neutron in 13C on the α-cluster configuration of the Hoyle state. For these purpose, we investigate the iso-scalar E0 transition probability from the ground 1/2- state to this excited states
Additional details
Identifiers
- DOI
- 10.1063/1.2943623;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1016
- Journal Issue
- 1
- Journal Page Range
- p. 451-453
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- From the dawn of Universe to the formation of solar system
- Acronym
- 10. international symposium on origin of matter and evolution of galaxies
- Dates
- 4-7 Dec 2007
- Place
- Sapporo (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40023419
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ALPHA PARTICLES; ASTROPHYSICS; CARBON 12; CARBON 13; CLUSTER MODEL; E0-TRANSITIONS; EXCITED STATES; NEUTRONS; NUCLEAR STRUCTURE; PROBABILITY; STRENGTH FUNCTIONS
- Descriptors DEC
- BARYONS; CARBON ISOTOPES; CHARGED PARTICLES; ELEMENTARY PARTICLES; ENERGY LEVELS; ENERGY-LEVEL TRANSITIONS; EVEN-EVEN NUCLEI; EVEN-ODD NUCLEI; FERMIONS; FUNCTIONS; HADRONS; IONIZING RADIATIONS; ISOTOPES; LIGHT NUCLEI; MATHEMATICAL MODELS; MULTIPOLE TRANSITIONS; NUCLEAR MODELS; NUCLEI; NUCLEONS; PHYSICS; RADIATIONS; STABLE ISOTOPES
Optional Information
- Notes
- (c) 2008 American Institute of Physics