Structure of the Hoyle State in 12C
- 1. Institut fuer Kernphysik, Technische Universitaet Darmstadt, D-64289 Darmstadt (Germany)
- 2. Gesellschaft fuer Schwerionenforschung, D-64291 Darmstadt (Germany)
- 3. National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824 (United States)
Description
The first excited 0+ state in 12C (Hoyle state) has been predicted to be a dilute self-bound gas of bosonic α particles, similar to a Bose-Einstein condensate. To clarify this conjecture, precise electron scattering data on form factors of the ground state and the transition to the Hoyle state are compared with results of the fermionic molecular dynamics model, a microscopic α-cluster model, and an α-cluster model with reduced degrees of freedom (in the spirit of a Bose-Einstein condensed state). The data indicate clearly a dilute density with a large spatial extension of the Hoyle state. A closer inspection of the model calculations, which reproduce the experimental findings, reveals that the term Bose-Einstein condensation of three α particles must not be taken too literally
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 98
- Journal Issue
- 3
- Journal Page Range
- p. 032501-032501.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38024579
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ALPHA PARTICLES; BOSE-EINSTEIN CONDENSATION; CARBON 12; CLUSTER MODEL; DEGREES OF FREEDOM; ELECTRONS; FORM FACTORS; GROUND STATES; MOLECULAR DYNAMICS METHOD
- Descriptors DEC
- CALCULATION METHODS; CARBON ISOTOPES; CHARGED PARTICLES; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; ENERGY LEVELS; EVEN-EVEN NUCLEI; FERMIONS; IONIZING RADIATIONS; ISOTOPES; LEPTONS; LIGHT NUCLEI; MATHEMATICAL MODELS; NUCLEAR MODELS; NUCLEI; PARTICLE PROPERTIES; RADIATIONS; STABLE ISOTOPES
Optional Information
- Notes
- (c) 2007 The American Physical Society