Published June 2010
| Version v1
Journal article
Shell-model calculations for neutron-rich carbon isotopes with a chiral nucleon-nucleon potential
- 1. Istituto Nazionale di Fisica Nucleare, Complesso Universitario di Monte S. Angelo, Via Cintia, I-80126 Napoli (Italy)
- 2. Dipartimento di Scienze Fisiche, Universita di Napoli Federico II, Complesso Universitario di Monte S. Angelo, Via Cintia, I-80126 Napoli (Italy)
Description
We have studied neutron-rich carbon isotopes in terms of the shell model employing a realistic effective Hamiltonian derived from the chiral N3LOW nucleon-nucleon potential. The single-particle energies and effective two-body interaction have both been determined within the framework of the time-dependent degenerate linked-diagram perturbation theory. The calculated results are in very good agreement with the available experimental data, providing a sound description of this isotopic chain toward the neutron drip line. The correct location of the drip line is reproduced.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.81.064303;
- arXiv
- arXiv:1005.2896v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 81
- Journal Issue
- 6
- Journal Page Range
- p. 064303-064303.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41117321
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- CARBON ISOTOPES; CHIRALITY; COMPUTERIZED SIMULATION; HAMILTONIANS; INTERACTIONS; NEUTRON-RICH ISOTOPES; NEUTRONS; NUCLEON-NUCLEON POTENTIAL; PERTURBATION THEORY; SHELL MODELS; SOUND WAVES; TIME DEPENDENCE; TWO-BODY PROBLEM
- Descriptors DEC
- BARYONS; BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; ELEMENTARY PARTICLES; FERMIONS; HADRONS; ISOTOPES; MANY-BODY PROBLEM; MATHEMATICAL MODELS; MATHEMATICAL OPERATORS; NUCLEAR MODELS; NUCLEONS; PARTICLE PROPERTIES; POTENTIALS; QUANTUM OPERATORS; RADIOISOTOPES; SIMULATION
Optional Information
- Notes
- (c) 2010 The American Physical Society