Shell-model calculations for neutron-rich carbon isotopes with a chiral nucleon-nucleon potential

Abstract

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 been both 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 dripline. The correct location of the dripline is reproduced.

5 pages, 4 figures, 5 tables, to be published in Physical Review C

References in corpus (5)

• Shell-model calculations and realistic effective interactions
• Lifetime measurements of first excited states in 16,18C
• Low Momentum Nucleon-Nucleon Interactions and Shell-Model Calculations
• Shell-model study of the N=82 isotonic chain with a realistic effective hamiltonian
• Self-Consistent Nuclear Shell-Model Calculation Starting from a Realistic NN Potential

Cited by in corpus (20)

• Chiral effective field theory and nuclear forces
• Evidence for the ground-state resonance of 26O
• Shrunk halo and quenched shell gap at $N=16$ in ${}^{22}$C: Inversion of $sd$ states and deformation effects
• The calculation of the neutrinoless double-beta decay matrix element within the realistic shell model
• Implications of a matter-radius measurement for the structure of Carbon-22
• Study of ground state properties of carbon isotopes with deformed relativistic Hartree-Bogoliubov theory in continuum
• Renormalization of the GT operator within the realistic shell model
• Ab initio Gamow in-medium similarity renormalization group with resonance and continuum
• Search for ${}^{21}$C and constraints on ${}^{22}$C
• Perturbative Approach to Effective Shell-Model Hamiltonians and Operators
• Shell-model study of quadrupole collectivity in light tin isotopes
• Observation of a low-lying neutron-unbound state in 19C
• The radius of a typical-mass neutron star and chiral effective field theory
• From Kuo-Brown to today's realistic shell-model calculations
• Structure of 16C from analyses of proton scattering data and the B(E2) problem
• Fully microscopic shell-model calculations with realistic effective hamiltonians
• Chiral nucleon-nucleon forces in nuclear structure calculations
• Neutrinoless Double-Beta Decay and Realistic Shell Model
• Study of nucleonic matter with a consistent two- and three-body perturbative chiral interaction
• An overview of symmetric nuclear matter properties from chiral interactions up to fourth order of the chiral expansion