Medium-mass nuclei from chiral nucleon-nucleon interactions
arXiv:0806.3478 · doi:10.1103/PhysRevLett.101.092502
Abstract
We compute the binding energies, radii, and densities for selected medium-mass nuclei within coupled-cluster theory and employ the "bare" chiral nucleon-nucleon interaction at order N3LO. We find rather well-converged results in model spaces consisting of 15 oscillator shells, and the doubly magic nuclei 40Ca, 48Ca, and the exotic 48Ni are underbound by about 1 MeV per nucleon within the CCSD approximation. The binding-energy difference between the mirror nuclei 48Ca and 48Ni is close to theoretical mass table evaluations. Our computation of the one-body density matrices and the corresponding natural orbitals and occupation numbers provides a first step to a microscopic foundation of the nuclear shell model.
5 pages, 5 figures
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- Complex coupled-cluster approach to an ab-initio description of open quantum systems
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- Fock space relativistic coupled-Cluster calculations of Two-Valence Atoms
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- Closed-shell properties of O with {\em ab initio} coupled-cluster theory
- Summation of Parquet diagrams as an ab initio method in nuclear structure calculations