Large-space shell-model calculations for light nuclei

Abstract

An effective two-body interaction is constructed from a new Reid-like $NN$ potential for a large no-core space consisting of six major shells and is used to generate the shell-model properties for light nuclei from $A$=2 to 6. (For practical reasons, the model space is partially truncated for $A$=6.) Binding energies and other physical observables are calculated and compare favorably with experiment.

prepared using LaTex, 21 manuscript pages, no figures

References in corpus (9)

• Construction of high-quality Nucleon-Nucleon potential models
• Monte Carlo evaluation of path integrals for the nuclear shell model
• Monte Carlo methods for the nuclear shell model
• Triton calculations with the new Nijmegen potentials
• Microscopic Calculations of the Spectra of Light Nuclei
• Simple approximation for the starting-energy-independent two-body effective interaction with applications to 6Li
• Medium corrections to the tensor interaction in nuclei: Energy difference of T=1 and T=0 J=0- states in 16O
• Minimizing Effective Many-Body Interactions
• Determination of Dipole Polarization Effects in ${}^7$Li and ${}^{11}$Li

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