Extensions to the No-Core Shell Model pp 33-77 | Cite as
Importance Truncated No Core Shell Model
Abstract
The NCSM has been very successful at describing light nuclei (\(A \le 6\)), and in some cases, has also been able to describe nuclei in the middle of the p-shell (see [1] for an extensive list of results). However, NCSM calculations in the middle or in the upper part of the p-shell (\(A \ge 10\)) become very difficult to perform. Currently, interesting nuclei such as the Carbon or Oxygen isotopes are beyond the capabilities of the NCSM. To extend our calculations to the start of the sd-shell, is an even more challenging task. It is possible to do some exploratory calculations for the start of the sd-shell, in which \(N_\mathrm{max}\le 4\), but fully converged results will be out of reach for many years. We remind the reader that by fully converged results, we mean calculations which are free of the two NCSM parameters (\(N_\mathrm{max}\) and \(\hbar \Omega \)).
Keywords
Reference State Basis Space Configuration Interaction Importance Measure Slater DeterminantReferences
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