Spectroscopic factor calculations in the \textit{ab initio} no-core shell model

Fuente: arXiv
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Main Authors: Xie, M. R., Li, J. G., Michel, N., Zuo, W.
Format: Preprint
Published: 2024
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author Xie, M. R.
Li, J. G.
Michel, N.
Zuo, W.
author_facet Xie, M. R.
Li, J. G.
Michel, N.
Zuo, W.
contents The convergence properties of spectroscopic factors in the \textit{ab initio} no-core shell model are hereby investigated. For this, we consider nuclear energies and spectroscopic factors in $A = 6$ and 7 isotopes, using the chiral forces NNLO$_{\rm opt}$ and N$^3$LO. While low-lying spectrum energy demonstrates remarkable convergence with the increase of model space within the no-core shell model, the spectroscopic factor exhibits no definitive convergence trend and seems independent of the employed nuclear interaction. The use of spectroscopic factors issued from the no-core shell model to calculate cross-sections of knockout reaction might then be questionable. The results are compared with that of the standard shell model and \textit{ab initio} Monte Carlo calculations.
format Preprint
id arxiv_https___arxiv_org_abs_2411_04719
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Spectroscopic factor calculations in the \textit{ab initio} no-core shell model
Xie, M. R.
Li, J. G.
Michel, N.
Zuo, W.
Nuclear Theory
The convergence properties of spectroscopic factors in the \textit{ab initio} no-core shell model are hereby investigated. For this, we consider nuclear energies and spectroscopic factors in $A = 6$ and 7 isotopes, using the chiral forces NNLO$_{\rm opt}$ and N$^3$LO. While low-lying spectrum energy demonstrates remarkable convergence with the increase of model space within the no-core shell model, the spectroscopic factor exhibits no definitive convergence trend and seems independent of the employed nuclear interaction. The use of spectroscopic factors issued from the no-core shell model to calculate cross-sections of knockout reaction might then be questionable. The results are compared with that of the standard shell model and \textit{ab initio} Monte Carlo calculations.
title Spectroscopic factor calculations in the \textit{ab initio} no-core shell model
topic Nuclear Theory
url https://arxiv.org/abs/2411.04719