Tensor force role in decays analyzed within the Gogny-interaction shell model
arXiv:2109.02205 · doi:10.1103/PhysRevC.103.064327
Abstract
Background: The half-life of the famous C decay is anomalously long, with different mechanisms: the tensor force, cross-shell mixing, and three-body forces, proposed to explain the cancellations that lead to a small transition matrix element. Purpose: We revisit and analyze the role of the tensor force for the decay of C as well as of neighboring isotopes. Methods: We add a tensor force to the Gogny interaction, and derive an effective Hamiltonian for shell-model calculations. The calculations were carried out in a - model space to investigate cross-shell effects. Furthermore, we decompose the wave functions according to the total orbital angular momentum in order to analyze the effects of the tensor force and cross-shell mixing. Results: The inclusion of the tensor force significantly improves the shell-model calculations of the -decay properties of carbon isotopes. In particular, the anomalously slow decay of C can be explained by the isospin part of the tensor force, which changes the components of N with the orbital angular momentum , and results in a dramatic suppression of the Gamow-Teller transition strength. At the same time, the description of other nearby decays are improved. Conclusions: Decomposition of wave function into components illuminates how the tensor force modifies nuclear wave functions, in particular suppression of -decay matrix elements. Cross-shell mixing also has a visible impact on the -decay strength. Inclusion of the tensor force does not seem to significantly change, however, binding energies of the nuclei within the phenomenological interaction.
arXiv comment8 Pages,7 Figures
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