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• W2596970420 abstract "We report on a quantitative study of the evolution of the nuclear shell structure, in particular, effective single-particle energies (ESPEs), based on the spin-tensor decomposition of an effective two-body shell-model interaction. While the global trend of the ESPEs is mainly due to the central term of the effective interaction, variations of shell gaps invoke various components of the in-medium NN force. From a detailed analysis of a well-fitted realistic interaction in the $sdpf$ shell-model space, two most important contributions for the evolution of the $Nphantom{rule{-0.16em}{0ex}}=phantom{rule{-0.16em}{0ex}}20$ and $Nphantom{rule{-0.16em}{0ex}}=phantom{rule{-0.16em}{0ex}}28$ shell gaps are confirmed to be the central term and the tensor term. The role of the latter is dominant to explain the energy shift of spin-orbit partners. Spin-tensor analysis of microscopic effective interactions in $sd$, $pf$, and $gds$ shell-model spaces, contrasted with that of the phenomenologically adjusted ones, shows no evidence of amplification of the tensor component contribution; however, it points toward the neglect of three-body forces in the present microscopic interactions." @default.
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• W2596970420 date "2012-09-10" @default.
• W2596970420 modified "2023-10-16" @default.
• W2596970420 title "Nuclear shell evolution and in-medium<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:mi>N</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:math>interaction" @default.
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• W2596970420 doi "https://doi.org/10.1103/physrevc.86.034314" @default.
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