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• W2805372783 abstract "In this paper we present an evolution of our derivation of the shell-model effective Hamiltonian, namely introducing effects of three-body contributions. More precisely, we consider a three-body potential at next-to-next-to-leading order in chiral perturbation theory, and the induced three-body forces that arise from many-body correlations among valence nucleons. The first one is included, in the derivation of the effective Hamiltonian for one- and two-valence nucleon-systems, at first order in the many-body perturbation theory. Namely, we include only the three-body interaction between one or two valence nucleons and those belonging to the core. For nuclei with more than two valence particles, both induced - turned on by the two-body potential - and genuine three-body forces come into play. Since it is difficult to perform shell-model calculations with three-body forces, these contributions are estimated for the ground-state energy only. In order to establish the reliability of our approximations, we focus attention on nuclei belonging to the p shell, aiming to benchmark our calculations against those performed with the ab initio no-core shell-model. The obtained results are satisfactory, and pave the way to the application of our approach to nuclear systems with heavier masses." @default.
• W2805372783 created "2018-06-13" @default.
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• W2805372783 date "2018-10-05" @default.
• W2805372783 modified "2023-10-17" @default.
• W2805372783 title "Realistic shell-model calculations for <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mi>p</mml:mi></mml:math> -shell nuclei including contributions of a chiral three-body force" @default.
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• W2805372783 doi "https://doi.org/10.1103/physrevc.98.044305" @default.
• W2805372783 hasPublicationYear "2018" @default.
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