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dc.contributor.authorBARRETT, Bruce R.
dc.contributor.authorDIKMEN, Erdal
dc.contributor.authorMARIS, Pieter
dc.contributor.authorSHIROKOV, Andrey M.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorSMIRNOVA, Nadya A.
dc.contributor.authorVARY, James P.
dc.date.issued2017
dc.date.conference2016-06-19
dc.description.abstractEnSeveral techniques now exist for performing detailed and accurate calculations of the structure of light nuclei, i.e., A ≤ 16. Going to heavier nuclei requires new techniques or extensions of old ones. One of these is the so-called No Core Shell Model (NCSM) with a Core approach, which involves an Okubo-Lee-Suzuki (OLS) transformation of a converged NCSM result into a single major shell, such as the sd-shell. The obtained effective two-body matrix elements can be separated into core and single-particle (s.p.) energies plus residual two-body interactions, which can be used for performing standard shell-model (SSM) calculations. As an example, an application of this procedure will be given for nuclei at the beginning ofthe sd-shell.
dc.language.isoen
dc.source.titleJPS Conf.Proc.
dc.title.enMicroscopic Shell Model Calculations for sd-Shell Nuclei
dc.typeCommunication dans un congrès
dc.identifier.doi10.7566/JPSCP.14.021006
dc.subject.halPhysique [physics]/Physique Nucléaire Théorique [nucl-th]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.page021006
bordeaux.volume14
bordeaux.countryJP
bordeaux.title.proceedingJPS Conf.Proc.
bordeaux.conference.cityNiigata
bordeaux.peerReviewednon
hal.identifierhal-02058579
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2016-06-24
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02058579v1
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