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dc.contributor.authorStroberg, S. R.
dc.contributor.authorHenderson, J.
dc.contributor.authorHackman, G.
dc.contributor.authorRuotsalainen, P.
dc.contributor.authorHagen, G.
dc.contributor.authorHolt, J. D.
dc.date.accessioned2022-06-21T10:24:05Z
dc.date.available2022-06-21T10:24:05Z
dc.date.issued2022
dc.identifier.citationStroberg, S. R., Henderson, J., Hackman, G., Ruotsalainen, P., Hagen, G., & Holt, J. D. (2022). Systematics of E2 strength in the sd shell with the valence-space in-medium similarity renormalization group. <i>Physical Review C</i>, <i>105</i>(3), Article 034333. <a href="https://doi.org/10.1103/PhysRevC.105.034333" target="_blank">https://doi.org/10.1103/PhysRevC.105.034333</a>
dc.identifier.otherCONVID_146519842
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/81928
dc.description.abstractBackground: Recent developments in ab initio nuclear theory demonstrate promising results in medium- to heavy-mass nuclei. A particular challenge for many of the many-body methodologies, however, is an accurate treatment of the electric-quadrupole, E2, strength associated with collectivity. Purpose: The valence-space in-medium similarity renormalization group (VS-IMSRG) is a particularly powerful method for accessing medium- and high-mass nuclei but has been found to underpredict E2 strengths. The purpose of this work is to evaluate the isospin dependence of this underprediction. Methods: We perform a systematic comparison of VS-IMSRG calculations with available literature. We make use of isoscalar and isovector contributions to the E2 matrix elements to assess isoscalar and isovector contributions to the missing strength. Results: It is found that the E2 strength is consistent throughout Tz=∣∣12∣∣, Tz=|1|, Tz=∣∣32∣∣, and Tz=2 pairs within the sd shell. Furthermore, no isovector contribution to the deficiency is identified. Conclusions: A comparison with toy-models and coupled-cluster calculations is used to discuss potential origins of the missing strength, which arises from missing many-particle, many-hole excitations out of the model space. The absence of any significant isovector contribution to the missing E2 strength indicates that the E2 strength discrepancy, and therefore any correction, is largely independent of the isospin of the nuclei in question.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.titleSystematics of E2 strength in the sd shell with the valence-space in-medium similarity renormalization group
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202206213535
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries3
dc.relation.volume105
dc.type.versionpublishedVersion
dc.rights.copyright©2022 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.105.034333
jyx.fundinginformationThis work has been supported by the Natural Sciences and Engineering Research Council of Canada (NSERC), The Canada Foundation for Innovation and the British Columbia Knowledge Development Fund. TRIUMF receives federal funding via a contribution agreement through the National Research Council of Canada. Computations were performed with an allocation of computing resources on Cedar at WestGrid and Compute Canada, and on the Oak Cluster at TRIUMF managed by the University of British Columbia department of Advanced Research Computing (ARC). Work at LLNL was performed under Contract No. DE-AC52-07NA27344. This work was supported by the Office of Nuclear Physics, U.S. Department of Energy, under Grant no. desc0018223 (NUCLEI SciDAC-4 collaboration) and by the Field Work Proposal No. ERKBP72 at Oak Ridge National Laboratory (ORNL). S.R.S. was supported by the U.S. Department of Energy office of Science, Office of Nuclear Physics, under Contract Nos. DE-FG02-97ER41014 and DEAC02-06CH11357. J.H. is supported at the University of Surrey under UKRI Future Leaders Fellowship Grant No. MR/T022264/1.
dc.type.okmA1


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