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Please use this identifier to cite or link to this item: http://repository.iitr.ac.in/handle/123456789/13464
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dc.contributor.authorSaxena A.-
dc.contributor.authorKumar A.-
dc.contributor.authorKumar V.-
dc.contributor.authorSrivastava, Praveen Chandra-
dc.contributor.authorSuzuki T.-
dc.date.accessioned2020-10-15T12:34:28Z-
dc.date.available2020-10-15T12:34:28Z-
dc.date.issued2019-
dc.identifier.citationHyperfine Interactions (2019), 240(1): --
dc.identifier.issn3043843-
dc.identifier.urihttps://doi.org/10.1007/s10751-019-1582-y-
dc.identifier.urihttp://repository.iitr.ac.in/handle/123456789/13464-
dc.description.abstractIn the present work, we have reported shell model results for open shell nuclei Ne, Mg and Si isotopes with 10 ≤ N ≤ 20 in sd-shell model space. We have performed calculations in sd shell with two ab initio approaches: in-medium similarity renormalization group (IM-SRG) and coupled-cluster (CC) theory. We have also performed calculations with phenomenological USDB interaction and chiral effective field theory based CEFT interaction. The results for rotational spectra and B(E2;21+→01+) transitions are reported for even-mass isotopes. The IM-SRG and CC results are in reasonable agreement with the experimental data except at N = 20. This demonstrates a validity of ab initio description of deformation for doubly open-shell nuclei for sd shell. To see the importance of pf orbitals, we have also compared our results with SDPF-MU interaction by taking account of 2p − 2h and 4p − 4h configurations in sd-pf -shell model space. © 2019, Springer Nature Switzerland AG.-
dc.language.isoen_US-
dc.publisherSpringer International Publishing-
dc.relation.ispartofHyperfine Interactions-
dc.subjectCollectivity-
dc.subjectEffective interactions-
dc.subjectIsland of inversion-
dc.subjectShell model-
dc.titleAb initio description of collectivity for sd shell nuclei-
dc.typeArticle-
dc.scopusid57209145804-
dc.scopusid57208748522-
dc.scopusid57197697623-
dc.scopusid57208202387-
dc.scopusid7409091140-
dc.affiliationSaxena, A., Department of Physics, Indian Institute of Technology, Roorkee, 247667, India-
dc.affiliationKumar, A., Department of Physics, Indian Institute of Technology, Roorkee, 247667, India-
dc.affiliationKumar, V., Department of Physics, Central University of Kashmir, Ganderbal, 191201, India-
dc.affiliationSrivastava, P.C., Department of Physics, Indian Institute of Technology, Roorkee, 247667, India-
dc.affiliationSuzuki, T., Department of Physics, College of Humanities and Science, Nihon Univerity, Sakurajosui 3, Setagaya-ku, Tokyo, 156-8550, Japan, National Astronomical Observatory of Japan, Osawa 2, Mitaka, Tokyo, 181-8588, Japan-
dc.description.fundingAcknowledgments AS acknowledges financial support from MHRD (Govt. of India) for her Ph.D. thesis work. Vikas Kumar acknowledges partial support from CUK.-
dc.description.correspondingauthorSaxena, A.; Department of Physics, Indian Institute of TechnologyIndia; email: asaxena@ph.iitr.ac.in-
Appears in Collections:Journal Publications [PH]

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