http://repository.iitr.ac.in/handle/123456789/13464
DC Field | Value | Language |
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dc.contributor.author | Saxena A. | - |
dc.contributor.author | Kumar A. | - |
dc.contributor.author | Kumar V. | - |
dc.contributor.author | Srivastava, Praveen Chandra | - |
dc.contributor.author | Suzuki T. | - |
dc.date.accessioned | 2020-10-15T12:34:28Z | - |
dc.date.available | 2020-10-15T12:34:28Z | - |
dc.date.issued | 2019 | - |
dc.identifier.citation | Hyperfine Interactions (2019), 240(1): - | - |
dc.identifier.issn | 3043843 | - |
dc.identifier.uri | https://doi.org/10.1007/s10751-019-1582-y | - |
dc.identifier.uri | http://repository.iitr.ac.in/handle/123456789/13464 | - |
dc.description.abstract | In 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.iso | en_US | - |
dc.publisher | Springer International Publishing | - |
dc.relation.ispartof | Hyperfine Interactions | - |
dc.subject | Collectivity | - |
dc.subject | Effective interactions | - |
dc.subject | Island of inversion | - |
dc.subject | Shell model | - |
dc.title | Ab initio description of collectivity for sd shell nuclei | - |
dc.type | Article | - |
dc.scopusid | 57209145804 | - |
dc.scopusid | 57208748522 | - |
dc.scopusid | 57197697623 | - |
dc.scopusid | 57208202387 | - |
dc.scopusid | 7409091140 | - |
dc.affiliation | Saxena, A., Department of Physics, Indian Institute of Technology, Roorkee, 247667, India | - |
dc.affiliation | Kumar, A., Department of Physics, Indian Institute of Technology, Roorkee, 247667, India | - |
dc.affiliation | Kumar, V., Department of Physics, Central University of Kashmir, Ganderbal, 191201, India | - |
dc.affiliation | Srivastava, P.C., Department of Physics, Indian Institute of Technology, Roorkee, 247667, India | - |
dc.affiliation | Suzuki, 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.funding | Acknowledgments AS acknowledges financial support from MHRD (Govt. of India) for her Ph.D. thesis work. Vikas Kumar acknowledges partial support from CUK. | - |
dc.description.correspondingauthor | Saxena, A.; Department of Physics, Indian Institute of TechnologyIndia; email: asaxena@ph.iitr.ac.in | - |
Appears in Collections: | Journal Publications [PH] |
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