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Valence 1s-0d proton vacancy of the <sup>32</sup>Si ground state

dc.contributor.authorWatwood, N.en
dc.contributor.authorHoffman, C. R.en
dc.contributor.authorKay, B. P.en
dc.contributor.authorTolstukhin, I. A.en
dc.contributor.authorChen, J.en
dc.contributor.authorTang, T. L.en
dc.contributor.authorBazin, D.en
dc.contributor.authorAyyad, Y.en
dc.contributor.authorBeceiro-Novo, S.en
dc.contributor.authorFreeman, S. J.en
dc.contributor.authorGaffney, L. P.en
dc.contributor.authorGarg, R.en
dc.contributor.authorJayatissa, H.en
dc.contributor.authorKuchera, A. N.en
dc.contributor.authorMacGregor, P. T.en
dc.contributor.authorMitchell, A. J.en
dc.contributor.authorMuñoz-Ramos, A.en
dc.contributor.authorMüller-Gatermann, C.en
dc.contributor.authorRecchia, F.en
dc.contributor.authorSantamaria, C.en
dc.contributor.authorSerikow, M. Z.en
dc.contributor.authorSharp, D. K.en
dc.contributor.authorWilson, G. L.en
dc.contributor.authorWuosmaa, A. H.en
dc.contributor.authorZamora, J. C.en
dc.date.accessioned2026-06-11T08:41:17Z
dc.date.available2026-06-11T08:41:17Z
dc.date.issued2025-11-05en
dc.description.abstractThe 32Si(3He,d) 33P reaction was studied in inverse kinematics at 6.3 MeV/u. States in 33P corresponding to the proton 1s-0d single-particle orbitals were identified up to ≈ 4.5 MeV in excitation energy. The (3He,d) spectroscopic factors were determined from distorted-wave Born approximation calculations. When combined with complementary neutron-adding data, the 1s-0d proton vacancies in the 32Si ground state were extracted. In conjunction with a reanalysis of data from previous single-particle measurements, the trends in proton and neutron vacancy were explored across the 28,30,32,34Si isotopes. Both proton and neutron vacancy data show gradual changes in their occupancies. The proton 1s1/2 orbitals in 32Si and 34Si are both consistent with being empty. The ground-state nucleon distributions are described by shell-model calculations constrained to the 1s-0d model space.en
dc.description.sponsorshipThis work was supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Contracts No. DE-AC02-06CH11357 (Argonne) and No. DE-SC0014552, by the UK Science and Technology Facility Council via Grants No. ST/T004797/1, No. ST/V001116/1, and No. ST/Y000323/1, by the International Technology Center Pacific (ITC-PAC) under Contract No. FA520919PA138 and Australian Research Council Grant No. DP210101201, and by Grants No. RYC2020-030669 and No. PID2022-142557NA-I00 funded by MCIN/AEI/ 10.13039/501100011033, FSE+ and FEDER, UE. This material is based upon work supported by NSF’s National Superconducting Cyclotron Laboratory which was a major facility fully funded by the National Science Foundation under Award No. PHY-1565546; SOLARIS is funded by the DOE Office of Science under the FRIB Cooperative Agreement No. DE-SC0000661. J.C. was supported by the National Natural Science Foundation of China under Contracts No. 12475120 and No. 12435010. Y.A. is supported by Grants No. RYC2019-028438-I and No. PID2021-125995NA-I00 funded by MCIN/AEI/10.13039/501100011033 and by the Regional Government of Galicia under the program “Proyectos de ex-celencia” Grant No. ED431F 2022/13.en
dc.description.statusPeer-revieweden
dc.format.extent9en
dc.identifier.issn2469-9985en
dc.identifier.otherORCID:/0000-0002-6742-695X/work/217149932en
dc.identifier.scopus105026262922en
dc.identifier.urihttps://hdl.handle.net/1885/733810522
dc.language.isoenen
dc.rightsPublisher Copyright: ©2025 American Physical Societyen
dc.sourcePhysical Review Cen
dc.titleValence 1s-0d proton vacancy of the <sup>32</sup>Si ground stateen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage9en
local.bibliographicCitation.startpage1en
local.contributor.affiliationWatwood, N.; Argonne National Laboratoryen
local.contributor.affiliationHoffman, C. R.; Argonne National Laboratoryen
local.contributor.affiliationKay, B. P.; Argonne National Laboratoryen
local.contributor.affiliationTolstukhin, I. A.; Argonne National Laboratoryen
local.contributor.affiliationChen, J.; Southern University of Science and Technologyen
local.contributor.affiliationTang, T. L.; Argonne National Laboratoryen
local.contributor.affiliationBazin, D.; Michigan State Universityen
local.contributor.affiliationAyyad, Y.; University of Santiago de Compostelaen
local.contributor.affiliationBeceiro-Novo, S.; University of A Corunaen
local.contributor.affiliationFreeman, S. J.; University of Manchesteren
local.contributor.affiliationGaffney, L. P.; University of Liverpoolen
local.contributor.affiliationGarg, R.; Michigan State Universityen
local.contributor.affiliationJayatissa, H.; Argonne National Laboratoryen
local.contributor.affiliationKuchera, A. N.; Davidson Collegeen
local.contributor.affiliationMacGregor, P. T.; University of Manchesteren
local.contributor.affiliationMitchell, A. J.; The Australian National Universityen
local.contributor.affiliationMuñoz-Ramos, A.; University of Santiago de Compostelaen
local.contributor.affiliationMüller-Gatermann, C.; Argonne National Laboratoryen
local.contributor.affiliationRecchia, F.; University of Paduaen
local.contributor.affiliationSantamaria, C.; Morgan State Universityen
local.contributor.affiliationSerikow, M. Z.; Michigan State Universityen
local.contributor.affiliationSharp, D. K.; University of Manchesteren
local.contributor.affiliationWilson, G. L.; Louisiana State Universityen
local.contributor.affiliationWuosmaa, A. H.; University of Connecticuten
local.contributor.affiliationZamora, J. C.; Michigan State Universityen
local.identifier.citationvolume112en
local.identifier.doi10.1103/4lzs-mv3len
local.identifier.puredddf0921-545b-4fd0-aab1-9923fb75f7eeen
local.identifier.urlhttps://www.scopus.com/pages/publications/105026262922en
local.type.statusPublisheden

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