002790638 001__ 2790638
002790638 003__ SzGeCERN
002790638 005__ 20211123142542.0
002790638 0247_ $$2DOI$$9APS$$a10.1103/PhysRevC.104.L051301$$qpublication
002790638 0248_ $$aoai:cds.cern.ch:2790638$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002790638 035__ $$9https://inspirehep.net/api/oai2d$$aoai:inspirehep.net:1965952$$d2021-11-15T15:23:39Z$$h2021-11-16T05:00:05Z$$mmarcxml
002790638 035__ $$9Inspire$$a1965952
002790638 041__ $$aeng
002790638 100__ $$aMacGregor, P T$$uManchester U.
002790638 245__ $$9APS$$aEvolution of single-particle structure near the $N=20$ island of inversion
002790638 246__ $$9APS$$aEvolution of single-particle structure near the N=20 island of inversion
002790638 260__ $$c2021
002790638 300__ $$a7 p
002790638 520__ $$9APS$$aThe single-particle properties of $^{29}$Mg have been investigated via a measurement of the $^{28}$Mg(d,p) 29Mg reaction, in inverse kinematics, using the ISOLDE Solenoidal Spectrometer. The negative-parity intruder states from the f p shell have been identified and used to benchmark modern shell-model calculations. The systematic data on the single-particle centroids along the $N = 17$ isotones show good agreement with shell-model predictions in describing the observed trends from stability toward $^{25}$O. However, there is also evidence that the effect of the finite geometry of the nuclear potential is playing a role on the behavior of the p orbitals near the particle-emission threshold.
002790638 540__ $$3publication$$aCC BY 4.0$$uhttps://creativecommons.org/licenses/by/4.0/
002790638 542__ $$3publication$$dauthors$$g2021
002790638 65017 $$2SzGeCERN$$aNuclear Physics - Experiment
002790638 690C_ $$aARTICLE
002790638 690C_ $$aCERN
002790638 693__ $$aCERN ISOLDE
002790638 700__ $$aSharp, D K$$uManchester U.
002790638 700__ $$aFreeman, S J$$uManchester U.
002790638 700__ $$aHoffman, C R$$uArgonne, PHY
002790638 700__ $$aKay, B P$$uArgonne, PHY
002790638 700__ $$aTang, T L$$uArgonne, PHY
002790638 700__ $$aGaffney, L P$$uLiverpool U.$$uCERN$$vCERN, CH-1211 Geneva 23, Switzerland
002790638 700__ $$aBaader, E F$$uCERN
002790638 700__ $$aBorge, M J G$$uMadrid, Inst. Estructura Materia
002790638 700__ $$aButler, P A$$uLiverpool U.
002790638 700__ $$aCatford, W N$$uSurrey U.
002790638 700__ $$aCropper, B D$$uManchester U.
002790638 700__ $$ade Angelis, G$$uINFN, Legnaro
002790638 700__ $$aKonki, J$$uCERN
002790638 700__ $$aKröll, Th$$uDarmstadt, Tech. Hochsch.
002790638 700__ $$aLabiche, M$$uDaresbury
002790638 700__ $$aLazarus, I H$$uDaresbury
002790638 700__ $$aLubna, R S$$uTRIUMF$$uFlorida State U.$$vDepartment of Physics, Florida State University, Tallahassee, Florida 32306, USA
002790638 700__ $$aMartel, I$$uLiverpool U.$$uHuelva U.$$vUniversidad de Huelva, 21071 Huelva, Spain
002790638 700__ $$aMcNeel, D G$$uConnecticut U.
002790638 700__ $$aPage, R D$$uLiverpool U.
002790638 700__ $$aPoleshchuk, O$$uLeuven U.
002790638 700__ $$aRaabe, R$$uLeuven U.
002790638 700__ $$aRecchia, F$$uPadua U.$$uINFN, Padua$$vINFN Sezione di Padova, Padova 35131, Italy
002790638 700__ $$aYang, J$$uLeuven U.
002790638 773__ $$cL051301$$mpublication$$n5$$pPhys. Rev. C$$v104$$y2021
002790638 8564_ $$82337132$$s586656$$uhttps://cds.cern.ch/record/2790638/files/PhysRevC.104.L051301.pdf$$yFulltext
002790638 960__ $$a13
002790638 980__ $$aARTICLE