Näytä suppeat kuvailutiedot

dc.contributor.authorTonev, D.
dc.contributor.authorde Angelis, G.
dc.contributor.authorDeloncle, I.
dc.contributor.authorGoutev, N.
dc.contributor.authorDe Gregorio, G.
dc.contributor.authorPavlov, P.
dc.contributor.authorPantaleev, I.L.
dc.contributor.authorIliev, S.
dc.contributor.authorYavahchova, M.S.
dc.contributor.authorBizzeti, P.G.
dc.contributor.authorDemerdjiev, A.
dc.contributor.authorDimitrov, D.T.
dc.contributor.authorFarnea, E.
dc.contributor.authorGadea, A.
dc.contributor.authorGeleva, E.
dc.contributor.authorHe, C.Y.
dc.contributor.authorLaftchiev, H.
dc.contributor.authorLenzi, S.M.
dc.contributor.authorLunardi, S.
dc.contributor.authorMarginean, N.
dc.contributor.authorMenegazzo, R.
dc.contributor.authorNapoli, D.R.
dc.contributor.authorNowacki, F.
dc.contributor.authorOrlandi, R.
dc.contributor.authorPenttilä, H.
dc.contributor.authorRecchia, F.
dc.contributor.authorSahin, E.
dc.contributor.authorSingh, R.P.
dc.contributor.authorStoyanova, M.
dc.contributor.authorUr, C.A.
dc.contributor.authorWirth, H.-F.
dc.date.accessioned2021-09-20T04:57:36Z
dc.date.available2021-09-20T04:57:36Z
dc.date.issued2021
dc.identifier.citationTonev, D., de Angelis, G., Deloncle, I., Goutev, N., De Gregorio, G., Pavlov, P., Pantaleev, I.L., Iliev, S., Yavahchova, M.S., Bizzeti, P.G., Demerdjiev, A., Dimitrov, D.T., Farnea, E., Gadea, A., Geleva, E., He, C.Y., Laftchiev, H., Lenzi, S.M., Lunardi, S., . . . Wirth, H.-F. (2021). Transition probabilities in 31P and 31S : A test for isospin symmetry. <i>Physics Letters B</i>, <i>821</i>, Article 136603. <a href="https://doi.org/10.1016/j.physletb.2021.136603" target="_blank">https://doi.org/10.1016/j.physletb.2021.136603</a>
dc.identifier.otherCONVID_100342730
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/77833
dc.description.abstractExcited states in the mirror nuclei 31P and 31S were populated in the 1p and 1n exit channels of the reaction 20Ne + 12C, at a beam energy of 33 MeV. The 20Ne beam was delivered for the first time by the Piave-Alpi accelerator of the Laboratori Nazionali di Legnaro. Angular correlations of coincident γ-rays and Doppler-shift attenuation lifetime measurements were performed using the multi-detector array GASP in conjunction with the EUCLIDES charged particle detector. In the observed B(E1) strengths, the isoscalar component, amounting to 24% of the isovector one, provides strong evidence for breaking of the isospin symmetry in the mass region. Self-consistent beyond mean field calculations using Equation of Motion method based on a chiral potential and including two- and three-body forces reproduce well the experimental B(E1) strengths, reinforcing our conclusion. Coherent mixing from higher-lying states involving the Giant Isovector Monopole Resonance accounts well for the effect observed. The breaking of the isospin symmetry originates from the violation of the charge symmetry of the two- and three-body parts of the potential, only related to the Coulomb interaction.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.subject.othermirror nuclei
dc.subject.otherlifetime measurements
dc.subject.othertransition probabilities
dc.subject.otherisospin symmetry
dc.subject.othermicroscopic multiphonon model
dc.titleTransition probabilities in 31P and 31S : A test for isospin symmetry
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202109204908
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.issn0370-2693
dc.relation.volume821
dc.type.versionpublishedVersion
dc.rights.copyright© 2021 Published by Elsevier B.V. Funded by SCOAP3
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2021.136603
jyx.fundinginformationThis research has been supported by the Bulgarian Science Fund under Contract No. 08/6, 13.12.2016. A. D. and E. G. are grateful to the National Post-doctoral students and young scientists program, funded by the Bulgarian Ministry of Education and Science.
dc.type.okmA1


Aineistoon kuuluvat tiedostot

Thumbnail

Aineisto kuuluu seuraaviin kokoelmiin

Näytä suppeat kuvailutiedot

CC BY 4.0
Ellei muuten mainita, aineiston lisenssi on CC BY 4.0