Näytä suppeat kuvailutiedot

dc.contributor.authorDanilov, A.N.
dc.contributor.authorDemyanova, A.S.
dc.contributor.authorOgloblin, A.A.
dc.contributor.authorBelyaeva, T.L.
dc.contributor.authorGoncharov, S.A.
dc.contributor.authorTrzaska, Wladyslaw
dc.contributor.editorGreco, V.
dc.contributor.editorCognata, M. La
dc.contributor.editorPirrone, S.
dc.contributor.editorRizzo, F.
dc.contributor.editorSpitaleri, C.
dc.date.accessioned2016-07-12T10:50:51Z
dc.date.available2016-07-12T10:50:51Z
dc.date.issued2016
dc.identifier.citationDanilov, A.N., Demyanova, A.S., Ogloblin, A.A., Belyaeva, T.L., Goncharov, S.A., & Trzaska, W. (2016). Cluster rotational bands in 11B. In V. Greco, M. L. Cognata, S. Pirrone, F. Rizzo, & C. Spitaleri (Eds.), <i>NN2015 : 12th International Conference on Nucleus-Nucleus Collisions 2015</i> (Article 04011). EDP Sciences. EPJ Web of Conferences, 117. <a href="https://doi.org/10.1051/epjconf/201611704011" target="_blank">https://doi.org/10.1051/epjconf/201611704011</a>
dc.identifier.otherCONVID_26114116
dc.identifier.otherTUTKAID_70638
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/50805
dc.description.abstractDifferential cross-sections of 11B+α inelastic scattering at E(α) = 65 MeV leading to most of the known 11B states at excitation energies up to 14 MeV were measured [1]. The data analysis was done using Modified diffraction model (MDM) [2] allowing determining radii of excited states. Radii of the states with excitation energies less than ∼ 7 MeV coincide with the radius of the ground state with an accuracy not less than 0.1 - 0.15 fm. This result is consistent with traditional view on shell structure of low-lying states in 11B. Most of the observed high-energy excited states are distributed among four rotational bands. Moments of inertia of band states are close to the moment of inertia of the Hoyle state of 12C. The calculated radii, related to these bands, are 0.7 - 1.0 fm larger than the radius of the ground state, and are close to the Hoyle state radius. These results are in agreement with existing predictions about various cluster structure of 11B at high excitation energies.
dc.language.isoeng
dc.publisherEDP Sciences
dc.relation.ispartofNN2015 : 12th International Conference on Nucleus-Nucleus Collisions 2015
dc.relation.ispartofseriesEPJ Web of Conferences
dc.subject.otherrotational bands
dc.subject.othercluster structure
dc.titleCluster rotational bands in 11B
dc.typeconferenceObject
dc.identifier.urnURN:NBN:fi:jyu-201607123573
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/ConferencePaper
dc.date.updated2016-07-12T09:15:03Z
dc.relation.isbn978-88-7438-101-2
dc.type.coarconference paper
dc.description.reviewstatuspeerReviewed
dc.relation.issn2100-014X
dc.type.versionpublishedVersion
dc.rights.copyright© The Authors, published by EDP Sciences SIF. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0.
dc.rights.accesslevelopenAccessfi
dc.relation.conferenceInternational Conference on Nucleus-Nucleus Collisions
dc.subject.ysoboori
jyx.subject.urihttp://www.yso.fi/onto/yso/p7591
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1051/epjconf/201611704011


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Näytä suppeat kuvailutiedot

© The Authors, published by EDP Sciences SIF. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0.
Ellei muuten mainita, aineiston lisenssi on © The Authors, published by EDP Sciences SIF. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0.