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dc.contributor.authorNovikov, K.
dc.contributor.authorHarca, I.M.
dc.contributor.authorKozulin, E.M.
dc.contributor.authorDmitriev, S.
dc.contributor.authorItkis, J.
dc.contributor.authorKnyazheva, G.
dc.contributor.authorLoktev, T.
dc.contributor.authorCorradi, L.
dc.contributor.authorValiente-Dobon, J.
dc.contributor.authorFioretto, E.
dc.contributor.authorMontanari, D.
dc.contributor.authorStefanini, A.M.
dc.contributor.authorVardaci, E.
dc.contributor.authorQuero, D.
dc.contributor.authorMontagnoli, G.
dc.contributor.authorScarlassara, F.
dc.contributor.authorStrano, E.
dc.contributor.authorPollarolo, G.
dc.contributor.authorPiot, J.
dc.contributor.authorMijatovi`c, T.
dc.contributor.authorSzilner, S.
dc.contributor.authorAckermann, D.
dc.contributor.authorChubarian, G.
dc.contributor.authorTrzaska, Wladyslaw
dc.date.accessioned2016-08-29T07:00:43Z
dc.date.available2016-08-29T07:00:43Z
dc.date.issued2016
dc.identifier.citationNovikov, K., Harca, I. M., Kozulin, E. M., Dmitriev, S., Itkis, J., Knyazheva, G., . . . Trzaska, W. (2016). The study of neutron-rich nuclei production in the region of the closed shell N=126 in the multi-nucleon transfer reaction 136Xe+208Pb. In <em>8th European Summer School on Experimental Nuclear Astrophysics (Santa Tecla School)</em> (pp. 012020). Journal of Physics: Conference Series, 703. Institute of Physics Publishing Ltd.. <a href="http://dx.doi.org/10.1088/1742-6596/703/1/012020">doi:10.1088/1742-6596/703/1/012020</a>
dc.identifier.otherTUTKAID_70784
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/51098
dc.description.abstractThe unexplored area of heavy neutron rich nuclei is extremely important for nuclear astrophysics investigations and, in particular, for the understanding of the r-process of astrophysical nucleogenesis. For the production of heavy neutron rich nuclei located along the neutron closed shell N=126 (probably the last ”waiting point” in the r-process of nucleosynthesis) the low-energy multi-nucleon transfer reaction 136Xe+208Pb at Elab=870MeV was explored. Due to the stabilizing effect of the closed neutron shells in both nuclei, N=82 and N=126, and the rather favorable proton transfer from lead to xenon, the light fragments formed in this process are well bound and the Q-value of the reaction is nearly zero. Measurements were performed with the PRISMA spectrometer in coincidence with an additional time-of-flight (ToF) arm on the +20 beam line of the PIAVE-ALPI accelerator in Legnaro, Italy. The PRISMA spectrometer allows identification of the A, Z and velocity of the projectile-like fragments (PLF), while the second arm gives access to the target-like fragments (TLF). Details on the experimental setup and preliminary results are reported.
dc.language.isoeng
dc.publisherInstitute of Physics Publishing Ltd.
dc.relation.ispartof8th European Summer School on Experimental Nuclear Astrophysics (Santa Tecla School)
dc.relation.ispartofseriesJournal of Physics: Conference Series;703
dc.subject.otherchemical elements
dc.subject.otherneutron beams
dc.subject.otherspectrometers
dc.subject.otherbeam lines
dc.subject.otherclosed shells
dc.subject.otherneutron shells
dc.subject.otherneutron-rich nuclei
dc.subject.othernuclear astro-physics
dc.subject.othertime of flight
dc.titleThe study of neutron-rich nuclei production in the region of the closed shell N=126 in the multi-nucleon transfer reaction 136Xe+208Pb
dc.typeconferenceObject
dc.identifier.urnURN:NBN:fi:jyu-201608013708
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/ConferencePaper
dc.date.updated2016-08-01T12:15:06Z
dc.type.coarconference paper
dc.description.reviewstatuspeerReviewed
dc.relation.issn1742-6588
dc.type.versionpublishedVersion
dc.rights.copyright© Published under licence by IOP Publishing Ltd. This is an open access article distributed under the terms of the Creative Commons Attribution (CC BY) licence.
dc.rights.accesslevelopenAccessfi
dc.rights.urlhttp://creativecommons.org/licenses/by/3.0/
dc.relation.doi10.1088/1742-6596/703/1/012020


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© Published under licence by IOP Publishing Ltd. This is an open access article distributed under the terms of the Creative Commons Attribution (CC BY) licence.
Except where otherwise noted, this item's license is described as © Published under licence by IOP Publishing Ltd. This is an open access article distributed under the terms of the Creative Commons Attribution (CC BY) licence.