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dc.contributor.authorNovikov, K. V.
dc.contributor.authorKozulin, E. M.
dc.contributor.authorKnyazheva, G. N.
dc.contributor.authorItkis, I. M.
dc.contributor.authorItkis, M. G.
dc.contributor.authorBogachev, A. A.
dc.contributor.authorDiatlov, I. N.
dc.contributor.authorCheralu, M.
dc.contributor.authorKumar, D.
dc.contributor.authorKozulina, N. I.
dc.contributor.authorPan, A. N.
dc.contributor.authorPchelintsev, I. V.
dc.contributor.authorVorobiev, I. V.
dc.contributor.authorTrzaska, W. H.
dc.contributor.authorHeinz, S.
dc.contributor.authorDevaraja, H. M.
dc.contributor.authorLommel, B.
dc.contributor.authorVardaci, E.
dc.contributor.authorSpinosa, S.
dc.contributor.authorDi Nitto, A.
dc.contributor.authorPulcini, A.
dc.contributor.authorKhlebnikov, S. V.
dc.contributor.authorSingh, Pushpendra P.
dc.contributor.authorSahoo, Rudra, N.
dc.contributor.authorGall, B.
dc.contributor.authorAsfari, Z.
dc.contributor.authorBorcea, C.
dc.contributor.authorHarca, I.
dc.contributor.authorFilipescu, D. M.
dc.date.accessioned2020-10-12T06:58:19Z
dc.date.available2020-10-12T06:58:19Z
dc.date.issued2020
dc.identifier.citationNovikov, K. V., Kozulin, E. M., Knyazheva, G. N., Itkis, I. M., Itkis, M. G., Bogachev, A.A., Diatlov, I. N., Cheralu, M., Kumar, D., Kozulina, N. I., Pan, A. N., Pchelintsev, I. V., Vorobiev, I. V., Trzaska, W. H., Heinz, S., Devaraja, H. M., Lommel, B., Vardaci, E., Spinosa, S., . . . Filipescu, D. M. (2020). Investigation of fusion probabilities in the reactions with 52,54Cr, 64Ni, and 68Zn ions leading to the formation of Z = 120 superheavy composite systems. <i>Physical Review C</i>, <i>102</i>(4), Article 044605. <a href="https://doi.org/10.1103/PhysRevC.102.044605" target="_blank">https://doi.org/10.1103/PhysRevC.102.044605</a>
dc.identifier.otherCONVID_42419250
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/72098
dc.description.abstractBackground: The formation of superheavy nuclei in fusion reactions is suppressed by a competing quasifission process. The competition between the formation of the compound nucleus and the quasifission depends strongly on the reaction entrance channel. Purpose: The investigation of fission and quasifission processes in the formation of Z=120 superheavy composite systems in the 52,54Cr+248Cm and 68Zn+232Th reactions, and their comparison with the 64Ni+238U reaction at energies in the vicinity of the Coulomb barrier. Methods: Mass-energy distributions of fissionlike fragments formed in the reactions 52,54Cr+248Cm and 68Zn+232Th at energies near the Coulomb barrier were measured using the double-arm time-of-flight spectrometer CORSET. Results: Capture cross sections for the reactions under investigation were measured. The most probable fragment masses and total kinetic energies as well as their variances in dependence on the interaction energy were studied for asymmetric and symmetric fragments. The fusion probabilities were estimated from the analysis of mass-energy distributions. Conclusions: The estimated fusion probability drops down by a factor of 103 in the 54Cr+248Cm reaction compared to the reactions of 48Ca ions with actinides. Among the studied reactions, the 54Cr+248Cm is the most favorable one for the production of the superheavy element with Z=120.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.subject.otherlow and intermediate energy heavy-ion reactions
dc.subject.othernuclear fusion
dc.titleInvestigation of fusion probabilities in the reactions with 52,54Cr, 64Ni, and 68Zn ions leading to the formation of Z = 120 superheavy composite systems
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202010126157
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries4
dc.relation.volume102
dc.type.versionpublishedVersion
dc.rights.copyright©2020 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.subject.ysofuusioreaktio
dc.subject.ysofissio
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p19475
jyx.subject.urihttp://www.yso.fi/onto/yso/p18705
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.102.044605
jyx.fundinginformationThis work was supported by the joint grant from the Russian Scientific Foundation (Project No. 19-42-02014) and the Department of Science and Technology of the Ministry of Science and Technology of India (Ref. No. DST/INT/RUS/RSF/P-23), the mobility fund of the Academy of Finland, the Istituto Nazionale di Fisica Nucleare (Italy), and Deutsche Forschungsgemeinschaft DFG Grants No. HE 5469/3-1 and No. DE 2946/1-1.
dc.type.okmA1


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