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dc.contributor.authorKozulin, E. M.
dc.contributor.authorKnyazheva, G. N.
dc.contributor.authorItkis, I. M.
dc.contributor.authorItkis, M. G.
dc.contributor.authorMukhamejanov, Y. S.
dc.contributor.authorBogachev, A. A.
dc.contributor.authorNovikov, K. V.
dc.contributor.authorKirakosyan, V. V.
dc.contributor.authorKumar, D.
dc.contributor.authorBanerjee, T.
dc.contributor.authorCheralu, M.
dc.contributor.authorMaiti, M.
dc.contributor.authorPrajapat, R.
dc.contributor.authorKumar, R.
dc.contributor.authorSarkar, G.
dc.contributor.authorTrzaska, W. H.
dc.contributor.authorAndreyev, A. N.
dc.contributor.authorHarca, I. M.
dc.contributor.authorMitu, A.
dc.contributor.authorVardaci, E.
dc.date.accessioned2022-02-28T09:34:24Z
dc.date.available2022-02-28T09:34:24Z
dc.date.issued2022
dc.identifier.citationKozulin, E. M., Knyazheva, G. N., Itkis, I. M., Itkis, M. G., Mukhamejanov, Y. S., Bogachev, A.A., Novikov, K. V., Kirakosyan, V.V., Kumar, D., Banerjee, T., Cheralu, M., Maiti, M., Prajapat, R., Kumar, R., Sarkar, G., Trzaska, W. H., Andreyev, A. N., Harca, I. M., Mitu, A., & Vardaci, E. (2022). Fission of 180,182,183Hg* and 178Pt* nuclei at intermediate excitation energies. <i>Physical Review C</i>, <i>105</i>(1), Article 014607. <a href="https://doi.org/10.1103/PhysRevC.105.014607" target="_blank">https://doi.org/10.1103/PhysRevC.105.014607</a>
dc.identifier.otherCONVID_104378553
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/79984
dc.description.abstractPurpose: The study of asymmetric and symmetric fission of 180,182,183Hg and 178Pt nuclei as a function of their excitation energy and isospin. Methods: Mass-energy distributions of fission fragments of 180Hg, 178Pt (two protons less than 180Hg), and 182Hg (two neutrons more than 180Hg) formed in the 36Ar+144Sm,142Nd, and 40Ca+142Nd reactions were measured at energies near and above the Coulomb barrier. Fission of 183Hg obtained in the reaction of 40Ca with 143Nd was also investigated to see if one extra neutron could lead to dramatic changes in the fission process due to the shape-staggering effect in radii, known in 183Hg. The measurements were performed with the double-arm time-of-flight spectrometer CORSET. Results: The observed peculiarities in the fission fragment mass-energy distributions for all studied nuclei may be explained by the presence of a symmetric fission mode and three asymmetric fission modes, manifested by the different total kinetic energies and fragment mass splits. The yield of symmetric mode grows with increasing excitation energy of compound nucleus. Conclusions: The investigated properties of asymmetric fission of 180,182,183Hg and 178Pt nuclei point out the existence of well-deformed proton shell at Z≈36 and a less deformed proton shell at Z ≈ 46.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.titleFission of 180,182,183Hg* and 178Pt* nuclei at intermediate excitation energies
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202202281708
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.issn2469-9985
dc.relation.numberinseries1
dc.relation.volume105
dc.type.versionpublishedVersion
dc.rights.copyright© 2022 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.subject.ysoplatina
dc.subject.ysofissio
dc.subject.ysoelohopea
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p12535
jyx.subject.urihttp://www.yso.fi/onto/yso/p18705
jyx.subject.urihttp://www.yso.fi/onto/yso/p14245
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.105.014607
jyx.fundinginformationThis work was supported by the joint Grant from the Russian Foundation for Basic Research (Grant No. 19-52-45023) and the Department of Science and Technology of the Ministry of Science and Technology of India (Grant No. INT/RUS/RFBR/387). A.N.A. was supported by the Grant from STFC (UK).
dc.type.okmA1


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