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Quasifission Dynamics in the Formation of Superheavy Elements

dc.contributor.authorHinde, D. J.en
dc.contributor.authorDasgupta, M.en
dc.contributor.authorJeung, D. Y.en
dc.contributor.authorMohanto, G.en
dc.contributor.authorPrasad, E.en
dc.contributor.authorSimenel, C.en
dc.contributor.authorWilliams, E.en
dc.contributor.authorCarter, I. P.en
dc.contributor.authorCook, K. J.en
dc.contributor.authorKalkal, Sunilen
dc.contributor.authorRafferty, D. C.en
dc.contributor.authorSimpson, E. C.en
dc.contributor.authorDavid, H. M.en
dc.contributor.authorDüllmann, Ch E.en
dc.contributor.authorKhuyagbaatar, J.en
dc.date.accessioned2025-06-10T11:36:14Z
dc.date.available2025-06-10T11:36:14Z
dc.date.issued2017-11-22en
dc.description.abstractSuperheavy elements are created through the fusion of two heavy nuclei. The large Coulomb energy that makes superheavy elements unstable also makes fusion forming a compact compound nucleus very unlikely. Instead, after sticking together for a short time, the two nuclei usually come apart, in a process called quasifission. Mass-angle distributions give the most direct information on the characteristics and time scales of quasifission. A systematic study of carefully chosen mass-angle distributions has provided information on the global trends of quasifission. Large deviations from these systematics at beam energies near the capture barrier reveal the major role played by the nuclear structure of the two colliding nuclei in determining the reaction outcome, and thus implicitly in hindering or favouring superheavy element synthesis.en
dc.description.sponsorship1Department of Nuclear Physics, Research School of Physics and Engineering, Australian National University, Canberra, ACT 2601, Australia 2GSI Helmholtzzentrum für Schwerionenforschung, D-64291 Darmstadt, Germany 3Helmholtz Institute Mainz, D-55099 Mainz, Germany 4Johannes Gutenberg Universität Mainz, D-55099 Mainz, Germanyen
dc.description.statusPeer-revieweden
dc.identifier.issn2101-6275en
dc.identifier.otherORCID:/0000-0002-7895-458X/work/161834903en
dc.identifier.otherORCID:/0000-0002-4595-0742/work/162291081en
dc.identifier.otherORCID:/0000-0002-5911-1333/work/162375717en
dc.identifier.otherORCID:/0000-0002-1677-9421/work/221768031en
dc.identifier.scopus85036645671en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=85036645671&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733757903
dc.language.isoenen
dc.relation.ispartofseriesFUSION 2017en
dc.rightsPublisher Copyright: © The Authors, published by EDP Sciences, 2017.en
dc.sourceEPJ Web of Conferencesen
dc.titleQuasifission Dynamics in the Formation of Superheavy Elementsen
dc.typeConference paperen
dspace.entity.typePublicationen
local.contributor.affiliationHinde, D. J.; School Administrative Support, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationDasgupta, M.; Gender Institute, Director Ias/Chair Board Ias, The Australian National Universityen
local.contributor.affiliationJeung, D. Y.; Non-Linear Physics Centre, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationMohanto, G.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationPrasad, E.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationSimenel, C.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationWilliams, E.; Gender Institute, Director Ias/Chair Board Ias, The Australian National Universityen
local.contributor.affiliationCarter, I. P.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationCook, K. J.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationKalkal, Sunil; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationRafferty, D. C.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationSimpson, E. C.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationDavid, H. M.; GSI Helmholtz Centre for Heavy Ion Researchen
local.contributor.affiliationDüllmann, Ch E.; GSI Helmholtz Centre for Heavy Ion Researchen
local.contributor.affiliationKhuyagbaatar, J.; GSI Helmholtz Centre for Heavy Ion Researchen
local.identifier.ariespublicationa383154xPUB9140en
local.identifier.citationvolume163en
local.identifier.doi10.1051/epjconf/201716300023en
local.identifier.pureb467bbbd-12a8-4d28-9ef2-37ac6a463765en
local.identifier.urlhttps://www.scopus.com/pages/publications/85036645671en
local.type.statusPublisheden

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