Competition between fusion and quasifission in the angular momentum dependent dynamics of heavy element synthesis reactions

dc.contributor.authorTanaka, T.
dc.contributor.authorHinde, David
dc.contributor.authorDasgupta, M.
dc.contributor.authorWilliams, E.
dc.contributor.authorVo-Phuoc, K.
dc.contributor.authorSimenel, C.
dc.contributor.authorSimpson, E. C.
dc.contributor.authorJeung, D. Y.
dc.contributor.authorP. Carter, I.
dc.contributor.authorCook, K. J.
dc.contributor.authorLobanov, N. R.
dc.contributor.authorLuong, D. H.
dc.contributor.authorPalshetkar, C.
dc.contributor.authorRafferty, D. C.
dc.contributor.authorRamachandran, K.
dc.date.accessioned2024-07-26T01:43:15Z
dc.date.available2024-07-26T01:43:15Z
dc.date.issued2023
dc.description.abstractBackground: Mass and angle distribution measurements have illuminated many aspects of the physical variables controlling quasifission. However, mapping from detection angle to reaction time is clouded by the wide range of contributing angular momenta L h̄, ranging from 0h̄ to the maximum of the reaction ( 100h̄), which complicates the mapping, and thus limits our understanding of the reaction dynamics. Purpose: To investigate the angular momentum dependence of the reaction dynamics in quasifission and determine the fission fragment mass evolutions in the reaction. Method: The mass and angular distributions of products of the reactions 52 Cr + 198 Pt and 54 Cr + 196 Pt were measured. The distributions were compared with quasifission simulation results. Results: Mass angle distributions are reproduced by utilizing a new quasifission mass evolution model, and including a mass-symmetric component associated with low L. The latter increases in yield at higher beam energy. Conclusions: The symmetric component represents the total of slow quasifission and fusion-fission. The increase in contribution with energy above the Coulomb barrier suggests that an extra-push energy is required to achieve fusion.
dc.description.sponsorshipThe authors acknowledge the Australian Research Council for support through Discovery Grants No. DP200100601, No. DP190100256, No. DP190101442, No. DP170102318, and No. DE140100784. Financial support from the NCRIS HIA capability for operation of the Heavy Ion Accelerator Facility is acknowledged. The authors thank T. Kibédi for his key role in operation of the Linac
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2469-9985
dc.identifier.urihttps://hdl.handle.net/1885/733714207
dc.language.isoen_AUen_AU
dc.publisherAmerican Physical Society
dc.relationhttp://purl.org/au-research/grants/arc/DP200100601
dc.relationhttp://purl.org/au-research/grants/arc/DP190100256
dc.relationhttp://purl.org/au-research/grants/arc/DP190101442
dc.relationhttp://purl.org/au-research/grants/arc/DP170102318
dc.rights© 2023 American Physical Society
dc.sourcePhysical Review C
dc.subjectNuclear physics
dc.titleCompetition between fusion and quasifission in the angular momentum dependent dynamics of heavy element synthesis reactions
dc.typeJournal article
dcterms.dateAccepted2023
dspace.entity.typePublication
local.bibliographicCitation.lastpage054601-12
local.bibliographicCitation.startpage054601-1
local.contributor.affiliationTanaka, T., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationHinde, D. Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationDasgupta, M., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationWilliams, E., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationVo-Phuoc, K., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationSimenel, C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationSimpson, E. C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationJeung, D. Y., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationCarter, I. P., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationCook, K. J., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationLobanov, N. R., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationLuong, D. H., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationPalshetkar, C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationRafferty, D. C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationRamachandran, K., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.authoremaildavid.hinde@anu.edu.au
local.contributor.authoruidu8203491
local.description.embargo2099-12-31
local.identifier.absfor510601 - Nuclear physics
local.identifier.ariespublicationa383154xPUB42029
local.identifier.doi10.1103/PhysRevC.107.054601
local.identifier.uidSubmittedByu5633413
local.publisher.urlhttps://journals.aps.org/prc/abstract/10.1103/PhysRevC.107.054601
local.type.statusPublished Version
publicationvolume.volumeNumber107

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