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Energy dependence of p+232 Th fission mass distributions: Mass-asymmetric standard I and standard II modes, and multichance fission

dc.contributor.authorBerriman, A. C.
dc.contributor.authorHinde, David
dc.contributor.authorJeung, D. Y.
dc.contributor.authorDasgupta, M.
dc.contributor.authorHaba, H.
dc.contributor.authorTanaka, T.
dc.contributor.authorBanerjee, K.
dc.contributor.authorBanerjee, T.
dc.contributor.authorBezzina, L. T.
dc.contributor.authorBuete, J.
dc.contributor.authorCook, K. J.
dc.contributor.authorParker-Steele, S.
dc.contributor.authorSengupta, C.
dc.contributor.authorSimenel, C.
dc.contributor.authorSimpson, E. C.
dc.contributor.authorStoyer, M. A.
dc.contributor.authorSwinton-Bland, B. M. A.
dc.contributor.authorWilliams, E.
dc.date.accessioned2024-07-26T04:25:14Z
dc.date.available2024-07-26T04:25:14Z
dc.date.issued2022
dc.description.abstractBackground: The predominant mass-asymmetric fission of actinide nuclides occurs mainly through the so- called standard I and standard II modes. Though understood to be caused by shape-dependent shell structures encountered between the fission barrier deformation and scission, the most relevant shell gaps are still not firmly established. The standard I mode had been associated with the spherical doubly magic 132 Sn, and thus the Z = 50 proton shell, but recently it has been proposed that standard I and standard II are associated with quadrupole and octupole deformed gaps at Z = 52 and 56, respectively. Purpose: We investigate how the relative probabilities of the standard I and standard II modes vary with excitation energy near threshold, probing where the two modes bifurcate. Methods: The Australian National University Heavy Ion Accelerator Facility and CUBE fission spectrometer have been used to measure fission mass distributions for the p +232 Th reaction (forming 233 Pa) at closely spaced bombarding energy intervals from 6.5 to 28 MeV. Results: A model-independent analysis of the energy dependence of the shape of the mass-asymmetric peak shows a strong dependence of the standard I and standard II relative probability on excitation energy near threshold. Conclusions: The results are consistent with the standard II mode having a lower fission barrier than standard I in 233 Pa, with the latter increasing continually in relative probability above its barrier energy. It is concluded that multichance fission, in particular last chance fission, plays a strong role in determining the observed energy dependence of all fission modes.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2469-9985
dc.identifier.urihttps://hdl.handle.net/1885/733714218
dc.language.isoen_AUen_AU
dc.publisherAmerican Physical Society
dc.rights© 2022 American Physical Society
dc.sourcePhysical Review C (nuclear physics)
dc.subjectNuclear physics
dc.titleEnergy dependence of p+232 Th fission mass distributions: Mass-asymmetric standard I and standard II modes, and multichance fission
dc.typeJournal article
dcterms.dateAccepted2022
dspace.entity.typePublication
local.bibliographicCitation.lastpage064614-18
local.bibliographicCitation.startpage064614-1
local.contributor.affiliationBerriman, A. C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationHinde, David, 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.affiliationDasgupta, M., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationHaba, H., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationTanaka, T., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationBanerjee, K., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationBanerjee, T., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationBezzina, L. T., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationBuete, J., 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.affiliationParker-Steele, S., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationSengupta, C., 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.affiliationStoyer, M. A., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University
local.contributor.affiliationSwinton-Bland, B. M. A., 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.authoruiddavid.hinde@anu.edu.au
local.description.embargo2099-12-31
local.identifier.absfor510601 - Nuclear physics
local.identifier.doi10.1103/PhysRevC.105.064614
local.publisher.urlhttps://journals.aps.org/prc/abstract/10.1103/PhysRevC.105.064614
publicationvolume.volumeNumber105

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