Exploring quasifission characteristics for ³⁴S+²³²Th forming ²⁶⁶Sg

dc.contributor.authorPrasad, E.
dc.contributor.authorWakhle, A.
dc.contributor.authorHinde, David
dc.contributor.authorWilliams, E.
dc.contributor.authorDasgupta, M.
dc.contributor.authorEvers, M.
dc.contributor.authorLuong, D. H.
dc.contributor.authorMohanto, G.
dc.contributor.authorSimenel, C.
dc.contributor.authorVo-Phuoc, K.
dc.date.accessioned2018-11-02T05:26:37Z
dc.date.available2018-11-02T05:26:37Z
dc.date.issued2016
dc.description.abstractBackground: Fission fragments from heavy ion collisions with actinide nuclei show mass-asymmetric and mass-symmetric components. The relative probabilities of these two components vary rapidly with beam energy with respect to the capture barrier, indicating a strong dependence on the alignment of the deformed nucleus with the partner in the collisions. Purpose: To study the characteristics of the mass-asymmetric quasifission component by reproducing the experimental mass-angle distributions to investigate mass evolution and sticking times. Methods: Fission fragment mass-angle distributions were measured for the 34S + 232Th reaction. Simulations to match the measurements were made by using a classical phenomenological approach. Mass ratio distributions and angular distributions of the mass-asymmetric quasifission component were simultaneously fit to constrain the free parameters used in the simulation. Results: The mass-asymmetric quasifission component—predominantly originating from tip (axial) collisions with the prolate deformed 232Th—is found to be peaked near A = 200 at all energies and center-of-mass angles. A Monte Carlo model using the standard mass equilibration time constant of 5.2 × 10−21 s predicts more symmetric mass splits. Three different hypotheses assuming (i) a mass halt at A = 200, (ii) a slower mass equilibration time, or (iii) a Fermi-type mass drift function reproduced the main experimental features. Conclusions:In tip collisions for the 34S + 232Th reaction, mass-asymmetric fission with A ∼ 200 is the dominant outcome. The average sticking time is found to be ∼7 × 10−21 s, independent of the scenario used for mass evolution.en_AU
dc.description.sponsorshipThe authors acknowledge support from the Australian Research Council through Grants No. FL110100098, No. FT120100760, No. DP130101569, No. DP140101337, and No. DE140100784. Support for accelerator operations through the NCRIS program is acknowledged.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2469-9985en_AU
dc.identifier.urihttp://hdl.handle.net/1885/148824
dc.publisherAmerican Physical Societyen_AU
dc.relationhttp://purl.org/au-research/grants/arc/FL110100098en_AU
dc.relationhttp://purl.org/au-research/grants/arc/FT120100760en_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP130101569en_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP140101337en_AU
dc.relationhttp://purl.org/au-research/grants/arc/DE140100784en_AU
dc.rights© 2016 American Physical Society. http://www.sherpa.ac.uk/romeo/issn/2469-9985/..."author can archive publisher's version/PDF" from SHERPA/RoMEO site (as at 2/11/18)en_AU
dc.sourcePhysical Review Cen_AU
dc.titleExploring quasifission characteristics for ³⁴S+²³²Th forming ²⁶⁶Sgen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2en_AU
local.bibliographicCitation.lastpage024607-14en_AU
local.bibliographicCitation.startpage024607-1en_AU
local.contributor.affiliationHinde, D., Research School of Physics & Engineering, The Australian National Universityen_AU
local.contributor.authoruidu8203491en_AU
local.identifier.citationvolume93en_AU
local.identifier.doi10.1103/PhysRevC.93.024607en_AU
local.publisher.urlhttps://www.aps.org/en_AU
local.type.statusPublished Versionen_AU

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