Exploring quasifission characteristics for ³⁴S+²³²Th forming ²⁶⁶Sg
| dc.contributor.author | Prasad, E. | |
| dc.contributor.author | Wakhle, A. | |
| dc.contributor.author | Hinde, David | |
| dc.contributor.author | Williams, E. | |
| dc.contributor.author | Dasgupta, M. | |
| dc.contributor.author | Evers, M. | |
| dc.contributor.author | Luong, D. H. | |
| dc.contributor.author | Mohanto, G. | |
| dc.contributor.author | Simenel, C. | |
| dc.contributor.author | Vo-Phuoc, K. | |
| dc.date.accessioned | 2018-11-02T05:26:37Z | |
| dc.date.available | 2018-11-02T05:26:37Z | |
| dc.date.issued | 2016 | |
| dc.description.abstract | Background: 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.sponsorship | The 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.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 2469-9985 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/148824 | |
| dc.publisher | American Physical Society | en_AU |
| dc.relation | http://purl.org/au-research/grants/arc/FL110100098 | en_AU |
| dc.relation | http://purl.org/au-research/grants/arc/FT120100760 | en_AU |
| dc.relation | http://purl.org/au-research/grants/arc/DP130101569 | en_AU |
| dc.relation | http://purl.org/au-research/grants/arc/DP140101337 | en_AU |
| dc.relation | http://purl.org/au-research/grants/arc/DE140100784 | en_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.source | Physical Review C | en_AU |
| dc.title | Exploring quasifission characteristics for ³⁴S+²³²Th forming ²⁶⁶Sg | en_AU |
| dc.type | Journal article | en_AU |
| dcterms.accessRights | Open Access | en_AU |
| local.bibliographicCitation.issue | 2 | en_AU |
| local.bibliographicCitation.lastpage | 024607-14 | en_AU |
| local.bibliographicCitation.startpage | 024607-1 | en_AU |
| local.contributor.affiliation | Hinde, D., Research School of Physics & Engineering, The Australian National University | en_AU |
| local.contributor.authoruid | u8203491 | en_AU |
| local.identifier.citationvolume | 93 | en_AU |
| local.identifier.doi | 10.1103/PhysRevC.93.024607 | en_AU |
| local.publisher.url | https://www.aps.org/ | en_AU |
| local.type.status | Published Version | en_AU |