Energy dependence of p+232 Th fission mass distributions: Mass-asymmetric standard I and standard II modes, and multichance fission
| dc.contributor.author | Berriman, A. C. | |
| dc.contributor.author | Hinde, David | |
| dc.contributor.author | Jeung, D. Y. | |
| dc.contributor.author | Dasgupta, M. | |
| dc.contributor.author | Haba, H. | |
| dc.contributor.author | Tanaka, T. | |
| dc.contributor.author | Banerjee, K. | |
| dc.contributor.author | Banerjee, T. | |
| dc.contributor.author | Bezzina, L. T. | |
| dc.contributor.author | Buete, J. | |
| dc.contributor.author | Cook, K. J. | |
| dc.contributor.author | Parker-Steele, S. | |
| dc.contributor.author | Sengupta, C. | |
| dc.contributor.author | Simenel, C. | |
| dc.contributor.author | Simpson, E. C. | |
| dc.contributor.author | Stoyer, M. A. | |
| dc.contributor.author | Swinton-Bland, B. M. A. | |
| dc.contributor.author | Williams, E. | |
| dc.date.accessioned | 2024-07-26T04:25:14Z | |
| dc.date.available | 2024-07-26T04:25:14Z | |
| dc.date.issued | 2022 | |
| dc.description.abstract | Background: 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.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 2469-9985 | |
| dc.identifier.uri | https://hdl.handle.net/1885/733714218 | |
| dc.language.iso | en_AU | en_AU |
| dc.publisher | American Physical Society | |
| dc.rights | © 2022 American Physical Society | |
| dc.source | Physical Review C (nuclear physics) | |
| dc.subject | Nuclear physics | |
| dc.title | Energy dependence of p+232 Th fission mass distributions: Mass-asymmetric standard I and standard II modes, and multichance fission | |
| dc.type | Journal article | |
| dcterms.dateAccepted | 2022 | |
| dspace.entity.type | Publication | |
| local.bibliographicCitation.lastpage | 064614-18 | |
| local.bibliographicCitation.startpage | 064614-1 | |
| local.contributor.affiliation | Berriman, A. C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Hinde, David, Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Jeung, D. Y., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Dasgupta, M., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Haba, H., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Tanaka, T., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Banerjee, K., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Banerjee, T., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Bezzina, L. T., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Buete, J., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Cook, K. J., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Parker-Steele, S., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Sengupta, C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Simenel, C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Simpson, E. C., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Stoyer, M. A., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Swinton-Bland, B. M. A., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.affiliation | Williams, E., Department of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University | |
| local.contributor.authoruid | david.hinde@anu.edu.au | |
| local.description.embargo | 2099-12-31 | |
| local.identifier.absfor | 510601 - Nuclear physics | |
| local.identifier.doi | 10.1103/PhysRevC.105.064614 | |
| local.publisher.url | https://journals.aps.org/prc/abstract/10.1103/PhysRevC.105.064614 | |
| publicationvolume.volumeNumber | 105 |