File:1-s2.0-S0370269318309614-main.pdf
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Français : It is well known that most actinides fission into fragments of unequal size. This contradicts liquid-drop-model theory from which symmetric fission is expected. The first attempt to understand this difference suggested that division leading to one of the fragments being near doubly magic 132Sn is favored by gain in binding energy. After the Strutinsky shell-correction method was developed an alternative idea that gained popularity was that the fission saddle might be lower for mass-asymmetric shapes and that this asymmetry was preserved until scission. Recently it was observed [Phys. Rev. Lett. 105 (2010) 252502] that 180Hg preferentially fissions asymmetrically in contradiction to the fragment-magic-shell expectation which suggested symmetric division peaked around 90Zr, with its magic neutron number Z=50, so it was presented as a “new type of asymmetric fission”. However, in a paper [Phys. Lett. B 34 (1971) 349] a “simple” microscopic mechanism behind the asymmetry of the actinide fission saddle points was proposed to be related to the coupling between levels of type [40ΛΩ] and [51ΛΩ]. The paper then generalizes this idea and made the remarkable prediction that analogous features could exist in other regions. In particular it was proposed that in the rare-earth region couplings between levels of type [30ΛΩ] and [41ΛΩ] would favor mass-asymmetric outer saddle shapes. In this picture the asymmetry of 180Hg is not a “new type of asymmetric fission” but of analogous origin as the asymmetry of actinide fission. This prediction has never been cited in the discussion of the recently observed fission asymmetries in the “new region of asymmetry”, in nuclear physics also referred to as the rare-earth region. We show by detailed analysis that the mechanism of the saddle asymmetry in the sub-Pb region is indeed the one predicted half a century ago. |
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https://www.sciencedirect.com/science/article/pii/S0370269318309614 https://doi.org/10.1016/j.physletb.2018.12.034 |
Author | T. Ichikawa and P. Möller |
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current | 20:14, 5 February 2022 | 1,239 × 1,652, 6 pages (2.95 MB) | Pamputt (talk | contribs) | Uploaded a work by T. Ichikawa and P. Möller from https://www.sciencedirect.com/science/article/pii/S0370269318309614 https://doi.org/10.1016/j.physletb.2018.12.034 with UploadWizard |
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Publisher | Elsevier B.V. |
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Software used | Elsevier |
File change date and time | 17:45, 25 February 2019 |
Date and time of digitizing | 17:45, 25 February 2019 |
Date metadata was last modified | 17:45, 25 February 2019 |
Copyright status | Copyrighted |
Identifier | doi:10.1016/j.physletb.2018.12.034 |
Conversion program | Acrobat Distiller 9.5.5 (Windows) |
Encrypted | no |
Page size | 595.276 x 793.701 pts |
Version of PDF format | 1.7 |
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10 February 2019
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