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Fission Product Yield Data for the Transmutation of Minor Actinide ...

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fission barrier remains). Only in <strong>the</strong> fission <strong>of</strong><br />

226 Ra and 232 Th does asymmetric fission persist<br />

in predictions up to higher energies than<br />

found in experiments — possibly caused by<br />

<strong>the</strong> ra<strong>the</strong>r slow disappearance <strong>of</strong> <strong>the</strong><br />

asymmetric fission with increasing excitation<br />

energy or from a lack <strong>of</strong> symmetric fission<br />

contributions from neutron deficient nuclides.<br />

(b) Post-neutron emission mass yields —<br />

generally too narrow, with <strong>the</strong> heavy wing<br />

underestimated by an order <strong>of</strong> magnitude that<br />

may be related to an overestimation <strong>of</strong> <strong>the</strong><br />

post-scission neutron multiplicity. The model<br />

neglects <strong>the</strong> neutron evaporation between<br />

saddle and scission points, which leaves too<br />

much excitation energy within <strong>the</strong> fission<br />

fragments. Consequently, <strong>the</strong> heavier<br />

fragment, which receives a larger portion <strong>of</strong><br />

<strong>the</strong> excitation energy <strong>of</strong> <strong>the</strong> fissioning system,<br />

evaporates more neutrons than <strong>the</strong> light<br />

fragment, reducing <strong>the</strong> width <strong>of</strong> <strong>the</strong> final mass<br />

distribution. However, <strong>the</strong>re is evidence from<br />

a comparison with experiments that <strong>the</strong> prescission<br />

neutron multiplicity is not completely<br />

incorrect and <strong>the</strong> calculated temperature <strong>of</strong><br />

<strong>the</strong> fissioning system is not excessively high. A<br />

more likely explanation is that <strong>the</strong> fragments<br />

evaporate too many neutrons because <strong>of</strong> an<br />

underestimation <strong>of</strong> <strong>the</strong> energy required <strong>for</strong><br />

<strong>the</strong> emission <strong>of</strong> particles.<br />

5.1.3.7. Summary <strong>of</strong> <strong>the</strong> essential features<br />

<strong>of</strong> <strong>the</strong> new models and systematics<br />

The five systematic approaches are derived<br />

from fitting functions representing <strong>the</strong> different<br />

fission modes to <strong>the</strong> experimental data. Parameters<br />

were <strong>the</strong>n fitted by expressions that describe <strong>the</strong><br />

dependences <strong>of</strong> <strong>the</strong>se parameters on <strong>the</strong> system<br />

target plus projectile and excitation energy. One<br />

model was also explored in which <strong>the</strong> fission yields<br />

are calculated from nuclear fission <strong>the</strong>ory to derive<br />

fission mechanisms and yield distributions.<br />

Liu developed systematics solely <strong>for</strong> postneutron<br />

emission yields from neutron induced 238 U<br />

fission by means <strong>of</strong> a non-linear least squares<br />

analysis and correlation study <strong>of</strong> <strong>the</strong> experimental<br />

data. This systematics approach is based on experimental<br />

data adjusted <strong>for</strong> mass resolution.<br />

Katakura and Wahl have fitted <strong>the</strong> experimental<br />

data <strong>for</strong> actinide nuclei with 3 to 7<br />

Gaussians. They used neutron and proton induced<br />

244<br />

fission reactions, assuming reflection symmetry in<br />

<strong>the</strong> shape <strong>of</strong> <strong>the</strong> mass distribution around a point <strong>of</strong><br />

symmetry calculated from <strong>the</strong> compound nucleus<br />

mass minus <strong>the</strong> average total number <strong>of</strong> emitted<br />

post (Katakura) or pre + post (Wahl) scission<br />

neutrons. Katakura can only predict post-neutron<br />

emission mass distributions. Wahl has not included<br />

<strong>the</strong> extensive measurements <strong>of</strong> Zöller [5.4], and this<br />

omission may be responsible <strong>for</strong> <strong>the</strong> discrepancies<br />

<strong>of</strong> his predictions compared with o<strong>the</strong>rs at higher<br />

energies (50–160 MeV).<br />

Kibkalo’s phenomenological model was<br />

originally designed to study mass distribution<br />

dependences on transferred angular momentum <strong>for</strong><br />

different projectiles, and was later adapted <strong>for</strong><br />

predictions <strong>of</strong> fission yields. The systematics are<br />

similar to Katakura and Wahl, but without <strong>the</strong> prior<br />

calculation <strong>of</strong> a point <strong>of</strong> mass symmetry in <strong>the</strong> mass<br />

distribution.<br />

The approach <strong>of</strong> Zhdanov et al. differs from<br />

o<strong>the</strong>rs in several respects:<br />

(a) Experimental mass and energy distributions<br />

<strong>of</strong> fragments are analysed;<br />

(b) Expressions <strong>for</strong> <strong>the</strong> different fission modes do<br />

not include assumptions concerning <strong>the</strong><br />

shapes <strong>of</strong> <strong>the</strong> distributions;<br />

(c) Parameter values <strong>for</strong> <strong>the</strong> systematics were<br />

derived by minimizing <strong>the</strong> differences<br />

between experimental and calculated mass<br />

distributions;<br />

(d) Charlier’s peak functions were used in <strong>the</strong><br />

systematics to describe <strong>the</strong> shapes <strong>of</strong> <strong>the</strong><br />

asymmetric components.<br />

Duijvestijn’s predictions are based entirely on<br />

<strong>the</strong>oretical models <strong>for</strong> <strong>the</strong> fission mechanisms and<br />

yield distributions. The fission cross-sections and<br />

emissive fission contributions are calculated by<br />

means <strong>of</strong> a modelling code to obtain <strong>the</strong> contributions<br />

from different fissioning systems. A revised<br />

version <strong>of</strong> <strong>the</strong> Brosa model [5.2] includes <strong>the</strong><br />

temperature dependence in <strong>the</strong> potential energy<br />

landscape <strong>of</strong> <strong>the</strong> nucleus to derive <strong>the</strong> probabilities<br />

<strong>for</strong> different fission modes. This approach is coupled<br />

with a model <strong>for</strong> <strong>the</strong> neck rupture to obtain <strong>the</strong><br />

mass and charge split <strong>for</strong> calculating <strong>the</strong> fission<br />

fragment and product mass and charge distributions.<br />

ALICE-91 [5.6], as well as <strong>the</strong> newly<br />

developed TALYS code [5.7], were used in <strong>the</strong><br />

benchmark exercise.

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