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ORNL-5388 - the Molten Salt Energy Technologies Web Site

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4-4<br />

Table 4.0-1 gives some of <strong>the</strong> pertinent neutronic properties of <strong>the</strong> different fis-<br />

sile nuclides for a specific <strong>the</strong>rmal-neutron energy.<br />

In discussing <strong>the</strong>se properties,* it<br />

is necessary to distinguish between <strong>the</strong> two functions of a fissile material: <strong>the</strong> production<br />

of energy (i.e., power) and <strong>the</strong> production of ezcess neutrons which when absorbed by fertile<br />

material will produce additional fissile fuel.<br />

Nuclide<br />

Table 4.0-1. Nuclear Parameters of <strong>the</strong> Principal Fissile Nuclides<br />

233U, 235U, 239Pu, and 241P~a9b at Thermal <strong>Energy</strong><br />

(Neutron <strong>Energy</strong> = 0.0252 eV, velocity = 2200 m/sec)<br />

Cross Section (barns)<br />

‘a uf uc<br />

a V n<br />

23311 578 2 2 531 2 2 47 1 0.089 2 0.002 2.487 2 0.007 2.284 2 0.006<br />

2351) 678 2 2 580 2 2 98 2 1 0.169 2 0.002 2.423 2 0.007 2.072 2 0.006<br />

239Pu 1013 2 4 742 2 3 271 3 0.366 2 0.004 2.880 5 0.009 2.109 2 0.007<br />

241Pu 1375 2 9 1007 7 368 2 8 0.365 2 0.009 2.934 2 0.012 2.149 2 0.014<br />

~~<br />

a<br />

G. C. Hanna et al., Atomic Energ. Rev. 7, 3-92 (1969); figures in <strong>the</strong> referenced article<br />

were all given to one additional significant figure,<br />

b~a = uf + uc; a = uc/uf; v = neutrons produced per fission; 11 = neutrons produced per atom<br />

destroyed = v/(l + a).<br />

The energy-production efficiency of a fissile material is directly related to its<br />

neutron capture-to-fission ratio (a), <strong>the</strong> smaller <strong>the</strong> ratio <strong>the</strong> greater <strong>the</strong> fraction of<br />

neutron-nuclide interactions that are energy-producing fissions. As indicated by Table<br />

4.0-1, at <strong>the</strong>rmal energy <strong>the</strong> value of a is significantly smaller for 233U than for <strong>the</strong><br />

o<strong>the</strong>r isotopes, and thus 233U has a greater energy-production efficiency than <strong>the</strong> o<strong>the</strong>r<br />

isotopes. (lhe energy released per fission differs only slightly for <strong>the</strong> above isotopes.)<br />

The neutron-production efficiency of a fissile material is determined by <strong>the</strong> number<br />

of neutrons produced per atom of fissile material destroyed (n), <strong>the</strong> higher <strong>the</strong> number <strong>the</strong><br />

more <strong>the</strong> neutrons that will be available for absorption in fertile material. Table 4.0-1<br />

shows that <strong>the</strong> n value for 233U is higher than that for any of <strong>the</strong> o<strong>the</strong>r nuclides, although<br />

plutonium would at first appear to be superior since it produces more neutrons per fission<br />

(v). The superiority of 233U results from <strong>the</strong> fact that a is lower for 233U and 0 = v/(l + a).<br />

Thus at <strong>the</strong>rmal energies 233U both yields more energy and produces more neutrons per atom<br />

destroyed than any of <strong>the</strong> o<strong>the</strong>r fissile nuclides.<br />

In <strong>the</strong> energy range of interest for fast reactors (~0.05 - 4.0 MeV), <strong>the</strong> situation<br />

is not quite so straightforward. Here again, <strong>the</strong> a value for 233U is significantly lower<br />

than <strong>the</strong> values for <strong>the</strong> o<strong>the</strong>r fissile nuclides, and, moreover, <strong>the</strong> microscopic cross section<br />

for fission is higher (see Fig. 4.0-1). The energy release per fission of 233U is<br />

somewhat less than that of <strong>the</strong> plutonium nuclides, but <strong>the</strong> energy release per atom of 233U<br />

destroyed is significantly higher than for th, othcr nuclides. Thus, from ths standpoint<br />

*Much of this discussion on <strong>the</strong> neutronic properties of nuclides is based on refs. 1 - 3.

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