09.05.2014 Views

nureg/cr-6700 - Oak Ridge National Laboratory

nureg/cr-6700 - Oak Ridge National Laboratory

nureg/cr-6700 - Oak Ridge National Laboratory

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Criticality Safety Section 3<br />

The fission product exhibiting the most rapid in<strong>cr</strong>ease with burnup is the stable nuclide 155 Gd. Its precursor<br />

155 Eu has a 4.75-year half-life, and so 155 Gd has not reached equilibrium even for a 70-GWd/t exposure. The<br />

importance of 155 Gd in<strong>cr</strong>eases by an order of magnitude between 20 and 60 GWd/t for cooling times greater<br />

than about 5 years, and it is one of the larger fission-product absorbers in high-burnup fuel. Another stable<br />

nuclide, 153 Eu, exhibits a similar, although less-pronounced effect, as its precursor 153 Gd and has a 241.6-day<br />

half-life. However, 153 Eu ranks considerably lower than 155 Gd in high-burnup fuel for cooling times more<br />

than 5 years.<br />

The <strong>cr</strong>iticality safety nuclide rankings were recomputed for the PWR fuel using a SAS2 model in which the<br />

specific power was 25 MW/t. In general, the nuclide rankings were not affected, except that (rarely) the<br />

order of two nuclides could be reversed. In those cases, the absorption rates for the nuclides whose order<br />

changed were essentially identical. The only noticeable difference in the actinides for decay times from 5 to<br />

100 years was an in<strong>cr</strong>ease of about 6% in the absorption fraction for 238 Pu. The amount of 238 Pu in<strong>cr</strong>eases<br />

because its precursor 237 U (produced both by capture from 235 U to 236 U and from (n,2n) from 238 U) undergoes<br />

relatively more decays to 237 Np when the power (and therefore flux) is lower. The biggest changes in<br />

fission-product absorption rates were for the stable 149 Sm (−11%) and 157 Gd (−15%) nuclides that have large<br />

capture <strong>cr</strong>oss sections.<br />

22

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!