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RRFM 2009 Transactions - European Nuclear Society

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switch from a fast to a thermal spectrum in the parameters above can at least be partially<br />

counteracted.<br />

Methodology<br />

For this preliminary parametric study it was decided to use the depletion code DARWIN 2.2<br />

[3] to handle both the JHR [2] case and the SFR [1] reference sample with the same program<br />

and data files. As a reference sample serves Am 0.1 U 0.9 O 2 because it’s a likely candidate for<br />

the actual experiment and has plenty of margin to change the fission rate by 235 U enrichment.<br />

Additionally similar compositions have already been investigated as transmutation/fertile<br />

blanket in the SFR core [3]. Starting from the reference sample U enrichment, neutron flux<br />

level and Am content, but not isotopic composition, were modified in the JHR spectrum to<br />

approach the behaviour of the same sample in the SFR. Table 1 shows reference case for<br />

both reactor spectra.<br />

SFR core<br />

JHR reflector<br />

max flux [n/s/cm²] 2.4667x10 15 5.1267x10 14<br />

spectrum<br />

ERANOS<br />

33 gr.<br />

TRIPOLI<br />

172 gr.<br />

reference sample Am 0.1 U 0.9 O 2<br />

density [g/cm³] 10.3<br />

U mass composition<br />

Am mass composition<br />

0.25% 235 U, 99.75% 238 U<br />

95% 241 Am, 5% 243 Am<br />

Tab 1: Reference cases for JHR and SFR<br />

The necessary neutron spectra were provided by existing detailed TRIPOLI4.4 and ERANOS<br />

models for the JHR, SFR and PHENIX and are shown below in figure 1.<br />

Neutron Spectrum<br />

1.E+15<br />

1.E+14<br />

1.E+13<br />

1.E+12<br />

JHR reflector<br />

SFR in core<br />

1.E+11<br />

1.E+10<br />

1.E+09<br />

1.E- 09 1.E- 08 1.E- 07 1.E- 06 1.E- 05 1.E- 04 1.E- 03 1.E- 02 1.E- 01 1.E+00 1.E+01 1.E+02<br />

Energy [MeV]<br />

Fig 1: Neutron spectrum used in the calculations<br />

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