Research Article

Developments in Sensitivity Methodologies and the Validation of Reactor Physics Calculations

Table 4

C/E and associated uncertainties (σ) before and after adjustment.

Type of experimentOld New Type of experimentOld New

U235 Capture PROFIL1a Cm244 TRAPU2b
U238 Capture PROFIL1a U238 Fission Rate COSMOc
Pu238 Capture PROFIL2a Np237 Fission Rate COSMOc
Pu239 (N,2N) PROFIL1a Pu238 Fission Rate COSMOc
Pu239 Capture PROFIL1a Pu239 Fission Rate COSMOc
Pu240 Capture PROFIL1a Pu240 Fission Rate COSMOc
Pu241 Capture PROFIL1a Pu241 Fission Rate COSMOc
Pu242 Capture PROFIL1a Pu242 Fission Rate COSMOc
Am241 Capture PROFIL1a Am241 Fission Rate COSMOc
Np237 Capture PROFIL2a Am243 Fission Rate COSMOc
U236 TRAPU2b GODIVAd
Np237 TRAPU2b U238 Fission Rate GODIVAd
Pu238 TRAPU2b Np237 Fission Rate GODIVAd
Pu239 TRAPU2b Pu239 Fission Rate GODIVAd
Pu240 TRAPU2b JEZEBEL9e
Pu241 TRAPU1b U238 Fission Rate JEZEBEL9e
Pu242 TRAPU1b Np237 Fission Rate JEZEBEL9d
Am241 TRAPU2b JEZEBEL0e
Am242 TRAPU2b CIRANOf
Am243 TRAPU1b ZPPR-15
Cm242 TRAPU1b ZPR-3/53
Cm243 TRAPU2b ZPR-3/54

Isotope A/B atom density ratio at the end of irradiation of a sample of isotope A.
aIsotope atom density at the end of irradiation of TRAPU fuel pins with different initial Pu vectors.
bNormalized fission rates and in the COSMO critical experiment at MASURCA.
cJEZEBEL9: Pu-239 Sphere.
dJEZEBEL0: Pu-239 Sphere with high Pu-240 content.
e of the critical experiment CIRANO (high Pu content) at MASURCA.