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 experiment
Old
New
Type of experiment
Old
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.