IMPACT OF THE FISSION YIELD COVARIANCE DATA IN BURN-UP CALCULATIONS

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IMPACT OF THE FISSION YIELD COVARIANCE DATA IN BRN-P CALCLATIONS O. Cabellos, D. Piedra, Carlos J. Diez Department of Nuclear Engineering, niversidad Politécnica de Madrid, Spain E-mail: oscar.cabellos@upm.es 1

Outline 1. Introduction: Burnup Credit 1.1 Pin-cell Burn-up AM Benchmark 1.2 Propagation of FY ncertainties in pin-cell burn-up Benchmark 1.3 State-of-art FY Covariance Data 1.3.1 Bayesian Methodology by Katakura 2. Methodology to propagate ND ncertainties 2.1 Monte Carlo Methodology: Number Density ncertainty 2.1.1 Monte Carlo Methodology: Number Density ncertainty for 148 Nd, 137 Cs and 139 La 2.1.2 Monte Carlo Methodology: Number Density ncertainty for 109 Ag and 129 I 2.1.3 Low correction for 109 Ag using Katakura correlation matrix 2.2 S/ Methodology: Number Density ncertainty 2.2.1 S/ Methodology: 148 Nd, 139 La and 137 Cs (burnup indicators) 2.2.2 S/ Methodology: 109 Ag and 129 I 3. ncertainty Propagation: Criticality ncertainty Summary and conclusions 2

1. Introduction: Burnup Credit In nuclear criticality safety studies involving spent fuel, burn-up credit is being pursued and has been implemented in many countries as a means of more accurately and realistically determining the system reactivity by taking into account a decrease in the reactivity of spent fuel during irradiation. Table 1. Commonly measured Fission Products of importance to different safety-related fuel applications. Ref.: Spent Nuclear Fuel Assay Data for Isotopic Validation State-of-the-art Report, NEA/NSC/WPNCS/DOC(2011)5 Expert Group on Assay Data of Spent Nuclear Fuel (EGADSNF) 3

1.1 Pin-cell Burn-up AM Benchmark Table A.10: Hot Full Power (HFP) conditions for fuel pin-cell test problem Fuel temperature (K) 900.0 Cladding Temperature (K) 600.0 Moderator (coolant) temperature (K) 562.0 Moderator (coolant) density (g/cm3) 0.7484 Reactor Power (MWt) 2772.0 Total number of fuel assemblies in the reactor core 177 Number of fuel rods per fuel assembly 208 Active core length (mm) 3571.20 Table A11: Configuration of pin-cell test problem nit cell pitch (mm) 14.427 Fuel pellet diameter (mm) 9.391 Fuel pellet material O2 Fuel density (g/cm3) 10.283 Fuel enrichment (w/o) 4.85 Cladding outside diameter (mm) 10.928 Cladding thickness (mm) 0.673 Cladding material Zircaloy-4 Cladding density (g/cm3) 6.55 Gap material He Moderator material H2O Table A12: Simplified operating history data for benchmark problem pin-cell calculation and specific power Operating cycle 1 Ref.: Benchmarks for ncertainty Analysis in Modelling (AM) for the Design, Operation and Safety Analysis of LWRs, Volume I: Specification and Support Data for Neutronics Cases(Phase I), NEA/NSC/DOC(2013)7 May 2013 Expert Group on ncertainty Analysis in Modelling Burn time (days) 1825.0 Final Burnup (GWd/MT) 61.28 Downtime (days) 1870.0 Specific power (kw/kg) 33.58 4

References on FY uncertainty calculations: 1.2 Propagation of FY ncertainties in pin-cell burn-up Benchmark J.S. Martínez et al., GRS Results for the Burnup Pin-cell Benchmark Propagation of Cross- Section, Fission Yields and Decay Data ncertainties, 7th Int. Workshop on ncertainty Analysis in Modeling, OECD/NEA, Paris, France. 10-12 April 2013. - Implemented in XSSA Methodology (Monte Carlo) using FY-ENDF/B-VII.1 Nd-148 Justification of FY covariance generation methodologies?? Table 2. Cumulative fission yield uncertainty value by fission in and Pu with thermal neutrons. Data processed from ENDF/B-VII.1 Fission Yield Data Library. < 1% CFY: Rel. err. By neutron thermal fission in: CFY: Rel. err. By neutron thermal fission in: (in%) Pu (in%) Pu 148 Nd 0.35 0.50 129 I 1.0 4.0 137 Cs 0.50 0.50 109 Ag 64.0 64.0 139 La 0.70 2.80 - - - 5

1.3 State-of-art FY Covariance Data 6

1.3 State-of-art FY Covariance Data FY covariance data generation: Great efforts have been committed to develop methodologies for correlation generation (full covariance matrices) for FY data. This task is in the scope of the framework of WPEC-SG37. Methodologies proposed at the kick-off meeting of WPEC-SG37 (May 2013), based on: o Perturbation theory applied to the Five Gaussians and Wahl s models (Musgrove et al., 1973; Wahl, 1988), proposed by Pigni et al. (2013). o Monte Carlo parameter perturbation using the GEF code (Schmidt and Jurado, 2010), presented by Schmidt (2013). o Bayesian/general least-squares (GLS) method, where the IFY covariance matrix is updated with information on the chain yields as proposed by Kawano and Chadwick (2013), and previously applied by Katakura (2012). A variation of this proposal, with IFYs covariance matrix updated with CFYs ones is described and reported by PM/SCK (L. Fiorito et al., 2014) 7

1.3.1 Bayesian Methodology by Katakura Ref. : Fission Yield Covariance generation, L. Fiorito et al. Annals of Nuclear Energy, 2014 8

2. Methodology to propagate ND ncertainties Monte Carlo burnup calculation SCALE6.1.2/TRITON o Generation of a set of 1000 FY random libraries for and Pu No-correlation. FY uncertainty is the standard deviation of ENDF/B-VII.1 Correlation matrix using Katakura methodology o PDF: Normal distribution, with zero for negative values. Sensitivity/ncertainty calculation SCALE6.1.2/TRITON - Calculation of Sensitivity coefficients: S FYi,j= ( N i /N i ) / ( FY i,j/fy i,j) - S/: 1 st Order Approximation, Sandwinch Formula 9

2.1 Monte Carlo Methodology: Number Density ncertainty Table 3. ncertainty in number density (in %) for some important fission products at 60 GWd/MT. Fission Yield source of uncertainty (standard deviation) is taken from ENDF/B-VII.1. i) No correlation between fission products ( FYs/No corr.) ii) FYs including correlations for and Pu taken from Katakura methodology ( FYs/Corr.) iii) GRS calculation Nuclide Corr. No corr. GRS XSSA Nuclide Corr. No corr. GRS XSSA 79 Se 3.5 16.0-142 Nd 0.8 3.5-90 Sr 0.8 6.2-143 Nd 0.4 6.5 5.9 95 Mo 0.5 8.4 7.9 144 Nd 0.2 3.9-99 Tc 0.8 10.0 9.5 145 Nd 0.4 7.1 6.7 101 Ru 0.7 4.6-146 Nd 0.7 10.8-106 Ru 1.2 13.7-148 Nd 0.8 13.7 13.0 103 Rh 1.1 12.1-147 Pm 0.6 10.3-109 Ag 10.9 17.8-147 Sm 0.5 9.4-125 Sb 4.2 19.1-149 Sm 0.6 12.2 10.6 129 I 2.7 20.7-150 Sm 0.6 10.3-135 I 2.8 4.3-151 Sm 0.7 11.7-131 Xe 0.4 6.9-152 Sm 0.6 11.3 8.8 135 Xe 0.4 5.1-151 Eu 0.7 12.1-133 Cs 0.3 3.4 1.7 153 Eu 0.8 9.9-134 Cs 0.3 3.0-154 Eu 0.8 10.4-135 Cs 0.3 3.4-155 Eu 1.0 9.5-137 Cs 0.5 1.5 1.7 155 Gd 1.0 10.5 8.8 139 La 0.9 3.2-156 Gd 1.2 9.0-144 Ce 0.2 8.0-157 Gd 1.3 9.5-158 Gd 2.3 11.3-10

2.1.1 Monte Carlo Methodology: Number Density ncertainty for 148 Nd, 137 Cs and 139 La Figure 1. Relative standard deviations (in %) of 148 Nd, 137 Cs and 139 La (burnup indicators). Calculations performed with SCALE6.1.2, a set of 1000 random fission yield libraries based on ENDF/B-VII.1. i) No corr. case, nocorrelation between FYs ii) Corr. case where fission yield correlation matrices supplied for and Pu using Katakura methodology. Relative Stanadard Deviation (in %) 20 15 10 5 0 0 20 40 60 Burnup (GWd/MT) Nd148_DFY/Corr. Cs137_DFY/Corr. La139_DFY/Corr. Nd148_DFY/No corr Cs137_DFY/No corr La139_DFY/No corr 11

2.1.2 Monte Carlo Methodology: Number Density ncertainty for 109 Ag and 129 I Figure 2. Relative standard deviations (in %) of 109 Ag (burn-up credit) and 129 I (waste management). Calculations performed with SCALE6.1.2, a set of 1000 random fission yield libraries based on ENDF/B-VII.1. i) No corr. case, nocorrelation between FYs ii) Corr. case where fission yield correlation matrices supplied for and Pu using Katakura methodology. WHY? 12

2.1.3 Low correction for 109 Ag using Katakura correlation matrix Mass Yield Data Table 4. Range of mass chain yield uncertainties (in %) reported by England (1993) by fission in and Pu with thermal neutrons. A mass Pu A mass Pu 109 4-6 2.8-4 137 0.35-0.5 0.35-0.5 129 0.7-1.0 2-2.8 139 0.5-0.7 2-2.8 - - - 148 <0.35.35-0.5 Ref.: England T., Rider B., 1993. Evaluation and Compilation of Fission Technical Report, LA-R-94-3106, LANL (1993) Mass Yield Data Deficiencies for 109 Ag: High value of MFY standard deviation Only takes into account correction for IFY for the same A (exception for Ru108) 13

Calculation of Sensitivity Coefficients: S FYi,j= ( N i /N i ) / ( FY i,j/fy i,j) 2.2 S/ Methodology: Number Density ncertainty 0.8 _IFY: 57-La-148 _IFY: 58-Ce-148 Sensitivity coefficient: ( 148 Nd / 148 Nd) / ( IFY/IFY) 0.6 0.4 0.2 0 0 20 40 60 Burnup (GWd/MT) Pu_IFY: 58-Ce-148 Pu_IFY: 59-Pr-148 Pu_IFY: 59-Pr-148M Figure 3. Sensitivity Nd 148 coefficients calculated with SCALE6.1.2/TRITON by a linear perturbation of the IFY values (sensitivities with values higher that 0.05 are shown) 14

2.2.1 S/ Methodology: 148 Nd, 139 La and 137 Cs (burnup indicators) Table 5. ncertainty of the main independent fission yield contributors to the generation of 137 Cs, 137 La and 148 Nd by fission in and Pu with thermal neutrons. Data processed from ENDF/B-VII.1 Fission Yield Data Library. IFY: Rel. err. Generation of 137 Cs by fission in: IFY: Rel. err. Generation of 139 La by fission in: IFY: Rel. err. Generation of 148 Nd by fission in: (in%) Pu (in%) Pu (in%) Pu 137 Te 8.0 64.0 139 I 8.0 23.0 148 La 64.0 64.0 137 I 4.0 6.0 139 Xe 2.0 4.0 148 Ce 23.0 45.0 137 Xe 2.8 4.0 139 Cs 4.0 23.0 148 Pr 64.0 64.0 - - - - - - 148M Pr 64.0 64.0 S/, Applying Sandwich Formula : Table 6. Comparison of S/ and Monte Carlo uncertainty prediction at 60 GWd/TM. FY uncertainty with No corr. Nuclide S/ Monte Carlo 148 Nd 14.2 13.7 137 Cs 1.50 1.50 139 La 3.20 3.20 15

2.2.2 S/ Methodology: 109 Ag and 129 I Calculation of Sensitivity Coefficients: S FYi,j= ( N i /N i ) / ( FY i,j/fy i,j) Figure 4. Sensitivity Ag 109 coefficients calculated with SCALE6.1.2/TRITON by a linear perturbation of the IFY values (sensitivities with values higher that 0.05 are shown) 16

2.2.2 S/ Methodology: 109 Ag and 129 I Table 7. ncertainty of the main independent fission yield contributors to the generation of 109 Ag and 129 I by fission in and Pu with thermal neutrons. Data processed from ENDF/B-VII.1 Fission Yield Data Library. IFY: Rel. err. (in%) Generation of 109 Ag by fission in: IFY: Rel. err. Generation of 129 I by fission in: Pu (in%) Pu 109 Mo 64.0 64.0 129M Sn 6.0 64.0 109 Tc 64.0 64.0 129 Sn 11.0 64.0 109 Ru 64.0 64.0 129 Sb 45.0 64.0 108 Ru 64.0 64.0 - - - Table 8. Comparison of S/ and Monte Carlo uncertainty prediction at 60 GWd/TM. FY uncertainty with No corr. Nuclide S/ Monte Carlo 109 Ag 25.0 17.8 129 I 20.3 20.7 WHY? Our Monte Carlo method uses a truncated Normal PDF. Then, the new random set yields a reduced uncertainty. 17

3. ncertainty Propagation: Criticality ncertainty Figure 5. Relative standard deviation in k eff (in %): i) SCALE/XSSA calculation performed by GRS [7] only uncertainties in cross-section data, ii) SCALE/TSNAMI calculation [2] only uncertainties in cross-section data, iii) SCALE/XSA calculation by GRS with uncertainties only in fission yield data taken from ENDF/B- VII.1/FY data library, iv) Monte Carlo with a set of 1000 different fission yield data libraries based on ENDF/B-VII.1 with nocorrelation between fission yields ( No corr. ) v) Monte Carlo with correlations generated by Katakura method in and Pu ( Corr. ). 18

Summary and conclusions The present study has demonstrated the importance of covariance terms if fission yield data libraries to improve estimations of uncertainties in burn-up applications Results in a LWR pin-cell burnup benchmark It has been proved that non-correlated independent fission yields data bring to overestimated uncertainties in the number density and criticality predictions Comparison between S/ and Monte Carlo shows good agreement (except for 109 Ag) Assessment of the methodology to generate fission yield covariance data based on Katakura model using information of experimental mass fission yield data Covariance fission yield data for and Pu fissile nuclides were processed Covariance for isotopes in the same mass chain are modified Covariance data (by Katakura) changes the criticality and number density uncertainties, reducing its variance to almost a negligible effect (except for 109 Ag) 19

Acknowledgements This work is supported by: Agreement between CSN & PM in the area of ncertainty Propagation for Neutronic Calculations (2012-16) 20