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Resonance Parameter Covariance Representation: File32 versus File33 Nuclear Data Week SG44 November 23, 2017 IRSN / PSN-EXP/SNC Luiz LEAL © IRSN

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Page 1: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Resonance Parameter CovarianceRepresentation: File32 versus File33

Nuclear Data Week SG44November 23, 2017

IRSN / PSN-EXP/SNCLuiz LEAL© IRSN

Page 2: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

▌Resonance Region Covariance

▌Evaluations for 48Ti;

▌FILE32 to FILE33 conversion;

▌Application;

▌Concluding Remarks;

OUTLINE

Luiz Leal, Nuclear Data Week SG44, November 23, 2017 2

Page 3: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Available Covariance Data in ENDFContents of File Types (MF)

MF=30: sensitivity data covariance filesMF=31: covariance for average number of neutrons

per fissionsMF=32: covariance for resonance parametersMF=33: covariance for reaction cross sectionsMF=34: covariance for angular distributionsMF=35: covariance for energy distributionsMF=36: covariance for angle-energy distributionsMF=37~38: nullMF=39: covariance for radionuclide production yieldsMF=40: covariance for radionuclide production cross

sections

3Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 4: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Conversion from FILE32 to FILE33Averaged Group Cross Sections

g xg xE

E

g

g

E E dE 1

( ) ( )

g E

E

E dEg

g

( )1

4Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 5: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Covariance Matrix for Group Cross Sections

If p1, p2, …,pn are evaluated resonanceparameters such that

x x np p p ( , ,..., )1 2

xg

xj

jjjp

p

5Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 6: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Group Covariance Matrix

Covariance of the group cross sections depends on the covariance of the resonanceparameters p as

These quantities are the resonance parameter covariancestored in the ENDF library (FILE32)

6Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 7: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Averaged Group Cross Section

▌Alternatively, the group covariance crosssection can also be obtained as

7Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 8: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Question:Can one find an equivalence ?

8Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 9: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

FILE32 to FILE33 ConversionTwo stages:

Stage 1: Process resonance parameter covariance andgenerate averaged group cross-section uncertainties andcorrelation matrices. Either PUFF/AMPX orNJOY/ERRORR can be used;

Note: choice of an appropriate energy group structure andflux weighting spectra.

Stage 2: Conversion of cross section uncertainty andcovariance generated in stage 1 into the ENDF FILE33format;

Note: Simple way that this can be achieved is by using theCOVCON module of the AMPX code system.

9Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 10: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Application

▌Process the 48Ti resonance parameterevaluation;

▌Choice of two energy group structures:Coarse: 44 groupsFiner : 380 groups

▌ Use AMPX/PUFF to process the covariancedata;

10Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 11: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

48Ti Resonance Evaluation▌Evaluation tool: SAMMY

▌Energy range: Thermal to 400 KeV

▌Experimental Data Base: transmission,

capture

▌Resonance Formalism: R-Matrix (Reich-

Moore)

▌Final Results: Resonance Parameters (RP)

and Resonance Parameter Covariance

(RPCM)

11Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 12: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Experimental Data Base(measurements done at ORELA)

Data Set Energy Range(keV)

Flight Path(meters)

Density(at/b)

Natural Titanium

Transmission 0.01 – 500.0 79.827 0.052966

Transmission 0.01 – 500.0 79.827 0.008785

Capture 0.01 – 500.0 40.116 0.035158

Enriched 48 (99.32 %)

Transmission 0.01 – 500.0 79.827 0.028185

Transmission 0.01 – 500.0 79.827 0.0011821

Capture 0.01 – 500.0 40.116 0.0091386

12Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 13: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Fitting of the total and capture cross sections

13Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 14: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Uncertainty and the correlation for the capture cross section

14Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 15: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Cross section at thermal and capture resonance integral

Quantity ENDF/B-VII.0 New 48TiEvaluation

σγ 7.84 8.32 ± 0.23

σs 4.36 4.04 ± 0.20

σt 12.20 12.35 ± 0.30

Iγ 3.68 3.78 ± 0.17

15Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 16: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

FILE32 to FILE33 Conversion

▌AMPX modules used: PRELL, PRILOSEC, PUFF, and

COVCONV

▌Energy Groups: 44-group and 380-group

▌In the resonance range up to 400 keV:

▌35-group of the 44-group

▌343-group of the 380

▌Three Cross Section Libraries:

▌RPCM_LIB: FILE32

▌CSCM_44LIB: FILE33 44-group

▌CSCM_380LIB: FILE33 380-group

▌BOXER and COVERX format

16Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 17: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

380-group (black line) and the 44-group (red line)

17Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 18: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Covariance Libraries Computer Storage

Library Size

RPCM_LIB 904 KB

CSCM_44LIB 95 KB

CSCM_380LIB 7.2 MB

18Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 19: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Test and Results

▌27-group and 238-group used for

calculating averaged cross section and

covariance

▌Constant energy neutron flux

▌Three Cross Section Libraries:

19Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 20: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Test and Results: 27-group calculated covariancefor the total cross section

20Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 21: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Test and Results: 27-group calculated covariancefor the capture cross section

21Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 22: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Test and Results: 238-group calculated covariancefor the total cross section

22Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 23: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Test and Results: 238-group calculated covariancefor the capture cross section

23Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 24: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Conclusions

▌Care must be taken when using few-group covariancerepresentations. It may be appropriate for the energyrange where the data are smooth and the resonancesare not present as for instance in the high energy region

▌For a detailed covariance results the use of the RPCM isrecommended

▌Conversion of the RPCM to CSCM using a fine energy-group structure must be examined so as to assure thatthe computer allocation size is not overwhelming largerthan that of the RPCM

▌In the resonance region few-group representation isacceptable when a general overview of the impact ofcovariance results is sought

24Luiz Leal, Nuclear Data Week SG44, November 23, 2017

Page 25: Resonance Parameter Covariance Representation: File32 versus File33 · 2017-11-21 · FILE32 to FILE33 Conversion AMPX modules used: PRELL, PRILOSEC, PUFF, and COVCONV Energy Groups:

Food for Thought

▌Impact of the weighting spectrum in thecovariance conversion from RPCM to CSCM

▌Impact of the cross section energy self-shielding

▌Impact of the cross section on thetemperature effect

25Luiz Leal, Nuclear Data Week SG44, November 23, 2017