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FIESTA2017 FIssion ExperimentS and Theoretical Advances Neutron Cross Section Evaluation of U-238 Hyeong Il Kim Nuclear Data Center Korea Atomic Energy Research Institute 2017. 9. 18

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Page 1: Neutron Cross Section Evaluation of U-238 - t2.lanl.gov · EMPIRE/TALYS NJOY MCNP Parameters Correction Modern Computing Power ˘ hrs FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I

FIESTA2017FIssion ExperimentS and Theoretical Advances

Neutron Cross Section Evaluation of U-238

Hyeong Il Kim

Nuclear Data CenterKorea Atomic Energy Research Institute

2017. 9. 18

Page 2: Neutron Cross Section Evaluation of U-238 - t2.lanl.gov · EMPIRE/TALYS NJOY MCNP Parameters Correction Modern Computing Power ˘ hrs FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I

Table of Contents

1 Introduction

2 Nuclear Data Evaluation

3 Results

4 Summary

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Introduction Overview

Introduction

Nuclear Data EvaluationAnalyzing the measured physical quanties

+ Combing them with theoretical predictions=> Extract the true values of such quantiesDataBase

ENDF Library (Compact format)Processed to Pointwised or Groupwised Libraries

ApplicationInputs for various simulation codes(MCNP, Geant4, PHITS, DRAGON, DANTSYS, DORT · · · )

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 1

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Introduction Overview

Nuclear data activities An example of nuclear data eval. for 235U

Applications

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 2

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Introduction Overview

Uranium

Abundances of natural uranium234U: 0.0054 %235U: 0.7204 %238U: 99.2742 %

U-238Fuel of nuclear reactor

LWR: 95 ∼ 97 %, HWR: 98 ∼ 99 %

Well evaluated but Continuoulsy updatedCurrent version:

ENDF/B-VII.1, JENDL-4.0, JEFF-3.2,CENDL-3.1,RUSFOND-2010,...Preliminary:

ENDF/B-VIII-b4, JEFF33T4

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 3

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Nuclear Data Evaluation Cross section

Cross sections for U-238

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 4

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Nuclear Data Evaluation Cross section

Cross Sections

Cross SectionsCross Section: function of the kinetic energy of the particle a

σ(Ea) =

∫ ∫d2σ(Ea,Eb,Ω)

dEbdΩdEbdΩ

Differential Cross Section: Distributions of an emitted particle foranlge or energy

dσ(Ea,Eb)

dEb

dσ(Ea,Ω)

Double-Differential Cross Section (DDX): Distributions of an emittedparticle for anlge and energy

d2σ(Ea,Eb,Ω)

dEbdΩ

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 5

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Nuclear Data Evaluation Nuclear Reaction

Interactions between particle and nucleus

Schrodinger equation(− ~2

2µO2 + U(r)

)Ψ = EΨ,

where Ψ(r , θ, φ) = R(r)Y ml (θ, φ).

Scattering matrix

Scatteringregion

Il(kr)

SlOl(kr)

r

Ψ(r) =i2

(Il(kr) − Sl Ol(kr)

)

Scattering Matrix

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 6

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Nuclear Data Evaluation Nuclear Reaction

Phenomenological Optical Model Potential (OMP)

U(r,E) = Vc(r,E)

−(VV(E) + iWV(E)) fV(r)

+(VD(E) − iWD(E))gD(r)

−2l · ~s(VSO(E) + iWSO(E))hSO(r),

Coulomb

Volume

Surface

Spin-Orbit

where VV,SO and WV,D,SO are the real and imaginary components of the volume central(V), surface-central (D) and spin-orbit (SO) potentials, respectively.

fi(r) =1

(1 − exp[(r − Ri)/ai]), gi(r) = −4aD

ddr

fi(r), hi(r) =1r

ddr

fi(r),

where the geometry parameters are the radius Ri = riA1/3, whith A begins atomic massnumber, and the diffuseness parameters ai.

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 7

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Nuclear Data Evaluation Nuclear Reaction

K-D form

VV(E) = v1[1 − v2(E − E f ) + v3(E − E f )2 − v4(E − E f )3],

WV(E) = w1(E − E f )2

(E − E f )2 + w22

,

WD(E) = d1(E − E f )2

(E − E f )2 + d23

exp[−d2(E − E f )],

VSO(E) = vso1exp[−vso2(E − E f )],

WD(E) = wso1(E − E f )2

(E − E f )2 + (wso2)2 ,

where E f ,N,Z and A are the Fermi energy, number of neutrons, number ofprotons, and mass number, respectively. In all cases, the geometry (ri, ai) of thepotential is assumed to be independent of the energy.

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 8

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Nuclear Data Evaluation Reaction Model

Model calculation

ModelOMP, Level density,preequilibrium, fissionmodel, γ-ray strengthfunction, · · ·

ParameterizationDefault parameters:Taken from therecommended data inRIPL-3 (Reference InputParameter Library)Parameterizing toreproduce the measureddata

Code: Empire-3.2

Model Calculations

χ2 & Eyeguide?(Exp. of Isotope)

χ2 & Eyeguide?(Exp. of Element)

Evaluated files

yes

no

yes

no

Adjustments

of parameters

Adjustments

of parameters

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Nuclear Data Evaluation Reaction Model

Total cross section

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Nuclear Data Evaluation Reaction Model

Elastic cross section

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Nuclear Data Evaluation Reaction Model

Elastic Angular Distribution

0 20 40 60 80 100 120 140 160 18010-1

100

101

102

103

104

105

106

107

108

109

1010 Angular Distribution1.500 x106

2.500 x105

4.000 x104

7.000 x103

12.000 x102

14.100 x101

15.000 x100

Energy (MeV)

Cro

ss S

ect

ion (

mb)

Discrepancies with total and elastic XSDo not consider too much in this work

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 12

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Nuclear Data Evaluation Reaction Model

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Nuclear Data Evaluation Reaction Model

Particle Spectra

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Nuclear Data Evaluation Reaction Model

Neutron proudctions induced by neutron with 14.1 MeV energy

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 15

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Nuclear Data Evaluation Reaction Model

Neutron proudctions induced by neutron around 14 MeV

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 16

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Nuclear Data Evaluation Recursive Evaluation

KAERI/NDC evaluation

Initial Models

Reaction Models ENDF-6 format

ACE fileCriticality

ParameterizationsEMPIRE/TALYS

NJOY

MCNP

ParametersCorrection

Modern Computing Power∼ hrs

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Results Cross Section

Results

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Results Cross Section

Prompt ν

Linear fit in energy bin

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Results Cross Section

Total ν

prompt ν + delayed ν from (ENDF/B-VII.1)

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Results Cross Section

Inelastic cross section

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Results Cross Section

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Results Cross Section

Capture cross section

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Results Cross Section

Fission cross section

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 24

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Results Cross Section

Fission spectra

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Results Cross Section

(n,2n) cross section

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Results ICSBEP

Criticality (Fast Spectra)

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Results ICSBEP

Criticality (Fast Spectra)

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Results ICSBEP

Cross Sections of U-235

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Summary

Summary

The U238 evaluation in fast neutron region was introduced.The fast check from evaluation to validation is possible by theup-to-date nuclear reaction model code and modern computingpower.Our U-238 evaluation will be finalized soon together with theU-235 one.

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Thank you for your attention!

FIESTA2017, Eldorado Hotel, Santa Fe, NM H. I. Kim 30