sensitivities of monte carlo simulations to ......27 novembre 2018 | slide 10 cea | 10 avril 2012...
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SENSITIVITIES OF MONTE
CARLO SIMULATIONS TO
NUCLEAR RESONANCE
PARAMETERS
E. Vandermeersch
P. Tamagno
C. De Saint Jean
NOVEMBER 27, 2018 | SLIDE 1CEA | 10 AVRIL 2012WPEC - SG44 AND 46
CROSS SECTIONS EVALUATION
CONTEXT
27 NOVEMBRE 2018
| SLIDE 2
CEA | 10 AVRIL 2012
+
Covariances
,... ,, FissionOMPRRRx
Neutron/Gamma
Transport
,...),,,,( ji fissionOMURRRRRn xxxxE
Integral Data
Assimilation
on Parameters
CROSS SECTIONS EVALUATION CONTEXT NOW
Processing
Real Life Application
IntegralExperiments
A long way between nuclear physics and reactor physicsFormat/processing issues Uncertainty a side product
– Expérience
– Model
+
Covariances
,... ,, FissionOMPRRRx
Neutron/Gamma
Transport
,...),,,,( ji fissionOMURRRRRn xxxxE
Integral Data
Assimilation
on Parameters
CROSS SECTIONS EVALUATION IN THE FUTURE ?
Real Life Application
IntegralExperiments
Direct connection between Nuclear Physicists and Reactor PhysicistsImpact of simplified nuclear data representation (format/processing)Neutronic parameters sensitivities (keff …) to basic nuclear data ((E),x)Better uncertaitny propagation covariances replaced by pdfs
– Expérience
– Model
CROSS SECTIONS EVALUATION
Various nuclear reaction models are used to describe the cross section
Nuclear reaction parameters are the initial information (x).
This work was limited to the R-Matrix formalism in the Resolved Resonance Range (RRR).
Future Works on RRR/URR and Continuum
27 NOVEMBRE 2018 | SLIDE 5CEA | 15 MAY 2018
Resonances, Coumpound nucleus et al. !
239Pu total cross section
Optical Models
Statistical Model
Transmission Models
R Matrix
',,, RaEx ca
aca SDRax ,,,, 0
,...,,,,2 WVdax cc
CONRAD COde for Nuclear Reaction Analysis and Data assimilation
Can work with various formalisms in Resolved Resonances Range (RRR) (R-Matrix
approximation, Reich-Moore, Multi-Level Breit-Wigner), Unresolved Resonances
Range (URR) (Average R-Matrix) and continuum (Optical model)
Used to compute cross sections 𝜎𝑖 ,𝑟 and their sensitivities 𝑆𝜎𝑖,𝑟, Γi to resonance
parameters Γi∶
𝑆𝜎𝑖,𝑟, Γi = න
𝐸,Ω
𝜕𝜎𝑖 ,𝑟 𝐸, Ω
𝜕Γi⋅ Γi𝑑𝐸𝑑Ω
NUCLEAR PHYSIC TOOL
AND NEUTRONIC CALCULATION TOOLS
27 NOVEMBRE 2018 | SLIDE 6CEA | 15 MAY 2018
TRIPOLI-4 neutron/gamma and electron transport in materials
Used to compute neutronic observables and their sensitivities𝑆𝜌,𝜎𝑛,𝑐 to cross sections 𝜎𝑖 ,𝑟 :
𝑆𝜌,𝜎𝑛,𝑐 = න
𝑟, 𝐸,Ω
𝜎𝑛,𝑐 𝑟, 𝐸 ⋅𝜕𝜌 𝑟, 𝐸, Ω
𝜕𝜎𝑛,𝑐 𝑟, 𝐸𝑑𝐸𝑑²𝛺𝑑3𝑟
PERTURBATIONS AND SENSITIVITIES
IN MONTE CARLO SIMULATIONS
Exact Perturbations & IFP method
Exact perturbation for two states of the reactor, with 𝓟 the production operator, 𝓚 the
disappearance operator, 𝜙 the direct flux and 𝜙† the adjoint flux:
𝛿𝜌 =𝜙2†, (𝜆2Δ𝓟 − Δ𝓚)𝜙1
𝜙2†, 𝓟1𝜙1
27 NOVEMBRE 2018 | SLIDE 7CEA | 15 MAY 2018
Notice that the adjoint flux can
be estimated with the Iterated
Fission Probability IL:
𝜙† ∝ 𝐼𝐿 =ෑ
𝑔=1
𝐿𝑘𝑔
𝑘𝑔→∞
F
A
C
F C A
C
A
Generation 1 Generation 2
N
IFP cycle principle
CONRAD AND TRIPOLI-4 JUNCTION
IFP algorithm + Link to CONRAD calculation
The IFP method uses the following algorithm:
This algorithm can be modified to compute sensitivities to resonance parameters with
CONRAD:
27 NOVEMBRE 2018 | SLIDE 8CEA | 15 MAY 2018
For each simulationFor each collision {
Retrieve reactionsFor each reaction
For each nucleus{Retrieve & compute parameters (cross section, local flux)Compute sensitivity or perturbationAdd score to required integrated value
}}
𝑆𝜌 ,Γi = න
𝐸,Ω
Γi ⋅𝜕𝜌 𝐸, Ω
𝜕Γi𝑑𝐸𝑑Ω = න
𝐸,Ω
𝑟
𝜕𝜌 𝐸, Ω
𝜕𝜎𝑖 ,𝑟 𝐸, Ω⋅𝜕𝜎𝑖 ,𝑟 𝐸, Ω
𝜕Γi⋅ Γi 𝑑𝐸𝑑Ω
SENSITIVITIES COMPUTATION
Extended IFP method
27 NOVEMBRE 2018 | SLIDE 9CEA | 15 MAY 2018
RESULTS
27 NOVEMBRE 2018
| SLIDE 10
CEA | 10 AVRIL 2012
RESULTS
27 NOVEMBRE 2018 | SLIDE 11CEA | 15 MAY 2018
System studied
Plutonium-Solution-Thermal (ICSBEP):
- 239Pu/240Pu: 20
PST scheme
RESULTS
27 NOVEMBRE 2018 | SLIDE 12CEA | 15 MAY 2018
239Pu 𝐸𝜆 sensitivities
27 NOVEMBRE 2018 | SLIDE 13CEA | 10 AVRIL 2012
RESULTS
239Pu 𝜆 sensitivities
27 NOVEMBRE 2018 | SLIDE 14CEA | 10 AVRIL 2012
RESULTS
239Pu 𝜆 sensitivities
27 NOVEMBRE 2018 | SLIDE 15CEA | 10 AVRIL 2012
RESULTS
239Pu 𝜆 sensitivities
RESULTS
27 NOVEMBRE 2018 | SLIDE 16CEA | 15 MAY 2018
Details of the cross sections sensitivities for the first 240Pu resonance. So-called "Sensitivity (E) to GN1/Eλ1" are in
fact σr𝜕ρ
𝜕σr E
𝜕σr E
𝜕ΓE , with r all the reactions possible for 240Pu
CONCLUSION
27 NOVEMBRE 2018
| SLIDE 17
CEA | 10 AVRIL 2012
CONCLUSION
A functional new method has been implemented, tested, compared withthe other methods.
Add and test new formalisms : RRR/URR/Continuum nuclear reactionsmodels
Improvements:o Short term Improve TRIPOLI-4/JIMMY/CONRAD coupling.o Mid-term Remove as much as possible format/processing
27 NOVEMBRE 2018 | SLIDE 18CEA | 15 MAY 2018
APPENDIX
Resizing of the energy grid
Each resonance influences only a few number of neighbours:
27 NOVEMBRE 2018 | SLIDE 19CEA | 15 MAY 2018
Neighboursresonances
Targeted parameters
Energy Grid
239Pu Fission cross section, with the 31st resonance 𝐸𝜆 modified by 5%
APPENDIX
Resizing of the energy grid
Each resonance influences only a few number of neighbours:
27 NOVEMBRE 2018 | SLIDE 20CEA | 15 MAY 2018
Neighboursresonances
Targeted parameters
Energy Grid
239Pu Fission cross section, with the 31st resonance 𝐸𝜆 modified by 5%
APPENDIX
Results
27 NOVEMBRE 2018 | SLIDE 21CEA | 15 MAY 2018
Impact of the direct batches number.
APPENDIX
Cross sections
27 NOVEMBRE 2018 | SLIDE 22CEA | 15 MAY 2018
239Pu radiative capture (MT=102), fission (MT=18) and elastic (MT=2) cross section
240Pu radiative capture (MT=102), fission (MT=18) and elastic (MT=2) cross section
APPENDIX
Cross sections
27 NOVEMBRE 2018 | SLIDE 23CEA | 15 MAY 2018
235U radiative capture (MT=102), fission (MT=18) and elastic (MT=2) cross section
Figure B.4 - 238U radiative capture (MT=102), fission (MT=18) and elastic (MT=2) cross section