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Development of an ENDF Thermal Library for SiO2 and Testing of ...

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<strong>Thermal</strong> Neutron Scattering<strong>an</strong>d Energy Tr<strong>an</strong>sferThe de Broglie wavelength (λ = h / p) <strong>of</strong> thermal neutrons (< ~ 1 eV) ison the order <strong>of</strong> the interatomic dist<strong>an</strong>ces in crystalline solids.The energy <strong>of</strong> thermal neutrons is <strong>of</strong> the same order as the vibrationalexcitation modes (e.g., phonons) available in condensed matter.σ TOTAL =σ INEL + σ EL + σ ABS4<strong>Thermal</strong> Neutron Scattering


Total Cross Section (barns)Modifying the Free-AtomCross Section <strong>for</strong> SiO 21000.0Free Gas <strong>Library</strong> (300 K)<strong>Thermal</strong> <strong>Library</strong> (300 K)K03ats)arn(bnctioSesrolCtaTo100.010.01.01.0E-05 1.0E-04 1.0E-03 1.0E-02 1.0E-01 1.0E+00 1.0E+01 1.0E+02 1.0E+03 1.0E+04 1.0E+05 1.0E+06 1.0E+07Energy (eV)6


Calculating the InelasticScattering Cross SectionDouble-differential cross section c<strong>an</strong> be written in terms <strong>of</strong> nuclearcross sections <strong>an</strong>d a scattering law:Simplified NJOY <strong>for</strong>m with S d (Q,ω) = 0:All that is required tosolve <strong>for</strong> σ inel is ρ(β)7


Calculating the ElasticScattering Cross SectionAll that is required tosolve <strong>for</strong> σ el is ρ(β)<strong>an</strong>d f i8


Structure <strong>of</strong> α-Quartz <strong>an</strong>d β-QuartzSilicons (yellow), Oxygens (red)11


Relative Density <strong>of</strong> States (1/eV)Relative Density <strong>of</strong> States (1/eV)Density <strong>of</strong> States3530252015Alpha PhaseBeta PhaseNatural Si in SiO 210500.00 0.02 0.04 0.06 0.08 0.10 0.12 0.14 0.16Energy (eV)3530Alpha Phase252015105Beta PhaseO-16 in SiO 200.00 0.02 0.04 0.06 0.08 0.10 0.12 0.14 0.16Energy (eV)12


VASP(DFT)PHONON(lattice dynamics)Hellm<strong>an</strong>n-Feynm<strong>an</strong>Forcesr(b) (DOS)LEAPR(NJOY)ACER (NJOY)(MCNP libraries)S ( ,b )Eel( E)THERMR(NJOY)Scattering Cross Sections inel (E ) <strong>an</strong>d el (E )


Cross-Section (barns)SiO 2 Calculated Cross SectionsCompared to Experimental Values100.0293.6 K[1] J. J. BLOSTEIN <strong>an</strong>d J. DAWIDOWSKI,“Experimental Neutron Data: Sigma(E)<strong>of</strong> Vitreous Silica (<strong>SiO2</strong>) Over the<strong>Thermal</strong> Energy R<strong>an</strong>ge,” PrivateCommunication, Inst. Balseiro y CentroAtomico Bariloche, Argentina (1999).10.0[2] B. M. RUSTAD, et al., “Neutron CrystalSpectrometer with R<strong>an</strong>ge Extended toSubthermal Energies,” Review <strong>of</strong>Scientific Instruments, 36, 887 (1965).1.01.0E-05 1.0E-04 1.0E-03 1.0E-02 1.0E-01 1.0E+00Neutron Energy (eV)14


ICSBEP HEU-MET-MIXED-005Benchmark15


BFS-79/3 Configuration16


Flux PercentageFlux Percentage<strong>Thermal</strong> Neutron Flux inFuel Tube Silica Pellets10.0%8.0%Silica Pelletsw/ Fast <strong>Library</strong>293.6 K800 K6.0%4.0%2.0%0.0%1.0E-03 1.0E-02 1.0E-01 1.0E+00 1.0E+01Upper Energy <strong>of</strong> Bin (eV)0.30%0.20%0.10%<strong>Thermal</strong> <strong>Library</strong>Contribution inSilica Pellets293.6 K800 K0.00%-0.10%-0.20%-0.30%-0.40%1.0E-03 1.0E-02 1.0E-01 1.0E+00 1.0E+01Upper Energy <strong>of</strong> Bin (eV)17


Flux PercentageFlux Percentage<strong>Thermal</strong> Neutron Flux inFuel Tube HEU Pellets7.0%6.0%5.0%HEUw/ Fast <strong>Library</strong>293.6 K800 K4.0%3.0%2.0%1.0%0.0%1.0E-03 1.0E-02 1.0E-01 1.0E+00 1.0E+01Upper Energy <strong>of</strong> Bin (eV)0.30%0.20%0.10%<strong>Thermal</strong> <strong>Library</strong>Contribution inHEU293.6 K800 K0.00%-0.10%-0.20%-0.30%-0.40%1.0E-03 1.0E-02 1.0E-01 1.0E+00 1.0E+01Upper Energy <strong>of</strong> Bin (eV)18


Differential Cross Section (b / eV)Secondary Neutron Energy DistributionDownscattering Example10.09.08.0E i = 0.112 eVPlots are normalized to 293.6 K (Phonons) such thatcross sections integrated over all energies are equal.293.6 K (Boltzm<strong>an</strong>n)293.6 K (Phonons)800 K (Phonons)7.06.05.04.0293.6 K: 62.5% total downscatter37.5% total upscatter800 K: 50.3% total downscatter49.7% total upscatter3.02.01.00.00.015 0.020 0.025 0.030 0.035 0.040 0.045 0.050Secondary Neutron Energy (eV)19


<strong>Thermal</strong> Contribution to Reactivity (pcm)<strong>Thermal</strong> <strong>Library</strong> Contribution to Reactivity(pcm)100274, +67293.6, +300200 300 400 500 600 700 800 900 1000 1100-100Benchmark Temperature (K)400, -149-200500, -234-300-400800, -3821000, -391-50022


Isotopics <strong>of</strong> Neutron Losses <strong>for</strong> SelectedFast <strong>an</strong>d <strong>Thermal</strong> LibrariesAbsorptionsFissionTemperature / <strong>Library</strong> H U-235 Si U-238 Al Other U-235293.6 K / Fast 16.941% 8.807% 11.108% 5.494% 5.068% 11.743% 40.839%293.6 K / Alpha <strong>Thermal</strong> 16.962% 8.808% 11.089% 5.489% 5.063% 11.740% 40.849%800 K / Fast 16.529% 9.115% 10.345% 5.662% 4.764% 12.006% 41.579%800 K / Alpha <strong>Thermal</strong> 16.613% 9.092% 10.475% 5.626% 4.819% 11.955% 41.420%1000 K / Fast 16.457% 9.126% 10.161% 5.637% 4.696% 12.100% 41.823%1000 K / Beta <strong>Thermal</strong> 16.528% 9.094% 10.290% 5.627% 4.745% 12.066% 41.650%23


Summary / Conclusions The phonon DOS <strong>for</strong> SiO 2 generated through a first-principlesapproach with the VASP / PHONON sequence c<strong>an</strong> produceaccurate thermal neutron scattering cross sections. The crystalstructure is the only fundamental input required. An <strong>ENDF</strong>-6 <strong>for</strong>mat thermal neutron scattering library <strong>for</strong> SiO 2was produced over a st<strong>an</strong>dard temperature grid (modelingα-quartz <strong>an</strong>d β-quartz) that is ready <strong>for</strong> submission to NNDC. The impact on k eff <strong>of</strong> accurate thermal scattering treatment <strong>of</strong>neutrons in SiO 2 in <strong>an</strong> ICSBEP benchmark is demonstrated. The use <strong>of</strong> a thermal neutron scattering library <strong>for</strong> SiO 2 maysignific<strong>an</strong>tly impact criticality calculations <strong>for</strong> geologic systems,especially in loss <strong>of</strong> heat removal accident scenarios.24

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