An Overview of What’s New in SCALE 5 S. M. Bowman, D. F. Hollenbach, M. D. DeHart, B. T. Rearden, I. C. Gauld, and S. Goluoglu Oak Ridge National Laboratory American Nuclear Society 2002 Winter Meeting
New Modules in SCALE 5 CENTRM: Continuous energy flux solution NITAWL-III: Compatible with ENDF/B-VI TSUNAMI: Sensitivity/uncertainty NEWT: 2-D flexible mesh STARBUCS: Burnup credit sequence SMORES: 1-D material optimization So many codes, so little time…
CENTRM/PMC CENTRM (Continuous Energy Transport Module) 1-D discrete ordinates code Problem-dependent pointwise continuous energy flux spectra at discrete spatial intervals for each unit cell Processes all resolved resonances in a mixture together PMC (Pointwise Multigroup Converter) Collapses pointwise continuous energy cross-sections for each nuclide into a set of problem dependent multigroup cross sections Separate CENTRM/PMC input files are created for each unit cell + one for all mixtures not in a unit cell
CENTRM/PMC (Cont.) Eliminate many of the limitations inherent in the Nordheim Integral Treatment used by NITAWL Overlapping resonances Multiple fissile materials in unit cell Assumed flux profile Process discrete level inelastic cross-section data Explicitly model rings in a fuel pin for spatial effect on the flux and cross sections
CENTRM/PMC (Cont.) Problem-dependent multigroup cross sections with accuracy of continuous energy cross sections ENDF/B-V continuous energy cross-section data files for CENTRM in SCALE 5 Correspond to ENDF/B-V 238- and 44 ‑ group libraries ENDF/B-VI continuous energy data for CENTRM under development for later release
SCALE 5 Criticality Sequence with CENTRM
NITAWL-III Can process multi-pole data, compatible with ENDF/B-VI cross-section data ENDF/B-VI multigroup library under development Processes cross-section data in the resolved resonance range for each nuclide individually Still limited to one fuel mixture per unit cell
Sensitivity/Uncertainty Codes Use adjoint-based first order linear perturbation theory to calculate sensitivities and propagate uncertainties Operate as automated SCALE analysis sequences k eff sensitivities to group-wise cross-section data are automatically generated for every reaction/nuclide/region (sensitivity profile) Group-wise sensitivity coefficients are written to data file for further analysis and plotting Other responses besides k eff can be added
TSUNAMI ( Tools for Sensitivity/UNcertainty Analysis Methodology Implementation) 1-D deterministic transport (XSDRNPM) 3-D Monte Carlo transport (KENO V.a) Produce sensitivity coefficients that represent the % change in k eff per % change in cross- section data Based on multigroup perturbation theory Accounts for effect of perturbations in resonance processing of cross-section data
Sensitivity Profiles Can Be Plotted to Highlight Similarities/Differences
Benefits of S/U Methodology Improved understanding of physics, identify parameters and regions of importance Validation: Establish similarity of experiments to system of interest Provides estimate of bias and uncertainty, including basis for interpolation and extrapolation beyond experiment range Identify experimental needs Optimize experiment design to best reduce bias and uncertainty in validation
NEWT Flexible Mesh S n NEW Transport algorithm 2-D discrete ordinates neutron transport code with flexible mesh capabilities Provides spatial and angular rigor necessary for advanced LWR fuel and MOX fuel designs Simple input concept based on SCALE user interface Grid generation is automated Generalized geometry capabilities, not limited to lattice configurations
PWR 17x17 Lattice =newt Calvert Cliffs fuel assembly (one-fourth) read parm fillmix=5 prtmxsec=no prtbroad=no sn=6 inners=10 outers=200 end parm read materials ! 3.0 enriched fuel, pin location 1 ! end end ! water (background material) ! end end materials read geom ' Fuel rod subgrid cylinder !fuel! end cylinder !clad! end ' Water hole subgrid cylinder !water hole! end cylinder !guide tube! end array domain boundary end geom end
Other Models Simple pin cell VENUS-2 MOX benchmark (1/4 core)
NEWT thermal spectra plots BWR w/ Gd rodsMOX Supercell
STARBUCS Features STARBUCS: Standardized Analysis of Reactivity for Burnup Credit using SCALE Integrated depletion analysis, cross-section processing and Monte Carlo criticality safety calculations for a 3-D system Uses existing, well-established modules in the SCALE system STARBUCS creates input, executes codes, and performs all data transfer functions
STARBUCS Features (cont.) Depletion analysis methodology Uses the ORIGEN-ARP sequence Cross-sections for depletion in ORIGEN-S obtained by interpolation of an existing ARP library Interpolation on enrichment, burnup, moderator density The analysis is extremely fast and accurate Criticality safety analysis KENO V.a or KENO VI Multigroup, 3-D analysis capability
STARBUCS Features (cont.) Flexible, easy-to-use sequence, uses input similar to existing SCALE modules Standard composition data used to define all materials in the problem (depletion and non-fuel) Depletion analysis input based on SAS2H-like input formats Any existing KENO V.a or KENO-VI input file (e.g., fresh fuel) can be used directly, with only minor changes
STARBUCS Features (cont.) Designed to simulate many of the important burnup credit phenomena identified in ISG-8, e.g., Axial and horizontal burnup variations Analyses can be performed for nuclide subgroups, i.e., evaluation of fission product margin Isotopic correction factors may be applied Sequence designed for, but is not restricted to, analysis of spent fuel casks Automatic loading curve generation under development
Data Flow in a BUC Analysis Spent fuel compositions for each spatial region (typically regions) separate burnup calculation for each region interpolation on compositions unreliable Extract nuclides for analysis Treatment of isotopic uncertainties - apply bias and/or uncertainty correction factors (if applicable) Resonance processing of multigroup cross sections Criticality calculation
SCALE Driver and STARBUCS Input ARP CSASI (BONAMI / NITAWL / ICE) End All regions complete? NO YES ORIGEN-S Spent fuel depletion and decay (repeat for all regions) WAX KENO V.a or KENO-VI Resonance cross-section processing (repeat for all regions) All regions complete? NO Combine cross sections for all regions Criticality calculation STARBUCS Burnup Credit Sequence for SCALE 5
SMORES SCALE Material Optimization and REplacement Sequence Performs automated 1-D optimization for criticality safety analysis
SMORES Methodology Prepare problem-dependent cross sections BONAMI/NITAWL-III, or BONAMI/CENTRM/PMC ICE creates a self-shielded macroscopic cross section library XSDRNPM 1-D calculation of forward and adjoint fluxes and k eff
SMORES Method (Cont.) Calculate the effectiveness functions and perform the optimization SWIF: First-order linear perturbation theory Determine the configuration that results in the highest k eff with given fissile amount Redistribute the fissile material and remove/redistribute other materials Determine the configuration that yields the specified k eff with minimum amount of fissile material Remove/redistribute the fissile and other materials
SMORES Example Spherical fissile system with 239 PuO2, polyethylene, and beryllium Eight equal-thickness zones Flat fissile material profile (initial k eff = 0.7) Determine maximum k eff for the system H2OH2O
SMORES Example (Cont.)
When will SCALE 5 be released? My final answer: When we have funding When it’s ready Sometime in 2003 You will be among the first to know if you join the SCALE News List