* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download handout - JAEA Nuclear Data Center
Density of states wikipedia , lookup
Energy harvesting wikipedia , lookup
Eigenstate thermalization hypothesis wikipedia , lookup
Work hardening wikipedia , lookup
Heat transfer physics wikipedia , lookup
Tight binding wikipedia , lookup
Energy applications of nanotechnology wikipedia , lookup
Radiation damage wikipedia , lookup
Nuclear Data and Materials Irradiation Effects - Analysis of irradiation damage structures and multiscale modeling - Toshimasa Yoshiie Research Reactor Institute, Kyoto University Comparison of irradiation effects between different facilities • Power reactors Research reactors • Neutron irradiation Ion irradiation Electron irradiation DPA (Displacement per atom) The number of displacement of one atom during irradiation DPA dose not represent the effect of cascades Estimation of irradiation damage • Ion irradiation 100MeV He,1018ions/cm2 • Neutron irradiation 1018n/cm2 ( >1MeV or >0.1MeV) • Displacement par atom (dpa) = αx deposited energy in crystal lattice 2x threshold energy of atomic displacement Kinchin-Pease model EP E DPA is the number of displacement for 1 atom during irradiation Frenkel pair formation Cascade formation Cascade Example of MD Simulation 40keV cascade of iron at 100K Clustering of Point Defects Stress field Interstitial Type Dislocation Loops in FCC Interstitial type dislocation loops in Al Voids Embrittlement Materials with no voids Materials with voids Stacking Fault Tetrahedra Stacking Fault Tetrahedra Cascade Damage High energy Particle Cascade Vacancy rich area Subcascades Interstitial rich area Nucleation of defect clusters Comparison of Subcascade Structures by Thin Foil Irradiation 14MeV neutrons at 300K. Neutron PKA TPKA 4mn E sin 2 , MT 2 Z4 Au, KENS irradiation and 14 MeV irradiation at room temperature KENS neutrons 14MeV neutrons 13 14MeV neutron irradiated Cu 14MeV neutron irradiated Cu 14MeV neutron irradiated Cu 14MeV neutron irradiated Cu Temperature Effects of Cascade Damage Lower temperature Subcascades Higher temperature Subcascades fuse into a large cluster Thin foil Irradiated Au by Fusion Neutrons A group of SFTs Subcascade structures A large SFT Cascade fuses into one SFT Fission-fusion Correlation of SFT in Au 0.017dpa 0.044dpa Large SFTs Small SFTs High number density of SFTs Low number density of SFTs Fusion neutrons Fission neutrons 563K 573K PKA Energy Spectrum Analysis N SFT E TH d ( E ) dE dE NSFT: the concentration of SFTs observed α: the SFT formation efficiency :the neutron fluence d :the dE α= 0.05 ETH = 80keV differential crosssection for PKA ETH :threshold energy for SFT formation MULTI-SCALE MODELING OF IRRADIATION EFFECTS IN SPALLATION NEUTRON SOURCE MATERIALS Toshimasa Yoshiie1, Takahiro Ito 2, Hiroshi Iwase 3, 4, Masayoshi Kawai3, Ippei Kishida4, Satoshi Yoshihisa Kaneko 5, Futoshi Shimizu5, Kunieda5, Koichi Sato41, Satoshi Shimakawa 6, Tokio Fukahori5, Satoshi Hashimoto , Naoyuki Hashimoto Yukinobu Watanabe7, Qiu Xu1, Shiori Ishino8 2 1Research Reactor Institute, Kyoto University Department of Mechanical Engineering, Toyohashi University of Technology High Energy Accelerator Research Organization Osaka City University 5Japan Atomic Energy Agency 6Hokkaido University 7 Kyushu University 8Univerity of Tokyo Motivation • Spallation neutron source and Accelerator Driven System (ADS) are a coupling of a target and a proton accelerator. High energy protons of GeV order irradiated in the target produce a large number of neutrons. • The beam window and the target materials thus subjected to a very high irradiation load by source protons and spallation neutrons generated inside the target. • At present, there are no materials that enable the window to be operational for the desired period of time without deterioration of mechanical properties. Importance of GeV Order Proton Irradiation Effects in Materials • Spallation neutron source J-PARC (Japan) SNS (USA) • Accelerator driven system (in the planning stage ) 800MW ADS (Minor Actinide transmutation, Japan Atomic Energy Agency) 5MW Accelerator driven subcritical reactor (Kyoto University, neutron source) Purpose and outline • In this paper, mechanical property changes of nickel by 3 GeV protons were calculated by multi-scale modeling of irradiation effects. Nickel is considered to be a most simple model material of austenitic stainless steels used in beam window. The code consists of four parts. • Nuclear reaction, the interaction between high energy protons and nuclei in the target is calculated by PHITS code from 10-22 s. • Atomic collision by particles which do not cause nuclear reactions is calculated by molecular dynamics and k-Monte Carlo. As the energy of particles is high, subcascade analysis is employed. In each subcascade, the direct formation of clusters and the number of mobile defects are estimated. • Damage structure evolution is estimated by reaction kinetic analysis. • Mechanical property change is calculated by using 3D discrete dislocation dynamics (DDD). Stress-strain curves of high energy proton irradiated nickel are obtained. PHITS High energy particle Size (m) Vacancy 10-20 10-15 10-10 10-5 100 105 1010 Data flow between each code Nuclear reactions (PHITS code) Primary knock-on energy spectrum Atomic collisions (Molecular dynamics) Point defect distribution Damage structural evolutions (Reaction kinetic analysis) Concentration of defect clusters Mechanical property change (Three-dimensional discrete dislocation dynamics) Stress-strain curve 1. Nuclear Reaction Nucleation rate of neutrons, photons, charged particles and PKA energy spectrum by them Ni 6 [10-10] 10-8 5 10-9 4 10-10 10 3 2 -11 10-12 10-3 1 -2 -1 10 10 10 PKA energy (MeV) 0 0 101 Number of PKA energy (left) and energy deposition by PKA (right) in 3 GeV proton irradiated Ni of 3 mm in thickness. Energy deposition by PKA (MeV) 3GeV protons Number of PKA / proton Result of PHITS Simulation Subcascade Analysis Large cascades are divided into subcascades. In the case of Ni, subcascade formation energy is calculated to be 10 keV. 6 [10-10] 10-8 5 10-9 4 10-10 3 2 10-11 10-12 10-3 1 10-2 10-1 100 PKA energy (MeV) 0 101 Energy deposition by PKA (MeV) Cascade Number of PKA / proton The number of subcascasdes are obtained from the result of PHITS. Number of subcascades by deposition of energy T N SC T 2TSC TSC : Subcascade formation energy Total number of subcascades t TMAX T SC dσ N SC dT dT 2. Atomic Collision Simulation by MD Calculation Condition Potential model by Daw and Baskes (1984) NVE ensemble ( i.e., number of the atoms, cell volume and energy were kept constant) 35x35x35 lattices (171500 atoms) in a z simulation cell y Periodic boundary condition for the x three directions 35a0 Initial condition : equilibrium for 50 ps at 300 K, 0MPa a0 : lattice constant at 300 K PKA energy:10keV MD runs with different initial directions of PKA ( none of which were parallel to the lattice vector.) Typical Distribution of Point Defects Marble : interstitial atoms,Violet :Vacancy cites 0.006ps 0.025ps 7.395ps 18.40ps 1.132ps 96.38ps Results of MD Calculation Number of vacancies Number of vacancies 105 104 103 102 101 100 10-1 10-3 800 10-2 10-1 100 Time (ps) 101 102 Temperature (K) Cascades terminated within 10~20ps 700 On average17 vacancies, 17 interstitials were produced. 600 Formation of defect clusters is calculated by k-Monte Carlo. 500 Clusters of three point defects are formed. 400 3. Damage Structure Evolution by Reaction Kinetic Analysis In order to estimate damage structural evolution, the reaction kinetic analysis is used. Assumptions used in the calculation are as follows: (1) Mobile defects are interstitials, di-interstitials, tri-interstitials, vacancies and divacancies. (2) Thermal dissociation is considered for di-interstitials, tri-interstitials di-vacancies and tri-vacancies, and point defect clusters larger than 4 are set for stable clusters. (3) Time dependence of 10 variables, concentration of interstitials, di-interstitials, triinterstitials, interstitial clusters (interstitial type dislocation loops), vacancies, divacancies, tri-vacancies, vacancy clusters (voids), total interstitials in interstitial clusters and total vacancies in vacancy clusters are calculated to 10 dpa. (4) Interstitial clusters (three interstitials) and vacancy clusters (three vacancies) are also formed directly in subcascades. (5) Materials temperature is 423 K during irradiation. The result is as follows, Formation of vacancy clusters of four vacancies, concentration: 0.59x10-3, Dislocation density: 1.1x10-9cm/cm3. Reaction Kinetic Analysis CI : Interstitial concentration (fractional unit). CV : Vacancy concentration Z : Cross section of reaction M: Mobility dCI 2 PI 2Z I , I M I CI Z I ,V ( M I M V )CI CV dt damage production I-I recombination mutual annihilation Z I , IC M I CI S I Z I ,VC M I CI SV M I CI CS ......... absorption by loops absorption by voids annihilation of interstitials at sink 4. Estimation of Mechanical Property Changes (Plastic Deformation of Metals) t Plastic Deformation of Metals Dislocation Glide along Slip Planes t Work Hardening ↓ Motions of Dislocation Lines e Calculation of Dislocation Motions Motions of Curved Dislocations External Stress Elastic Interaction between Dislocations Line Tension Very Complicated ! Division of a Dislocation Line ↓ Discrete Dislocation Dynamics (DDD) Simulation 3D-Discrete Dislocation Dynamics Edge+Screw Dislocation Model Devincre (1992~) Stresses from another segment External Stress Mixed Dislocation Model Zbib, et al (1998~) Schwarz et al Fivel et al ,Cai et al Line tension Peach-Koehler Force Dislocation Velocity b Connection of Dislocation Segments with Mixed Characters Model Crystal and Mobile Dislocation Ni: shear modulus = 76.9 Gpa Poisson’s ratio = 0.31 Burgers vector = 0.24916 nm Stress axis = [1 0 0] Mobile dislocation slip plane=(1 1 1) slip vector=[1 0 1] Obstacles(void) 0.593×10-3 void/ atom the density along the slip plane : 1.10x104 void / μm2 0.14μm 0.14μm 0.14μm Interaction between Dislocation and void Detrapping angle Determination of Detrapping Angle (Statistic Energy Calculation Method) ( l l l) (Ī l 0) void (Ī Ī 2) [lll] [ Ī Ī 2] [ Ī l 0] Stress Size and orientation of model lattice used for Static energy calculation of dislocation movement. b is the Burgers vector. Stable atomic position is determined by an effective medium theory (EMT) potential for Ni fitted by Jacobsen et al. [K. W. Jacobsen, P. Stoltze, J. K. Norskov, Surf. Sci. 366 (1996) 394]. Determination of Detrapping Angle between Edge Dislocations and 4 Vacancies -10 0 10 10 20 10 20 10 20 10 Motion of dislocation near the slip plane under shear stress. X axis and Y axis are by atomic distance. In the left figure, a dislocation is separated into two partials. Four vacancies are at (16.0, 0.722, -0.408), (15.5, -0.144, -0.408), (16.0, 0.144, 0.408) and (15.5, 1.01, 0.408). Other figures indicate only right partial. 20 10 20 10 0 -10 65 ° 10 20 Dislocation Motion by DDD Simulation (no void) 400MPa 600MPa 700MPa Dislocation motion in the crystal with randomly-distributed voids Normal stress 0MPa 200MPa 300MPa 400MPa 500MPa 600MPa 650MPa 700MPa 750MPa 800MPa Stress-Strain Curves Calculated with DDD Simulation Plastic shear strain gp = A b / V Plastic strain ep = gp Sf A: area swept by a dislocation b: Burgers vector V: volume of model crystal (x10-6) Sf: Schmid factor Summary Importance of nuclear data for materials irradiation effects was shown. DPA is not good measure of irradiation damage. PKA energy spectrum is more useful to analyze damage structures. As an example of the analysis, the mechanical property change in Ni by 3 GeV proton irradiation was calculated and preliminary results were obtained. Nuclear reactions : PHITS PKA energy spectrum Atomic collision : MD, k-Monte Carlo, Subcascade analysis. The number of point defects and clusters in the subcascade Damage structure evolution : Reaction kinetic analysis Void density, Dislocation density Mechanical properties : Discrete dislocation dynamics Statistic energy calculation Stress strain curve Important data for materials irradiation effects High energy particles Primary knock on atom energy spectrum Formation rate of atoms by nuclear reactions High energy particle energy spectrum