Lloyd M J, Martinez E, Messina L, Nguyen-Manh D
Department of Materials, University of Oxford, Parks Road, Oxford, OX13PH, United Kingdom.
United Kingdom Atomic Energy Authority, Culham Science Centre, Abingdon, Oxfordshire, OX143DB, United Kingdom.
J Phys Condens Matter. 2021 Sep 15;33(47). doi: 10.1088/1361-648X/ac1ec4.
In this study, radiation-induced precipitation of transmutation products is addressed via the development of a new solute and vacancy concentration dependant Ising model for the W-Re-Os system. This new model includes interactions between both Os and Re atoms with vacancies, thus facilitating more representative simulations of transmutation in fusion reactor components. Local solute concentration dependencies are introduced for the W-Re, W-Os and Re-Os pair interactions. The model correctly accounts for the repulsion between small clusters of vacancies and the attraction between larger clusters/voids, via the introduction of local vacancy concentration dependant interaction coefficients between pairs of atoms and vacancies. To parameterise the pair interactions between atoms and/or vacancies, the enthalpy of mixing, Δ, for various configurations and solute/defect concentrations, was calculated using density functional theory, within 6 binary systems: W-Re, W-Os, Re-Os, W-vacancy, Re-vacancy and Os-vacancy. The new energy model was implemented into the SPPARKS Monte Carlo code, and successfully used to predict the formation of voids decorated with Re and Os solute atoms. Analysis suggests that there is a strong thermodynamic tendency for Os to bind to these voids with a comparatively weaker binding from Re atoms. The binding energies of various solute/vacancy clusters were calculated and showed that Re and Os solute atoms tend to stabilise small clusters of vacancies, increasing the attractive binding energy between the constituents.
在本研究中,通过开发一种新的、依赖于溶质和空位浓度的W-Re-Os系统伊辛模型,来探讨辐射诱导的嬗变产物沉淀。这个新模型包括Os和Re原子与空位之间的相互作用,从而有助于对聚变反应堆部件中的嬗变进行更具代表性的模拟。引入了W-Re、W-Os和Re-Os对相互作用的局部溶质浓度依赖性。该模型通过引入原子对与空位之间依赖于局部空位浓度的相互作用系数,正确地解释了小空位团簇之间的排斥以及较大团簇/空隙之间的吸引。为了参数化原子和/或空位之间的对相互作用,使用密度泛函理论在6个二元系统(W-Re、W-Os、Re-Os、W-空位、Re-空位和Os-空位)中计算了各种构型和溶质/缺陷浓度下的混合焓Δ。新的能量模型被应用到SPPARKS蒙特卡罗代码中,并成功用于预测由Re和Os溶质原子装饰的空隙的形成。分析表明,Os有很强的热力学倾向与这些空隙结合,而Re原子的结合相对较弱。计算了各种溶质/空位团簇的结合能,结果表明Re和Os溶质原子倾向于使小空位团簇稳定,增加了组分之间的吸引结合能。