论文标题
将机器学习和光谱结合到模拟反应性原子 +硅藻碰撞
Combining Machine Learning and Spectroscopy to Model Reactive Atom + Diatom Collisions
论文作者
论文摘要
对于反应性原子+硅硅碰撞的任意初始条件的产品平移,振动和旋转能量分布的预测在大气再进入中具有相当大的实际兴趣。由于众多可访问状态,从显式(准经典或量子)动力学研究中确定必要的信息是不切实际的。在这里,基于转换能量和产物振动状态的机器学习(ML)模型,该模型是根据基于Dunham扩展的光谱,RO振动耦合的能量表达来定量的,并在定量上进行了测试。这项工作中考虑的所有模型都重现了从准经典轨迹(QCT)模拟确定的最终状态分布,并使用$ r^2 \ sim 0.98 $。作为进一步的验证,由机器学习模型确定的热速率与显式QCT模拟的模型一致,并证明原子学细节是由机器学习保留的,这使得它们适合于更粗糙的模拟中的应用。更普遍的是,发现ML适合从混合计算/实验数据中设计强大而准确的模型,这些模型也可能在物理科学的其他领域中引起人们的关注。
The prediction of product translational, vibrational, and rotational energy distributions for arbitrary initial conditions for reactive atom+diatom collisions is of considerable practical interest in atmospheric re-entry. Due to the large number of accessible states, determination of the necessary information from explicit (quasi-classical or quantum) dynamics studies is impractical. Here, a machine-learned (ML) model based on translational energy and product vibrational states assigned from a spectroscopic, ro-vibrational coupled energy expression based on the Dunham expansion is developed and tested quantitatively. All models considered in this work reproduce final state distributions determined from quasi-classical trajectory (QCT) simulations with $R^2 \sim 0.98$. As a further validation, thermal rates determined from the machine-learned models agree with those from explicit QCT simulations and demonstrate that the atomistic details are retained by the machine learning which makes them suitable for applications in more coarse-grained simulations. More generally, it is found that ML is suitable for designing robust and accurate models from mixed computational/experimental data which may also be of interest in other areas of the physical sciences.