Dantus Marcos
Department of Chemistry, Michigan State University, East Lansing, MI 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA.
Science. 2024 Aug 9;385(6709):eadk1833. doi: 10.1126/science.adk1833.
The chemical composition of the interstellar medium and planetary atmospheres is constantly in flux as atoms and molecules collide and interact with high-energy particles such as electrons, protons, and photons. These transformative processes ultimately lead to the coalescence of molecules and eventually the birth of stars. Our understanding of these chemical ecosystems relies on models that synthesize data from gas-phase experiments, providing insights into reaction cross sections. This Review examines efforts to delve into the fundamental bond-forming and bond-breaking dynamics that occur during bimolecular and electron-initiated reactions. These experiments involve clever approaches to establish a time reference and the collision geometry necessary for tracking atomic motion with femtosecond time resolution. Findings from these efforts enhance present models and improve predictions for molecule-molecule and electron-molecule collisions.
星际介质和行星大气的化学成分不断变化,因为原子和分子与电子、质子和光子等高能粒子发生碰撞和相互作用。这些转化过程最终导致分子聚合并最终形成恒星。我们对这些化学生态系统的理解依赖于从气相实验中合成数据的模型,从而深入了解反应截面。本综述探讨了深入研究双分子反应和电子引发反应中发生的基本成键和断键动力学的努力。这些实验采用了巧妙的方法来建立时间参考以及以飞秒时间分辨率跟踪原子运动所需的碰撞几何结构。这些研究成果改进了现有模型,并提高了对分子 - 分子和电子 - 分子碰撞的预测能力。