首页|利用激光溅射超声分子束对激发态SiO分子在193nm下的光解动力学成像研究

利用激光溅射超声分子束对激发态SiO分子在193nm下的光解动力学成像研究

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SiO是星际空间中广泛分布的一种分子.由于该分子具有较高的解离能,之前的研究均聚焦于其光谱研究而鲜少聚焦在光解动力学研究上.本文利用时间切片-离子速度成像技术,观察到了高振动激发的电子基态SiO(X1∑+,v=13~18)在193 nm下激发至电子激发态SiO(A1∏,E1∑+)并解离为Si(3P)+O(3P)的光解过程.此高振动激发的SiO分子由激光溅射固体硅棒并由氧气作为反应气和载气获得.根据实验得到的光解产物动能能谱,确定了SiO分子的解离能De(Si-O)为67253±110 cm-1(8.34±0.01 eV).SiO的光解动力学加深了对富含岩石的流星在地球大气中燃烧时的硅化学反应,以及燃烧所产生的SiO在吸收紫外区光子后的光解反应机理的理解.
Imaging Photodissociation Dynamics of Excited SiO Molecules at 193 nm with Laser Ablation Supersonic Beam
SiO is a wide-spread molecule found in interstel-lar space.Previous research has primarily focused on its spectroscopy,while its photodissociation dynamics is elusive to study due to high dissocia-tion energy.Using time-sliced ion velocity imag-ing technique,we observed the Si(3P)+O(3P)photodissociation process resulting from the exci-tation of highly vibrationally excited SiO(X1E+,v=13-18)molecules to the SiO(A1∏,E1∑+)states at 193 nm.The vibrationally excited SiO molecules were generated via laser ablation of sili-con rod with the collision of the oxygen molecular beam acting as carrier gas and reaction gas.The bond dissociation energy De(Si-O)is deter-mined to be 67253±110 cm-1(8.34±0.01 eV)based on the kinetic energy distribution spec-trum.The SiO photodissociation study has deepened our understanding of the mechanisms of silicon chemistry for silica-rich rocky meteors as they burn in the Earth's atmosphere,and the dissociation of SiO from ablation of meteoroids following ultraviolet photon absorption.

PhotodissociationSiOVibrational excitationLaser ablationTime-sliced ion velocity imaging

马玉杰、李芳芳、闫东、徐昂、周倜、刘嘉兴、王凤燕

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复旦大学化学系,上海市分子催化和功能材料重点实验室,能源材料化学协同创新中心,上海 200438

光解 SiO 振动激发 激光溅射 时间切片-离子速度成像

2024

化学物理学报(英文版)
中国物理学会

化学物理学报(英文版)

CSTPCDEI
影响因子:0.162
ISSN:1674-0068
年,卷(期):2024.37(6)