Fast estimation of intersystem crossing rate constants of radical pairs

被引:1
|
作者
Valiev, Rashid R. [1 ]
Nasibullin, Rinat T. [1 ]
Juttula, Severi [1 ]
Kurten, Theo [1 ]
机构
[1] Univ Helsinki, Dept Chem, POB AI Virtanens plats 1 55, Helsinki 00014, Finland
基金
芬兰科学院;
关键词
SELF-REACTIONS; OXIDATION; MECHANISM; HYDROCARBONS; MOLECULES; CHEMISTRY; KINETICS;
D O I
10.1039/d4nj03110e
中图分类号
O6 [化学];
学科分类号
0703 ;
摘要
The spin-flip or intersystem crossing (ISC) process plays a main role in photophysics and photochemistry. ISC is the radiationless electronic transition between singlet and triplet states. ISC is responsible for phosphorescence and the chemical reaction which happens only in the electronic state with the specific spin. One specific and challenging case is the formation of accretion products in peroxy radical cross-reactions, recently demonstrated to be important in atmospheric chemistry. Here, the ISC or spin-flip occurs between triplet and singlet states of a complex of two alkoxy radicals (RO center dot & ctdot;R ' O-center dot). The complex is initially formed in a triplet state, while the formation of the ROOR ' accretion product can only happen on the singlet surface. Therefore, the ISC rate dictates the rate of this reaction. We developed a fast algorithm to calculate ISC rate constants (kISC) between the lowest electronic states of alkoxy radical pairs. The kISC calculation requires the spin-orbital coupled interaction matrix elements (SOCME) and the excitation energies (E) of the involved electronic states. The E and SOCME are calculated quickly using the CASSCF level of theory, and a novel analytical expression, respectively. Finally, the kISC calculation is performed efficiently; within 5-60 seconds even for radical pairs with the large substituents such as CH3(CO)CH2O(center dot) and HOCH2CH(O-center dot)CH2CH3. This algorithm is applied to a large number of radical pairs with different substituents, and the kISC is calculated for 95 875 radical pair conformers using this algorithm. It provides an opportunity to generate large amounts of data (input and output values, e.g. geometries and associated ISC rates) quickly. Therefore, we believe that the fast algorithm can be useful not only for photophysical calculations, but also for Big Data creation to implement machine learning methods. The spin-flip or intersystem crossing (ISC) process plays a main role in photophysics and photochemistry.
引用
收藏
页码:18314 / 18319
页数:6
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