Petrenko Taras, Neese Frank
Lehrstuhl für Theoretische Chemie, Universität Bonn, Wegelerstrasse 12, 53115 Bonn, Germany.
J Chem Phys. 2007 Oct 28;127(16):164319. doi: 10.1063/1.2770706.
A general method for the simulation of absorption (ABS) and fluorescence band shapes, resonance-Raman (rR) spectra, and excitation profiles based on the time-dependent theory of Heller is discussed. The following improvements to Heller's theory have been made: (a) derivation of new recurrence relations for the time-dependent wave packet overlap in the case of frequency changes between the ground and electronically excited states, (b) a new series expansion that gives insight into the nature of Savin's preresonance approximation, (c) incorporation of inhomogeneous broadening effects into the formalism at no additional computational cost, and (d) derivation of a new and simple short-time dynamics based equation for the Stokes shift that remains valid in the case of partially resolved vibrational structure. Our implementation of the time-dependent theory for the fitting of experimental spectra and the simulation of model spectra as well as the quantum mechanical calculation of the model parameters is discussed. The implementation covers all electronic structure approaches which are able to deliver ground- and excited-state energies and transition dipole moments. The technique becomes highly efficient if analytic gradients for the excited-state surface are available. In this case, the computational cost for the simultaneous prediction of ABS, fluorescence, and rR spectra is equal to that of a single excited-state geometry optimization step while the limitations of the short-time dynamics approximation are completely avoided. As a test case we discuss the well-known case of the strongly allowed 1 (1)A(g) --> 1 (1)B(u) transition in 1,3,5 trans-hexatriene in detail using method ranging from simple single-reference treatments to elaborate multireference electronic structure approaches. At the highest computational level, the computed spectra show the best agreement that has so far been obtained with quantum chemical methods for this problem.
讨论了一种基于海勒含时理论模拟吸收(ABS)和荧光带形状、共振拉曼(rR)光谱以及激发轮廓的通用方法。对海勒理论进行了以下改进:(a)在基态和电子激发态之间频率变化的情况下,推导了含时波包重叠的新递推关系;(b)给出了一种新的级数展开,深入了解了萨文预共振近似的本质;(c)以不增加计算成本的方式将非均匀展宽效应纳入形式体系;(d)推导了一种新的、简单的基于短时动力学的斯托克斯位移方程,该方程在部分分辨的振动结构情况下仍然有效。讨论了我们对含时理论的实现,用于拟合实验光谱和模拟模型光谱以及模型参数的量子力学计算。该实现涵盖了所有能够提供基态和激发态能量以及跃迁偶极矩的电子结构方法。如果有激发态表面的解析梯度,该技术将变得非常高效。在这种情况下,同时预测ABS、荧光和rR光谱的计算成本等同于单个激发态几何优化步骤的成本,同时完全避免了短时动力学近似的局限性。作为一个测试案例,我们详细讨论了1,3,5-反式己三烯中强允许的1 (1)A(g) --> 1 (1)B(u)跃迁这一著名案例,使用的方法从简单的单参考处理到精细的多参考电子结构方法。在最高计算水平下,计算得到的光谱与量子化学方法在该问题上迄今获得的最佳结果吻合。