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CUMULATIVE REACTION PROBABILITY VIA TRANSITION STATE WAVE PACKETS

机译:过渡态波包的累积反应概率

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A new time-dependent approach to the cumulative reaction probability, N(E), has been developed based on the famous formulation given by Miller and co-workers [J. Chem. Phys. 79, 4889 (1983)], N(E) = [(2 pi)(2)/2] tr[delta(E-H)F delta(E-H)F]. Taking advantage of the fact that the flux operator has only two nonzero eigenvalues, we evaluate the trace efficiently in a direct product basis of the first flux operator eigenstates and the Hamiltonian eigenstates on the dividing surface (internal states). Because the microcanonical density operator, delta(E-H), will eliminate contributions to N(E) from an internal state with the energy much higher than the total energy E, we can minimize the number of internal states required by choosing a dividing surface with the lowest density of internal states. If the dividing surface is located in an asymptotic region, one just needs to include all the open channels, i.e., with internal energy lower than the total energy. Utilizing the Fourier transform for delta(E-H), we can obtain the information for all the energies desired by propagating these wave packets once. Thus the present approach will be much more efficient than the initial state selected wave packet (ISSWP) approach to N(E) for systems with many rotation degrees of freedom because the density of states in asymptotic region for such systems is much higher than that in the transition state region. With the present method one can also calculate the cumulative reaction probability from an initial state (or to a final state) by locating the second flux operator in the corresponding asymptotic region. This provides an alternative to the ISSWP approach which may be more efficient if the reaction probabilities from a large number of initial states are desired. The method is applied to the 3D H + H-2 (even rotation) reaction for J=0 by locating the first dividing surface in the transition state region. The demonstration also shows an aspect less than ideal; the contribution to N(E) from a wave packet may be slightly larger than 1 or slightly smaller than 0, making it improper to interpret the contribution as a probability. (C) 1996 American Institute of Physics. [References: 54]
机译:基于米勒及其同事给出的著名公式,已经开发了一种新的时间依赖性累积反应概率方法N(E)。化学物理79,4889(1983)],N(E)= [(2 pi)(2)/ 2] tr [delta(E-H)F delta(E-H)F]。利用通量算子只有两个非零特征值的事实,我们在分割面上的第一通量算子本征态和哈密顿本征态(内部态)的直接积基础上有效地评估了轨迹。由于微规范密度算子delta(EH)将消除内部状态对N(E)的贡献,该内部状态的能量远高于总能量E,因此我们可以通过选择一个具有内部状态的最低密度。如果分隔表面位于渐近区域,则只需要包括所有明渠,即内部能量低于总能量。利用delta(E-H)的傅立叶变换,我们可以通过传播这些波包一次来获得所有所需能量的信息。因此,对于具有许多旋转自由度的系统,本方法比针对N(E)的初始状态选择波包(ISSWP)方法效率更高,这是因为此类系统的渐近区域中的状态密度大大高于N(E)。过渡状态区域。通过本方法,还可以通过将第二通量算子定位在相应的渐近区域中来计算从初始状态(或最终状态)的累积反应概率。这提供了ISSWP方法的替代方法,如果需要大量初始状态的反应概率,则可能更有效。通过将第一个分割面置于过渡态区域中,将该方法应用于J = 0的3D H + H-2(均匀旋转)反应。演示还显示了一个不理想的方面。波包对N(E)的贡献可能略大于1或略小于0,这使得将贡献解释为概率是不合适的。 (C)1996年美国物理研究所。 [参考:54]

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