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首页> 外文期刊>International Journal of Quantum Chemistry >Simulating X-ray absorption spectra with complete active space self-consistent field linear response methods
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Simulating X-ray absorption spectra with complete active space self-consistent field linear response methods

机译:采用完整的主动空间自洽励磁响应方法模拟X射线吸收光谱

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In this work, two approaches for simulating X-ray absorption (XA) spectra with the complete active space self-consistent field (CASSCF) linear response (LR) method are introduced. The first approach employs the well-known core-valence separation (CVS) approximation, which is predominantly used by many other electronic structure methods for simulating X-ray spectra. The second ansatz uses the harmonic Davidson algorithm for finding interior eigenvalues that lie close to a target excitation energy shift and virtually solves a shifted-and-inverted (S&I) generalized eigenvalue problem. LR-CASSCF K-edge transition energies are systematically blueshifted though have consistently smaller errors than those of the CAS or restricted active space (RAS) configuration interaction (CI) methods. For simple molecules at which the core hole can only be created at a single site, the state-specific RASSCF or n-electron valence second-order perturbation theory/RASCI gave more accurate principal K-edge excitation energies. If the core hole can be created at multiple sites, the LR-CASSCF approaches perform much better than RASSCF. Moreover, we observed that the LR-CASSCF variants were the only MR methods discussed here that predicted correctly the order of O K-edge features in the ozone molecule and the permanganate ion. The peak separation of edge features in ozone was as accurate as with equation-of-motion coupled cluster singles and doubles. The error of the CVS approximation turned out to be very system dependent and in some cases amounted up to 1.0 eV for the K-edge excitation energies. Those CVS errors are still acceptable if one considers the observed deviation from the experimental reference by 5-11 eV. The deviations made in the XAS intensities were even more pronounced. CVS and the full S&I oscillator strengths could differ even by a factor of 2.8. Since the S&I approach is at least as efficient as the LR-CASSCF method for valence excitations, future endeavors to improve the accuracy by accounting for dynamic correlation could be built on top of the full S&I approach.
机译:本文介绍了用完全有源空间自洽场(CASSCF)线性响应(LR)方法模拟X射线吸收(XA)光谱的两种方法。第一种方法采用众所周知的核价分离(CVS)近似,这主要被许多其他电子结构方法用于模拟X射线光谱。第二种安萨茨算法使用谐波戴维森算法来寻找靠近目标激励能量偏移的内部特征值,实际上解决了偏移和反转(S&I)广义特征值问题。LR-CASSCF K边跃迁能被系统地蓝移,尽管其误差始终小于CAS或受限活动空间(RAS)组态相互作用(CI)方法的误差。对于核心空穴只能在单个位置产生的简单分子,特定于状态的RASSCF或n-电子价二阶微扰理论/RASCI给出了更精确的主K边激发能。如果可以在多个位置创建岩芯孔,LR-CASSCF方法的性能要比RASSCF好得多。此外,我们还观察到,LR-CASSCF变体是本文讨论的唯一能够正确预测臭氧分子和高锰酸盐离子中O K边缘特征顺序的MR方法。臭氧边缘特征的峰值分离与运动方程耦合的团簇单重和双重峰一样精确。CVS近似的误差非常依赖于系统,在某些情况下,K边激发能的误差高达1.0 eV。如果考虑到观测到的与实验参考值的偏差为5-11 eV,则这些CVS误差仍然可以接受。XAS强度的偏差更为明显。CVS和完整的S&I振荡器强度可能相差2.8倍。由于S&I方法至少与LR-CASSCF方法对价态激发的效率相同,未来通过考虑动态相关性来提高精度的努力可以建立在完整S&I方法之上。

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