DOI: 10.1039/C9NR00967A, Paper
Fluorescence lifetime imaging technology is used to reveal the interaction between defects and exciton annihilation in monolayer WS2.
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A perturbation theory‐based algorithm for the iterative orbital update in complete active space self‐consistent‐field (CASSCF) calculations is presented. It is based on single‐excitation amplitudes obtained from a perturbative configuration interaction calculation using the Dyall Hamiltonian as a zeroth‐order Hamiltonian. These amplitudes are used for the construction of the exponential of an anti‐Hermitian matrix which can be used for the orbital update. Combined with DIIS, this approach leads to rapid convergence of the CASSCF iteration procedure.
A perturbation theory‐based algorithm for the iterative orbital update in complete active space self‐consistent‐field (CASSCF) calculations is presented. Following Angeli et al. (J. Chem. Phys. 2002, 117, 10525), the first‐order contribution of singly excited configurations to the CASSCF wave function is evaluated using the Dyall Hamiltonian for the determination of a zeroth‐order Hamiltonian. These authors employ an iterative diagonalization of the first‐order density matrix including the first‐order correction arising from single excitations, whereas the present approach uses the single‐excitation amplitudes directly for the construction of the exponential of an anti‐Hermitian matrix resulting in a unitary matrix which can be used for the orbital update. At convergence, the single‐excitation amplitudes vanish as a consequence of the generalized Brillouin's theorem. It is shown that this approach in combination with direct inversion of the iterative subspace (DIIS) leads to very rapid convergence of the CASSCF iteration procedure. © 2019 Wiley Periodicals, Inc.
A perturbation theory‐based algorithm for the iterative orbital update in complete active space self‐consistent‐field (CASSCF) calculations is presented. It is based on single‐excitation amplitudes obtained from a perturbative configuration interaction calculation using the Dyall Hamiltonian as a zeroth‐order Hamiltonian. These amplitudes are used for the construction of the exponential of an anti‐Hermitian matrix which can be used for the orbital update. Combined with DIIS, this approach leads to rapid convergence of the CASSCF iteration procedure.
A perturbation theory‐based algorithm for the iterative orbital update in complete active space self‐consistent‐field (CASSCF) calculations is presented. Following Angeli et al. (J. Chem. Phys. 2002, 117, 10525), the first‐order contribution of singly excited configurations to the CASSCF wave function is evaluated using the Dyall Hamiltonian for the determination of a zeroth‐order Hamiltonian. These authors employ an iterative diagonalization of the first‐order density matrix including the first‐order correction arising from single excitations, whereas the present approach uses the single‐excitation amplitudes directly for the construction of the exponential of an anti‐Hermitian matrix resulting in a unitary matrix which can be used for the orbital update. At convergence, the single‐excitation amplitudes vanish as a consequence of the generalized Brillouin's theorem. It is shown that this approach in combination with direct inversion of the iterative subspace (DIIS) leads to very rapid convergence of the CASSCF iteration procedure. © 2019 Wiley Periodicals, Inc.
A combination of statistical learning theory and optimization provides both theoretical results and implementable algorithms to solve real problems in machine learning. These results are successfully and flexibly applied to predict atomization energies in quantum chemistry by digging deeply the inner structure of loss functions and statistical errors. This approach is flexible even for traditional kernel ridge regression.
Machine learning promises to accelerate materials discovery by allowing computational efficient property predictions from a small number of reference calculations. As a result, the literature has spent a considerable effort in designing representations that capture basic physical properties. Our work focuses on the less‐studied learning formulations in this context in order to exploit inner structures in the prediction errors. In particular, we propose to directly optimize basic loss functions of the prediction error metrics typically used in the literature, such as the mean absolute error or the worst case error. In some instances, a proper choice of the loss function can directly reduce reasonably the prediction performance in the desired metric, albeit at the cost of additional computations during training. To support this claim, we describe the statistical learning theoretic foundations, and provide supporting numerical evidence with the prediction of atomization energies for a database of small organic molecules.

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Interest in organic radicals is fuelled by their potential role in designing organic materials and complex electronic structure. A multireference perturbative method with improved virtual orbitals has been used as an affordable, efficient and robust device for studying radicals. The method is tailored to tackle open‐ and closed‐shell states with the same accuracy. An intricate balance between different correlation effects is tangled in the accurate description of multiple states and their gaps.
IVO‐SSMRPT is an affordable and accurate type of state‐specific multireference perturbation (SSMRPT) theory that adds dynamic correlation energy to improved virtual orbital (IVO) complete active space configuration interaction (CASCI) wave functions using a single‐root parametrization of multi‐root Hilbert‐space ansatz. We applied it to many chemically important di‐ and tri‐radicals to analyze the geometries and electronic properties of spectroscopic interest for both closed‐ and open‐shell singlet‐ and nonsinglet ground as well as excited states. We observed that IVO‐SSMRPT identifies optimized geometries, splitting between multiplets and frequencies for several radicals that are similar to those displayed by current generation state‐of‐the‐art methods but with admiringly decreased computational effort. This study illustrates the importance of having an accurate treatment of both nondynamical and dynamical correlation effects when examining multiradical species. Chemically and spectroscopically relevant answers can be obtained using our computationally tractable method. Our method will be a serviceable avenue for portraying open‐shell interactions in other radicals.
NO dimerization on Ag and Cu clusters differs very much from that in gas phase. The nondynamical electron correlation effect is very small and the reaction easily occurs with nearly no barrier and significantly large exothermicity on these clusters.
Experimentally observed NO dimerization on Cu and Ag surfaces is surprising because binding energy of NO dimer is very small in gas phase. MRMP2, MP2 to MP4, CCSD(T), and DFT studies of NO dimerization on Ag2 and Cu2 clusters disclosed that the CCSD(T) method could be applied to this reaction on Ag2 and Cu2 unlike NO dimerization in gas phase which exhibits significantly large nondynamical electron correlation effect. Charge‐transfer (CT) from Ag2 and Cu2 to NO moieties plays important role in NN bond formation between two NO molecules. This CT considerably decreases nondynamical correlation effect. Also, the DFT method could be applied to this NO dimerization, if appropriate DFT functional is used; all pure functionals examined here and most of the hybrid functionals underestimated the activation barrier (E a), while only ωB97X provided E a similar to CCSD(T)‐calculated value. NO dimerization on similar Cu2 and Cu5 needs moderately larger E a than those on Ag2 and Ag5, because frontier orbital participating in the CT exists at lower energy in Cu2 and Cu5 than in Ag2 and Ag5. The E a decreases in the order Ag2 >> Ag38 > Ag7 ∼ Ag5 and the reaction energy (ΔE) is positive (endothermic) in Ag2 but significantly negative in Ag38, Ag7, and Ag5, indicating that various Ag clusters could be effective for NO dimerization except for Ag2. The decreasing order of E a and increasing order of exothermicity are attributed to increasing order of the frontier orbital energy of Ag2 < Ag38 < Ag7 ∼ Ag5. © 2018 Wiley Periodicals, Inc.