Department of Chemistry, Washington State University, Pullman, Washington 99164, USA.
J Chem Phys. 2013 Sep 7;139(9):094302. doi: 10.1063/1.4818725.
Atomization energies were calculated using explicitly correlated coupled cluster methods with correlation consistent basis sets for a series of 19 small molecules containing 3d transition metal atoms. The atomization energies were calculated using a modified Feller-Peterson-Dixon approach in which CCSD(T) complete basis set (CBS) limits were obtained using extrapolations of aVTZ∕aVQZ CCSD(T)-F12b correlation energies, and then a series of additive contributions for relativity, core correlation, higher order correlation, and zero-point vibrations were included. The frozen-core CBS limits calculated with F12 methods closely matched the more computational expensive conventional awCVQZ∕awCV5Z CBS extrapolations, with a mean unsigned deviation of just 0.1 kcal∕mol. In particular, the CCSD(T∗)-F12b∕aVDZ and aVTZ atomization energies were more accurate on average than the conventional CCSD(T)∕aVQZ and aV5Z results, respectively. In several cases the effects of higher order correlation beyond CCSD(T), as judged by CCSDT and CCSDT(Q)Λ calculations, were greater than 1 kcal∕mol, reaching 4.5 kcal∕mol for CrO3. For the 16 molecules of this study with experimental uncertainties of ∼3.5 kcal∕mol or less, the final composite heats of formation have a mean unsigned deviation (MUD) from experiment of just 1.3 kcal∕mol, which is slightly smaller than the average of the experimental uncertainties, 1.8 kcal∕mol. The root mean square deviation (RMS) is only slightly larger at 1.7 kcal∕mol. Without the contributions due to higher order correlation effects, the MUD and RMS rise to 2.1 and 2.8 kcal∕mol, respectively. To facilitate the F12 calculations, new (aug-)cc-pVnZ∕MP2Fit (n = Q, 5) and (aug-)cc-pwCVTZ∕MP2Fit auxiliary basis sets were also developed for the transition metal atoms.
使用包含 3d 过渡金属原子的 19 种小分子系列的显式相关耦合簇方法和相关一致基组计算了原子化能。使用经过修正的 Feller-Peterson-Dixon 方法计算了原子化能,其中 CCSD(T)完全基组 (CBS) 极限值是通过对 CCSD(T)-F12b 相关能量进行 VTZ∕aVQZ 的外推得到的,然后加入了一系列相对论、核心相关、高阶相关和零点振动的加和贡献。使用 F12 方法计算的冻结核 CBS 极限值与更具计算成本的传统 awCVQZ∕awCV5Z CBS 外推值非常吻合,平均未签名偏差仅为 0.1 kcal∕mol。特别是,与传统的 CCSD(T)∕aVQZ 和 aV5Z 结果相比,CCSD(T∗)-F12b∕aVDZ 和 aVTZ 的原子化能平均更为准确。在某些情况下,超越 CCSD(T)的高阶相关效应,如 CCSDT 和 CCSDT(Q)Λ 计算所判断的那样,超过 1 kcal∕mol,对于 CrO3 达到 4.5 kcal∕mol。对于本研究中的 16 种分子,其实验不确定度约为 3.5 kcal∕mol 或更小,最终的复合生成热的平均未签名偏差 (MUD) 仅为实验值的 1.3 kcal∕mol,略小于实验不确定度的平均值,即 1.8 kcal∕mol。均方根偏差 (RMS) 仅略大,为 1.7 kcal∕mol。如果没有高阶相关效应的贡献,MUD 和 RMS 将分别上升至 2.1 和 2.8 kcal∕mol。为了方便 F12 的计算,还为过渡金属原子开发了新的 (aug-)cc-pVnZ∕MP2Fit(n = Q,5)和(aug-)cc-pwCVTZ∕MP2Fit 辅助基组。