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- W3100202234 abstract "Scalar relativistic corrections to atomization energies of 1st-and 2nd-row molecules can be rationalized in terms of a simple additive model, linear in changes in atomic s populations. In a sample of 200 first-and second-row molecules, such a model can account for over 98% of the variance (99% for the first-row subset). The remaining error can be halved again by adding a term involving the change in atomic p populations: those coefficients need not be fitted but can be fixed from atomic electron affinity calculations. This model allows a fairly accurate a priori estimate for the importance of scalar relativistic corrections on a reaction energy, at essentially zero computational cost. While this is not a substitute for explicit calculation of Douglas-Kroll-Hess (DKH) or exact two-component (X2C) relativistic corrections, the model offers an interpretative tool for the chemical analysis of scalar relativistic contributions to reaction energies." @default.
- W3100202234 created "2020-11-23" @default.
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- W3100202234 date "2018-08-17" @default.
- W3100202234 modified "2023-09-24" @default.
- W3100202234 title "A simple model for scalar relativistic corrections to molecular total atomisation energies" @default.
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- W3100202234 doi "https://doi.org/10.1080/00268976.2018.1509147" @default.
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