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Updated: Jan 14, 2026

Preparation of Enantiopure Non-Activated Aziridines and Synthesis of Biemamide B, D, and epiallo-Isomuscarine
Published on: June 13, 2022
Alchemical diastereomers from antisymmetric alchemical perturbations
O Anatole von Lilienfeld1,2,3,4,5,6, Giorgio Domenichini7,8
1Department of Chemistry, University of Toronto, St. George Campus, Toronto, Ontario M5S 1A1, Canada.
Abstract:
The energy difference between two iso-electronic systems can be approximated by the first order Hellmann-Feynman derivative with respect to the linear alchemical coupling parameter, evaluated using the electron density of the corresponding averaged Hamiltonian. This approximation is exact up to third order because even-order contributions cancel out. This finding holds for any iso-electronic compound pair (dubbed "alchemical diastereomers"), regardless of differences in configuration, composition, or energy, and consequently, relative energy estimates for all possible iso-electronic alchemical diastereomer pairs require only O(1) self-consistent field cycles for any given averaging reference Hamiltonian. We discuss the relation to the Verlet algorithm, alchemical harmonic approximation (AHA) [Krug et al., J. Chem. Phys. 162, 044101 (2025)], relative properties such as forces, ionization potential or electron affinities, and Levy's formula for relative energies among iso-electronic systems that uses the averaged electron density of the two systems [Levy, J. Chem. Phys. 70, 1573 (1979)]. Density functional theory based estimates accurately reflect trends in the charge-neutral iso-electronic diatomic molecule series with 14 protons (N2, CO, BF, BeNe, LiNa, HeMg, HAl), with systematically increasing errors. Using alchemical Hellmann-Feynman derivatives for toluene, we demonstrate the concept's broader applicability by estimating relative energies for all 36 possible alchemical diastereomer pairs from vertical iso-electronic charge-neutral antisymmetric BN doping of toluene's aromatic ring, with mean absolute errors of a few milli-Hartrees.
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