The authors present a new semiclassical phase-space approach to molecular dynamics that goes beyond the Born-Oppenheimer (BO) approximation. The key idea is to construct an electronic Hamiltonian that depends on both nuclear coordinates and momenta, rather than just coordinates as in the standard BO framework.
The authors demonstrate that this phase-space Hamiltonian can effectively account for electronic inertial effects, which are typically neglected in traditional surface hopping dynamics. Specifically, they show that under pure molecular translations and rotations, the phase-space approach prevents unphysical non-adiabatic transitions between electronic states that would occur in a standard BO surface hopping simulation.
The authors provide several numerical examples to support their theory, including the dynamics of a traveling hydrogen atom, rigid rotations of an H2+ molecule, and rotations of H2+ with spin-orbit coupling. These results highlight the power of the phase-space formalism in capturing electronic inertial effects and maintaining the conservation of total angular momentum, which is crucial for accurately modeling phenomena like spin-phonon interactions and chiral-induced spin selectivity.
The authors emphasize that the phase-space approach can be efficiently implemented using a linear combination of atomic orbitals (LCAO) basis, making it applicable to realistic-sized molecular systems. They also discuss future applications of this method, such as studying electron-phonon problems in condensed phase systems and exploring spin-dependent electron transfer processes.
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arxiv.org
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by Xuezhi Bian,... : arxiv.org 10-03-2024
https://arxiv.org/pdf/2410.01156.pdfDaha Derin Sorular