Matter Modeling Asked by Etienne Palos on August 19, 2021
I am new to the world of Molecular Dynamics, and am curious to know exactly what is considered to be an ab initio Molecular Dynamics (AIMD) method, and how do they work?
The seminal work by Roberto Car and Michele Parrinello, titled "Unified Approach for Molecular Dynamics and Density-Functional Theory" was published 35 years ago!
I have recently come across the following "types" of MD methods while reading some research papers:
If I am missing methods, which I am sure I am, please feel free to add them through an answer!
Also, it would be appreciated if one method is explained per answer, and is summarized in 2-3 paragraphs.
ab initio Ehrenfest Dynamics
From Li et.al.,2005, JCP
"The Born Oppenheimer (BO) and extended Lagrangian (EL) trajectories are founded on the assumption that a single electronic potential surface governs the dynamics. .. A major limitation of adiabatic trajectories is that they are not applicable to reactions involving nonadiabatic electronic processes, i.e., multiple potential-energy surfaces." (Ex: Conical Intersections)
To account for electronic adiabaticity, we solve the full time-dependent Schrödinger equation for both nuclear and electronic degrees of freedom. In Ehrenfest methodology, the adiabatic potential energy surface
$$ E_{eff} = langlePhi|hat{H_{el}}|Phirangle = sum_i |a_i|^2 E_i^2$$ Thus, the atoms evolve on an effective potential representing an average over the adiabatic states weighted by their state populations $|a_i|^2$. The method is also therefore referred to as mean-field approach. As a comparison, for BOMD/Ehrenfest dynamics:
$$hat{H}_{el} (mathbf{r}; mathbf{R}) Phi_k(mathbf{r}; mathbf{R}) = E^{el}_k(mathbf{R})Phi_k(mathbf{r}; mathbf{R})$$
$$M_Iddot{mathbf{R}}_I =-nabla_IE^{el}_k(mathbf{R})=-mathop{nabla_I}_{text{min }Phi_k}langlePhi_k|hat{H}_{el}|Phi_krangle$$
The electronic wavefunction $Phi_k(mathbf{r}; mathbf{R})$ is static (only implicit time-dependence) and the nuclear degrees of freedom are handled classically. The nuclear degrees of freedom are decoupled from electronic degrees of freedom, while for each MD step the electronic wavefunction has to be optimized for the ground state.
$$ihbarfrac{partial Phi(mathbf{r};mathbf{R},t)}{partial t}= hat{H}_{el} (mathbf{r}; mathbf{R}) Phi(mathbf{r};mathbf{R},t) $$
$$M_Iddot{mathbf{R}}_I =-nabla_Ilanglehat{H}_{el}(mathbf{r};mathbf{R})rangle$$
Here we have an explicit time dependence of the electronic wavefunction. Electronic and nuclear time evolutions are propagated with a three-time-step integrator. The electronic wavefunction is evolved via TD-SCF approach.
Answered by mykd on August 19, 2021
Car-Parrinello MD avoids repeatedly solving the electronic problem by propagating the orbitals as if they were particles governed by Newton's equations. This is much more efficient than having to solve at each time step as is done in Born-Oppenheimer MD, though at the cost of decreasing the maximum timestep for the dynamics (too large a step will lose the ground state), slightly reduced accuracy (not exactly at the ground state for each time step) and introducing a spurious "mass parameter" to describe the electronic motion.
To address these problems, Thomas Kuhne et al. developed the "Car-Parrinello like approach to BOMD", also referred to as second-generation CPMD. The key differences of this approach are:
There are some finer details to make this scheme work (specific parameterization of $mathbf{C}$, how $gamma$ is obtained) which are available in the original papers (both of which have arXiv preprint versions available).
Implementations:
References:
Answered by Tyberius on August 19, 2021
An approximation of BOMD (Born-Oppenheimer MD) where fictitious dynamics is used on the electrons to keep them close to their ground state, so that we do not have to keep solving for their ground state at every single step. We start with Newton's 2nd law (as does classical MD), but instead of the force being calculated by a full-fledged ab initio calculation at every step, the force itself has an EOM (equation of motion) which below is given by Eq. eqref{eq:fictitious}. For one nucleus with position $vec{r}$ and several electrons with orbitals ${psi_i}$ we get:
begin{align} tag{1} vec{F} &= mvec{ddot{r}} \ - nabla , Eleft[{ psi_i } , vec{r} right] &= mvec{ddot{r}}tag{2}\ mu ddot{psi}_i(vec{r},t) &= - frac{delta E}{delta psi_i^*(vec{r},t)} + sum_j Lambda_{ij} psi_j(vec{r},t),tag{3}label{eq:fictitious} end{align}
where $Lambda_{ij}$ is a matrix of Lagrange multipliers to allow satisfaction of the constraint that the wavefunctions $psi_i$ must be orthogonal; and $E[{psi_i},vec{r}]$ is an energy functional (usually a Kohn–Sham energy one). For several nucleii, just make a new subscript for $vec{r}$ and change the functional to $E[{psi_i},{vec{r_I}}]$, then the equations are exactly the same.
Implemented in:
Answered by Nike Dattani on August 19, 2021
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