CHAPTER 2: THEORETICAL AND COMPUTATIONAL BACKGROUND
2.4 Theory of Electronic Stopping
2.4.2 Simulating Electronic Stopping with RT-TDDFT
According the Runge-Gross theorem [70], it is possible for electron dynamics to be treated efficiently using time-dependent density functional theory (TDDFT) [7,23]. This
presents opportunities for studying the electronic stopping process without reliance on analytical models. For metals, the electronic stopping power is a linear function of ion velocity in the low velocity limit, and the slope is called the friction coefficient. Nazarov and co-workers demonstrated the calculation of the friction coefficients for a series of metals with various projectile ions using TDDFT and its current density functional theory variation [71,72]. Campillo and co-workers reported the stopping power calculation over a wide range of ion velocity using the LR-TDDFT [73].
In the last several years, scientists have started to explore the use of RT-TDDFT simulations to obtain electronic stopping power by directly simulating the electronic response to the projectile ion. This approach was found to be quite successful for obtaining the linear part of the electronic stopping power [74,75], and it also seemed promising for obtaining the electronic stopping power curve even for higher ion velocities [76,77] beyond the Bragg peak (peak in stopping power curve).
In order to simulate the non-equilibrium quantum dynamics of electrons in response to an energetic ion, we need to balance computational accuracy and efficiency. Although several methods and codes already exist for performing RT-TDDFT calculations (see Refs. [24,33,34,43,78-84]) this work requires a numerical implementation that scales efficiently on thousands of processors in massively parallel computers because large system sizes with thousands of electrons needs to be simulated for accurate modeling (as discussed in subsection 2.4.1). The computational approach we employ in this work is the direct calculation of the stopping power via its definition as the deposited energy as a function of the ion displacement x at a constant velocity v:
where E is the electronic energy in the system and the bracket indicates a classical ensemble average of ion trajectories at constant ion velocity [69,85]. For calculating this quantity, one performs a series of non-equilibrium electron dynamics simulation with different ion
velocities. The projectile ion is introduced in the simulation cell after the equilibrium electronic structure is obtained for the system using a standard DFT calculation. The RT- TDDFT simulation is then performed with the projectile ion moving at a constant velocity. By constraining the ion velocity, the total electronic energy increases, allowing for
calculation of the electronic stopping power for the given velocity.
Fig. 2.2. Electron density change in response to an energetic proton traveling with a velocity of 2.0 a.u. in a homogeneous electron gas. A steady state needs to be reached in the simulation before the energy derivative (stopping power) is obtained to calculate the electronic stopping power.
The non-equilibrium electronic response to the ion movement is obtained in the RT- TDDFT simulation only after the steady state is reached in the simulation, requiring a large simulation supercell. A case for the homogeneous electron gas is shown as an example in
Figure 2.2. The electronic energy derivative with respect to the ion displacement (Eq. 2.39) is then numerically calculated and the ensemble average is taken. In the electronic stopping simulation, only the projectile ion is moved and no other atoms are allowed to move, and thus no contributions from nuclear stopping (elastic collision) enter in the simulation although it would be negligible in any case at the velocities that we are interested in.
In a realistic system (unlike the homogeneous electron gas widely studied in the literature), atomic nuclei of the system complicate the numerical calculation of the electronic energy change (Eq. 2.39), especially because non-local pseudo-potentials are typically used for treating core electrons. The pseudo-potentials are given as the sums of local potentials and separable non-local operators
(2.40) where 𝜓˜™šV is an atomic pseudo-wavefunctions and 𝛿𝑉
˜ is an angular momentum-specific
potentials as defined in Kleinman-Bylander representation [40]. The construction of the pseudo-potentials needs to be performed more carefully than for standard DFT calculations, minimizing the cut-off radius as detailed in Ref. [69]. The pseudo-potentials are generated by inverting the atomic Kohn-Sham equation for a specific XC potential [86], with a rather small cut-off radius of ( typically ~1 a.u.). Most of the error resulting from the use of non- local pseudo-potentials can be removed by performing separate Born-Oppenheimer MD calculations on the same path [87], but a separate procedure of baseline fitting is generally required for calculating the energy derivative. Another approach that we found to remediate this problem is to calculate the electronic stopping power from the average nonadiabatic “drag” force (NA force) on the projectile rather than the total change in energy of the system.
r' ˆVext r =Vlocal(r)δ(r'−r)+ r'ψlm PS δVl δVlψlm PS r ψlm PS δVl ψlm PS l,m
∑
This approach is discussed in more detail in Chapter 4 and in Appendix B. Of course, there are many more physical and numerical complications in the simulation of electronic stopping and calculation of stopping power with RT-TDDFT, such as time step, plane-wave cutoff energy, etc. These issues are the primary subject of the work detailed in Chapter 4.
Although this work focuses on first-principles RT-TDDFT simulations as a means to go beyond analytical models, the computational cost of our approach is very high and it is desirable to advance analytical models using the first-principles simulations at the same time. First-principles simulations provide us with great details of the non-equilibrium electronic structure in electronic stopping processes, which allows us to systematically examine the validity of the plane-wave Born approximation in the analytical models (see, in particular, Chapters 3, 5, and 6). This key approximation results in a mathematically closed expression with a projectile charge that is independent of its velocity. Here, we have made progress in tackling this challenge by employing the first-principles quantum mechanical simulation to quantify the velocity-dependent effective charge. Such efforts will also help connect the wealth of existing understanding and recent increasingly popular efforts in simulating electronic stopping from first-principles quantum mechanical theory.
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