Abstract
The present chapter is dedicated to the numerical methods for solving the time-dependent Schrödinger equation for the nuclei.
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- 1.
A large part of this chapter is taken form the MCTDH lecture notes of H.-D. Meyer written by Daniel Pelaez-Ruiz. The authors sincerely thank Dr. Pelaez for letting them use his script.
- 2.
- 3.
For the primitive basis set of each coordinate, we use a DVR (see Sect. 8.1.3), more precisely HO DVR for \(R_1\) and a sine DVR for \(R_2\) with \(R_1\) \(\in \) [3.8, 5.6] a.u. and an unrestricted Legendre DVR for \(\theta \). Here, \(N_1\) = 36 for \(r_d\), \(N_2\) = 24 for \(r_v\), and \(N_3\) = 60 for \(\theta \).
- 4.
For the primitive basis set of each coordinate, we use a DVR (see Sect. 8.1.3), more precisely a sine DVR for \(R_1\) and \(R_2\) with \(R_1\) \(\in \) [0.6, 6.24] and 48 functions and \(R_2\) \(\in \) [1.0, 9.04] a.u. and 68 functions, and a Legendre DVR for \(\theta \) with 31 functions.
- 5.
A two-layers ML-MCTDH is identical to standard MCTDH
- 6.
Actually, we are considering the wavefunction of a particular total angular momentum J (that makes the dissociate coordinate R one-dimensional). Hence \(\Psi \) should be replaced with \(\Psi ^J\), but for the sake of simplicity we suppress the total angular momentum label J.
- 7.
The initial state is assumed to have no density beyond \(R_c\), i.e. \(\theta (R-R_c) |\Psi (R,{\varvec{q}},t=0)|^2 \equiv 0\).
- 8.
Actually \(P_{\gamma \nu }\) commutes with \(F_\gamma \). Thus \(P_{\gamma \nu }\, F_\gamma = F_\gamma \, P_{\gamma \nu } = P_{\gamma \nu }\, F_\gamma \, P_{\gamma \nu }\). The extra projector is added for symmetry reasons only.
- 9.
- 10.
Here the strength parameter \(\eta \) is included in the definition of W, in contrast to Sect. 8.5.
- 11.
Of course, mode combination can be used. Then \(h_r^{(\kappa )}\) operates on the \(\kappa \)-th particle in Eq. (8.333) and the integrals become low-dimensional rather than one-dimensional ones.
- 12.
Note that the root-mean-square error is given by \({\textit{rmse}}=\sqrt{ \Delta ^2/N_{\text {tot}}}\), where \(N_{\text {tot}}\) is the total number of grid points.
- 13.
Actually, we loop over the modes and update \(V^{\tiny {\text {ref}}}\) after each new SPP(k).
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Gatti, F., Lasorne, B., Meyer, HD., Nauts, A. (2017). Introduction to Numerical Methods. In: Applications of Quantum Dynamics in Chemistry. Lecture Notes in Chemistry, vol 98. Springer, Cham. https://doi.org/10.1007/978-3-319-53923-2_8
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