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Manual: Migrate howto:tddft from wiki (Orig. Author: Anna Hehn)
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maxdepth: 1
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---
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X-Ray <https://www.cp2k.org/howto:xas_tdp>
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Optical <https://www.cp2k.org/howto:tddft>
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tddft
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Infrared <https://brehm-research.de/spectroscopy>
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raman
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nmr
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512
docs/methods/properties/tddft.md
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docs/methods/properties/tddft.md
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# Optical Spectroscopy
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This is a short tutorial on how to run linear-response time-dependent density functional theory
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(LR-TDDFT) computations for absorption and emission spectroscopy. The TDDFT module enables a
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description of excitation energies and excited-state computations within the Tamm-Dancoff
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approximation (TDA) featuring GGA and hybrid functionals as well as semi-empirical simplified TDA
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kernels. The details of the implementation can be found in [Strand2019] and in [Hehn2022] for
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corresponding excited-state gradients. Note that the current module is based on an earlier TDDFT
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implementation [](#Iannuzzi2005). Please cite these papers if you were to use the TDDFT module for
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the computation of excitation energies ([Strand2019], [](#Iannuzzi2005)) or excited-state gradients
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([Hehn2022]).
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## Brief theory recap
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The implementation in CP2K is based on the Tamm-Dancoff approximation (TDA), which describes each
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excited state $p$ with the excitation energy $\Omega^p$ and the corresponding excited-state
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eigenvectors $\mathbf{X}^p$ as an Hermitian eigenvalue problem
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$$
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\mathbf{A} \mathbf{X}^p &= \Omega^p \mathbf{S} \mathbf{X}^p \, , \\
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\sum_{\kappa k} [ F_{\mu \kappa \sigma} \delta_{ik} - F_{ik \sigma} S_{\mu \kappa} ] X^p_{\kappa k \sigma} + \sum_{\lambda} K_{\mu \lambda \sigma} [\mathbf{D}^{{\rm{\tiny{X}}}p}] C_{\lambda i \sigma} &= \sum_{\kappa} \Omega^p S_{\mu \kappa} X^p_{\kappa i \sigma} \, .
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$$
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The Hermitian matrix $\mathbf{A}$ contains as zeroth-order contributions the difference in the
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Kohn-Sham (KS) orbital energies $\mathbf{F}$, and to first order kernel contributions $\mathbf{K}$
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which comprise --depending on the chosen density functional approximation -- Coulomb $\mathbf{J}$
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and exact exchange $\mathbf{K}^{\rm{\tiny{EX}}}$ contributions as well as contributions due to the
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exchange-correlation (XC) potential $\mathbf{V}^{\rm{\tiny{XC}}}$ and kernel
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$\mathbf{f}^{\rm{\tiny{XC}}}$,
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$$
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F_{\mu \nu \sigma} [\mathbf{D}] &= h_{\mu \nu} + J_{\mu \nu \sigma} [\mathbf{D}] - a_{\rm{\tiny{EX}}}K^{\rm{\tiny{EX}}}_{\mu \nu \sigma} [\mathbf{D}] + V_{\mu \nu \sigma}^{\rm{\tiny{XC}}} \, , \\
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K_{\mu \nu \sigma} [\mathbf{D}^{{\rm{\tiny{X}}}p}] &= J_{\mu \nu \sigma} [\mathbf{D}^{{\rm{\tiny{X}}}p}] - a_{\rm{\tiny{EX}}} K^{\rm{\tiny{EX}}}_{\mu \nu \sigma}[\mathbf{D}^{{\rm{\tiny{X}}}p}] + \sum_{\kappa \lambda \sigma'} f^{\rm{\tiny{XC}}}_{\mu \nu \sigma,\kappa \lambda \sigma'} D_{\kappa \lambda \sigma'}^{{\rm{\tiny{X}}}p} \, .
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$$
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$\mathbf{S}$ denotes the atomic-orbital overlap matrix, $\mathbf{C}$ the occupied ground-state KS
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orbitals and $\mathbf{D}$ and $\mathbf{D}^{\rm{\tiny{X}}}$ ground-state and response density
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matrices,
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$$
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D_{\mu \nu \sigma} &= \sum_k C_{\mu k \sigma} C_{\nu k \sigma}^{\rm{T}} \, , \\
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D_{\mu \nu \sigma}^{{\rm{\tiny{X}}}p} &= \frac{1}{2} \sum_{k} ( X^p_{\mu k \sigma} C_{\nu k \sigma}^{\rm{T}} + C_{\mu k \sigma} (X^p_{\nu k \sigma})^{\rm{T}} ) \, .
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$$
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Within the current implementation, symmetrization and orthogonalization of the response density
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matrix is ensured at each step of the Davidson algorithm. The current implementation features to
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approximate the exact exchange contribution of hybrid functionals using the auxiliary density matrix
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method (ADMM). Furthermore, the standard kernel can be approximated using the semi-empirical
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simplified Tamm-Dancoff approximation (sTDA), neglecting in this case XC contributions and
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approximating both Coulomb and exchange contributions $\mathbf{J}$ and $\mathbf{K}$ using
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semi-empirical operators $\boldsymbol{\gamma}^{\rm{\tiny{J}}}$ and
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$\boldsymbol{\gamma}^{\rm{\tiny{K}}}$ depending on the interatomic distance $R_{AB}$ of atoms $A$
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and $B$,
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$$
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\gamma^{\rm{\tiny{J}}}(A,B) &= \left ( \frac{1}{(R_{AB})^{\alpha} + \eta^{-\alpha}} \right)^{1/\alpha} \, , \\
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\gamma^{\rm{\tiny{K}}}(A,B) &= \left ( \frac{1}{(R_{AB})^{\beta} +( a_{\rm{\tiny{EX}}}\eta)^{- \beta} } \right )^{1/\beta} \, ,
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$$
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that depend on the chemical hardness $\eta$, the Fock-exchange mixing parameter $a_{\rm{\tiny{EX}}}$
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and powers of $\alpha$ and $\beta$ for either Coulomb and exchange interactions.
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Within the current implementation, oscillator strengths can be calculated for molecular systems in
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the length form and for periodic systems using the velocity form (see [Strand2019]).
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Based on the TDA eigenvalue problem, excited-state gradients can be formulated based on a
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variational Lagrangian for each excited state $p$,
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$$
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L [\mathbf{X}, \mathbf{C}, \Omega, \bar{\mathbf{W}}^{\rm{\tiny{X}}}, \bar{\mathbf{Z}}, \bar{\mathbf{W}}^{\rm{\tiny{C}}} ] &= \Omega - \sum_{\kappa \lambda k l \sigma} \Omega ( X_{\kappa k \sigma }^{\rm{T}} S_{\kappa \lambda } X_{\lambda l \sigma} - \delta_{kl} ) \\
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&- \sum_{kl \sigma} ( \bar{W}_{kl \sigma}^{\rm{\tiny{X}}} )^{\rm{T}} \sum_{\kappa \lambda} \frac{1}{2} ( C_{\kappa k \sigma}^{\rm{T}} S_{\kappa \lambda} X_{\lambda l \sigma} + X_{\kappa k \sigma}^{\rm{T}}S_{\kappa \lambda} C_{\lambda l \sigma}) \\
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&+ \sum_{\kappa k \sigma}( \bar{Z}_{\kappa k \sigma})^{\rm{T}} \sum_{\lambda} ( F_{\kappa \lambda \sigma}C_{\lambda k \sigma} - S_{\kappa \lambda } C_{\lambda k \sigma} \varepsilon_{k \sigma}) \\
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&- \sum_{kl\sigma} (\bar{W}^{\rm{\tiny{C}}}_{kl \sigma})^{\rm{T}} ( S_{kl \sigma} - \delta_{kl})\, .
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$$
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introducing Lagrange multipliers $\bar{\mathbf{W}}^{\rm{\tiny{X}}}$,
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$\bar{\mathbf{W}}^{\rm{\tiny{C}}}$, and $\bar{\mathbf{Z}}$ to ensure stationarity of the
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corresponding ground-state (GS) equations and to account for the geometric dependence of the
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Gaussian orbitals and thus requiring to solve the Z vector equation iteratively.
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## The LR-TDDFT input section
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To compute absorption spectra, parameters defining the LR-TDDFT computation have to be specified in
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the [TDDFPT](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT) subsection. Furthermore,
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[RUN_TYPE](#CP2K_INPUT.GLOBAL.RUN_TYPE) has to be set to `ENERGY` and the underlying KS ground-state
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reference has to be specified in the [DFT](#CP2K_INPUT.FORCE_EVAL.DFT) section.
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The most important keywords and subsections of [TDDFPT](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT)
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are:
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- [KERNEL](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.KERNEL): option for the kernel matrix
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$\mathbf{K}$ to choose between the full kernel for GGA or hybrid functionals and the simplified
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TDA kernel
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- [NSTATES](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.NSTATES): number of excitation energies to be
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computed
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- [CONVERGENCE](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.CONVERGENCE): threshold for the convergence
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of the Davidson algorithm
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- [RKS_TRIPLETS](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.RKS_TRIPLETS): option to switch from the
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default computation of singlet excitation energies to triplet excitation energies
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- [RESTART](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.RESTART): the keyword enables the restart of
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the TDDFPT computation if a corresponding restart file (.tdwfn) exists
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- [WFN_RESTART_FILE_NAME](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.WFN_RESTART_FILE_NAME): for a
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restart of the TDDFPT computation, the name of the restart file has to be specified using this
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keyword
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To compute excited-state gradients and thus corresponding fluorescence spectra, the excited state to
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be optimized furthermore has to be specified by adding the subsection `EXCITED_STATES` of the
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section `DFT`.
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## Simple examples
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### Excitation energies for acetone
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The following input is a standard input for calculating excitation energies with the hybrid
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functional PBE0. It should be noted that it is possible to compute the exact exchange integrals for
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hybrid functionals analytically at however high computational costs. It is therefore recommended to
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use the Auxiliary Density Matrix Method (ADMM) [](#Guidon2010) to approximate the exact exchange
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contribution. For GGAs, the corresponding ADMM sections are not required and it is sufficient to
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specify the chosen functional in the subsection `&XC_FUNCTIONAL` of the `&XC` section.
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```none
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&GLOBAL
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PROJECT S20Acetone
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RUN_TYPE ENERGY
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PREFERRED_DIAG_LIBRARY SL
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PRINT_LEVEL medium
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&END GLOBAL
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&FORCE_EVAL
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METHOD Quickstep
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&PROPERTIES
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&TDDFPT ! input section for TDDFPT
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KERNEL FULL ! specification of the underlying kernel matrix K
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! FULL kernel is for GGA and hybrid functional computations
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! sTDA kernel is referring to a semi-empirical sTDA computation
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NSTATES 10 ! specifies the number of excited states to be computed
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MAX_ITER 100 ! number of iterations for the Davidson algorithm
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CONVERGENCE [eV] 1.0e-7 ! convergence threshold in eV
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RKS_TRIPLETS F ! Keyword to choose between singlet and triplet excitations
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! &XC ! If choosing kernel FULL, the underlying functional can be
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! &XC_FUNCTIONAL PBE0 ! specified by adding an XC section
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! &END XC_FUNCTIONAL ! The functional can be chosen independently from the chosen
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! &END XC ! GS functional except when choosing ADMM
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! &MGRID ! It is also possible to choose a separate grid for the real-space
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! CUTOFF 800 ! integration of the response density in the TDDFT part,
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! REL_CUTOFF 80 ! however, in general a consistent setup for GS and ES is recommended
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! &END MGRID
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&END TDDFPT
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&END PROPERTIES
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&DFT
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&QS
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METHOD GPW
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EPS_DEFAULT 1.0E-17
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EPS_PGF_ORB 1.0E-20
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&END QS
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&SCF
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SCF_GUESS restart
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&OT
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PRECONDITIONER FULL_ALL
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MINIMIZER DIIS
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&END OT
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&OUTER_SCF
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MAX_SCF 900
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EPS_SCF 1.0E-7
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&END OUTER_SCF
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MAX_SCF 10
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EPS_SCF 1.0E-7
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&END SCF
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POTENTIAL_FILE_NAME POTENTIAL_UZH
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BASIS_SET_FILE_NAME BASIS_MOLOPT_UZH
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BASIS_SET_FILE_NAME BASIS_ADMM_UZH
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&MGRID
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CUTOFF 800
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REL_CUTOFF 80
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&END MGRID
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&AUXILIARY_DENSITY_MATRIX_METHOD ! For hybrid functionals, it is recommended to choose ADMM
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METHOD BASIS_PROJECTION ! the ADMM environment for ground and excited state has to be
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EXCH_SCALING_MODEL NONE ! identical
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EXCH_CORRECTION_FUNC NONE ! Triple-zeta auxiliary basis sets are recommended (see below)
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ADMM_PURIFICATION_METHOD NONE ! For periodic systems (see below), only specific ADMM options
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&END AUXILIARY_DENSITY_MATRIX_METHOD ! are available
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&POISSON
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PERIODIC NONE
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POISSON_SOLVER WAVELET
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&END
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&XC
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&XC_FUNCTIONAL PBE0
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&END XC_FUNCTIONAL
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&END XC
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&END DFT
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&SUBSYS
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&CELL
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ABC [angstrom] 14.0 14.0 14.0
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PERIODIC NONE
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&END CELL
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&COORD
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C 0.000000 1.282877 -0.611721
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C 0.000000 -1.282877 -0.611721
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C 0.000000 0.000000 0.185210
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O 0.000000 0.000000 1.392088
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H 0.000000 2.133711 0.059851
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H -0.876575 1.319344 -1.256757
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H 0.876575 1.319344 -1.256757
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H 0.000000 -2.133711 0.059851
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H 0.876575 -1.319344 -1.256757
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H -0.876575 -1.319344 -1.256757
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&END COORD
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&TOPOLOGY
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&CENTER_COORDINATES T
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&END
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&END
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&KIND H
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BASIS_SET ORB DZVP-MOLOPT-PBE0-GTH-q1 ! in general it is recommended to use larger basis sets
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BASIS_SET AUX_FIT admm-dzp-q1 ! for the primary and auxiliary basis (TZVP/tzp)
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POTENTIAL GTH-PBE0-q1
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&END KIND
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&KIND O
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BASIS_SET ORB DZVP-MOLOPT-PBE0-GTH-q6
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BASIS_SET AUX_FIT admm-dzp-q6
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POTENTIAL GTH-PBE0-q6
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&END KIND
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&KIND C
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BASIS_SET ORB DZVP-MOLOPT-PBE0-GTH-q4
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BASIS_SET AUX_FIT admm-dzp-q4
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POTENTIAL GTH-PBE0-q4
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&END KIND
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&END SUBSYS
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&END FORCE_EVAL
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```
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In the resulting output file, there is a `TDDFPT` section reporting the steps of the calculations.
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The initial guess is referring to the zeroth-order KS energy differences with the printout also
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listing the transition from the corresponding occupied to virtual orbital.
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```none
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-------------------------------------------------------------------------------
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- TDDFPT Initial Guess -
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-------------------------------------------------------------------------------
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State Occupied -> Virtual Excitation
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number orbital orbital energy (eV)
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-------------------------------------------------------------------------------
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1 12 13 6.63336
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2 11 13 9.62185
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3 10 13 10.34045
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4 9 13 10.78846
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5 8 13 11.05691
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6 12 14 12.07194
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7 7 13 12.42370
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8 6 13 12.63557
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9 12 15 12.65312
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10 5 13 12.68633
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```
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After convergence of the iterative Davidson algorithm, CP2K is printing for each of the calculated
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excited states the excitation energy in eV, the corresponding transition dipole as well as the
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oscillator strength. The form of the dipole transition integrals can be chosen by modifying the
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keyword [DIPOLE_FORM](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.DIPOLE_MOMENTS.DIPOLE_FORM). Possible
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options are `BERRY` (valid for fully periodic systems only), `LENGTH` (valid for molecular systems
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only) and `VELOCITY` (both). When referring to the length form, the reference point to calculate
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electric dipole moments can be chosen in the subsection by specifying the coordinates of the
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reference point
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[REFERENCE_POINT](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.DIPOLE_MOMENTS.REFERENCE_POINT) or by
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choosing one of the options `COM` (center of mass), `COAC` (center of atomic charges),
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`USER_DEFINED` (user-defined point) and `ZERO` (origin of the coordinate system) for the
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[REFERENCE](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.DIPOLE_MOMENTS.REFERENCE) keyword.
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```none
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-------------------------------------------------------------------------------
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- TDDFPT run converged in 10 iteration(s)
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-------------------------------------------------------------------------------
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R-TDDFPT states of multiplicity 1
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Transition dipoles calculated using velocity formulation
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State Excitation Transition dipole (a.u.) Oscillator
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number energy (eV) x y z strength (a.u.)
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------------------------------------------------------------------------
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TDDFPT| 1 4.67815 2.4840E-08 -1.9187E-08 5.9673E-08 5.21038E-16
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TDDFPT| 2 8.73074 -8.1610E-09 1.0502E-08 9.1823E-08 1.84132E-15
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TDDFPT| 3 9.17033 1.6661E-02 2.4911E-08 -9.2612E-08 6.23670E-05
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TDDFPT| 4 9.70094 -2.3716E-09 7.2323E-07 7.0660E-01 1.18663E-01
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TDDFPT| 5 9.88658 -3.1922E-08 -4.1476E-01 1.0768E-06 4.16669E-02
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TDDFPT| 6 10.78269 3.5483E-08 4.2695E-01 -1.3123E-07 4.81550E-02
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TDDFPT| 7 10.82893 2.3885E-01 -3.0329E-08 4.5882E-09 1.51356E-02
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TDDFPT| 8 10.92800 -2.4034E-07 -2.4299E-08 5.8160E-08 1.65293E-14
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TDDFPT| 9 11.32208 8.3808E-08 -6.8844E-01 1.9166E-07 1.31469E-01
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TDDFPT| 10 11.97282 1.2605E-08 1.7029E-08 3.3026E-01 3.19930E-02
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```
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A more detailed analysis of the excitations is given subsequently, listing orbital contributions for
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each transition with the corresponding excitation amplitudes. The keyword
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[MIN_AMPLITUDE](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.MIN_AMPLITUDE) regulates the threshold for
|
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the smallest amplitude to print.
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```none
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-------------------------------------------------------------------------------
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- Excitation analysis -
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-------------------------------------------------------------------------------
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State Occupied Virtual Excitation
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number orbital orbital amplitude
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-------------------------------------------------------------------------------
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1 4.67815 eV
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12 13 0.998438
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2 8.73074 eV
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10 13 0.995560
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6 13 0.087643
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3 9.17033 eV
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9 13 0.993356
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7 13 0.075589
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4 9.70094 eV
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11 13 -0.893130
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12 16 0.297568
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5 13 0.269023
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12 28 -0.108047
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9 15 0.066145
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9 30 -0.050159
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```
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### Excited-state gradient for acetone
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|
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To perform an excited-state optimization for emission spectroscopy, the run type has to be set to
|
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`GEO_OPT` and the state to be optimized has to be specified in the
|
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[EXCITED_STATES](#CP2K_INPUT.FORCE_EVAL.DFT.EXCITED_STATES) section. Note that the number of excited
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states chosen in the TDDFPT section should be larger or at least equal to the number of the chosen
|
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excited state.
|
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|
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```none
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&GLOBAL
|
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PROJECT S20Acetone
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RUN_TYPE ENERGY_FORCE ! The run type has to be changed to ENERGY_FORCE of GEO_OPT
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PREFERRED_DIAG_LIBRARY SL
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PRINT_LEVEL medium
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&END GLOBAL
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&PROPERTIES
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&TDDFPT
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NSTATES 10
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MAX_ITER 100
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CONVERGENCE [eV] 1.0e-7
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RKS_TRIPLETS F
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ADMM_KERNEL_CORRECTION_SYMMETRIC T ! required keyword when using hybrid functionals and ADMM for
|
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&END TDDFPT ! the exact exchange contribution for ES gradients
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&END PROPERTIES
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...
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&DFT
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&QS
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METHOD GPW
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EPS_DEFAULT 1.0E-17
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EPS_PGF_ORB 1.0E-20
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&END QS
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&EXCITED_STATES T
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STATE 1 ! the excited state to be optimized has to be specified in this section
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&END EXCITED_STATES
|
||||
&SCF
|
||||
SCF_GUESS restart
|
||||
&OT
|
||||
PRECONDITIONER FULL_ALL
|
||||
MINIMIZER DIIS
|
||||
&END OT
|
||||
&OUTER_SCF
|
||||
MAX_SCF 900
|
||||
EPS_SCF 1.0E-7
|
||||
&END OUTER_SCF
|
||||
MAX_SCF 10
|
||||
EPS_SCF 1.0E-7
|
||||
&END SCF
|
||||
...
|
||||
&END DFT
|
||||
```
|
||||
|
||||
The resulting output file contains for each step of the geometry optimization the already explained
|
||||
output of the TDDFPT computation and additionally information on the excited state that is optimized
|
||||
as well as the iterative solution of the Z vector equations.
|
||||
|
||||
```none
|
||||
!--------------------------- Excited State Energy ----------------------------!
|
||||
Excitation Energy [Hartree] 0.1719188002
|
||||
Total Energy [Hartree] -36.3332484083
|
||||
!-----------------------------------------------------------------------------!
|
||||
!--------------------------- Excited State Forces ----------------------------!
|
||||
|
||||
Iteration Method Restart Stepsize Convergence Time
|
||||
------------------------------------------------------------------------------
|
||||
1 PCG F 0.00E+00 0.0231470476 0.02
|
||||
2 PCG F 0.30E+00 0.0003972862 1.56
|
||||
3 PCG F 0.60E+00 0.0000361012 3.11
|
||||
4 PCG F 0.62E+00 0.0000031865 4.65
|
||||
5 PCG F 0.63E+00 0.0000002183 6.19
|
||||
6 PCG F 0.73E+00 0.0000000147 7.73
|
||||
7 PCG F 0.70E+00 0.0000000014 9.27
|
||||
8 PCG F 0.72E+00 0.0000000001 10.82
|
||||
9 PCG F 0.71E+00 0.0000000000 12.35
|
||||
!-----------------------------------------------------------------------------!
|
||||
|
||||
ENERGY| Total FORCE_EVAL ( QS ) energy [a.u.]: -36.333248408276823
|
||||
|
||||
-------------------------------------------------------------------------------
|
||||
```
|
||||
|
||||
### Choosing a semi-empirical kernel
|
||||
|
||||
To speed up computation times for broad-band absorption spectra, a semi-empirical simplified
|
||||
Tamm-Dancoff (sTDA) kernel can be chosen by setting
|
||||
[KERNEL](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.KERNEL) to `sTDA`. The semi-empirical electron
|
||||
repulsion operators depend on several empirical parameters, which need to be adjusted depending on
|
||||
the system under investigation. Most importantly, the amount of exact exchange, scaled by adjusting
|
||||
the parameter $a_{\rm{\tiny{EX}}}$ needs to be chosen carefully and is really crucial to ensure a
|
||||
well-balanced treatment of exact exchange in the GS and ES potential energy surfaces. Too large
|
||||
fractions of exchange in the excited state can lead to negative excitation energies. In general, a
|
||||
relatively small amount of exchange $a_{\rm{\tiny{EX}}}=0.2 / 0.1$ is therefore recommended.
|
||||
|
||||
For details on the STDA method see also <https://github.com/grimme-lab/stda>.
|
||||
|
||||
The most important keywords of the subsection [sTDA](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.STDA)
|
||||
are:
|
||||
|
||||
- [FRACTION](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.STDA.FRACTION): fraction of exact exchange
|
||||
$a_{\rm{\tiny{EX}}}$
|
||||
- [MATAGA_NISHIMOTO_CEXP](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.STDA.MATAGA_NISHIMOTO_CEXP):
|
||||
keyword to modify the parameter $\alpha$ of $\gamma^{\rm{\tiny{J}}}$
|
||||
- [MATAGA_NISHIMOTO_XEXP](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.STDA.MATAGA_NISHIMOTO_XEXP):
|
||||
keyword to modify the parameter $\beta$ of $\gamma^{\rm{\tiny{K}}}$
|
||||
- [DO_EWALD](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.STDA.DO_EWALD): keyword to switch on Ewald
|
||||
summation for the Coulomb contributions, required when treating periodic systems. (Exact exchange
|
||||
is treated within the minimum image convention and does not require any adjustment.)
|
||||
|
||||
```none
|
||||
&PROPERTIES
|
||||
&TDDFPT
|
||||
KERNEL sTDA ! switches on the semi-empirical kernel sTDA
|
||||
&sTDA
|
||||
FRACTION 0.2 ! it is crucial to adjust the fraction of exact exchange
|
||||
&END sTDA
|
||||
NSTATES 10
|
||||
MAX_ITER 100
|
||||
CONVERGENCE [eV] 1.0e-7
|
||||
RKS_TRIPLETS F
|
||||
&END TDDFPT
|
||||
&END PROPERTIES
|
||||
```
|
||||
|
||||
In the output, it can be checked that the sTDA kernel was switched on and the correct parameters for
|
||||
$\alpha$, $\beta$ and $a_{\rm{\tiny{EX}}}$ were chosen:
|
||||
|
||||
```none
|
||||
sTDA| HFX Fraction 0.2000
|
||||
sTDA| Mataga-Nishimoto exponent (C) 1.5160
|
||||
sTDA| Mataga-Nishimoto exponent (X) 0.5660
|
||||
sTDA| TD matrix filter 0.10000000E-09
|
||||
|
||||
-------------------------------------------------------------------------------
|
||||
- sTDA Kernel: Create Matrix SQRT(S) -
|
||||
-------------------------------------------------------------------------------
|
||||
```
|
||||
|
||||
The subsequent printout is then identical to the printout for GGA and hybrid functional kernels:
|
||||
|
||||
```none
|
||||
R-TDDFPT states of multiplicity 1
|
||||
Transition dipoles calculated using velocity formulation
|
||||
|
||||
State Excitation Transition dipole (a.u.) Oscillator
|
||||
number energy (eV) x y z strength (a.u.)
|
||||
------------------------------------------------------------------------
|
||||
TDDFPT| 1 4.88982 8.2927E-09 8.6085E-09 -2.2495E-08 7.77366E-17
|
||||
TDDFPT| 2 9.05888 4.5649E-09 -4.9483E-09 -8.2739E-08 1.52940E-15
|
||||
TDDFPT| 3 9.23700 1.4100E-02 -1.2802E-08 3.2962E-08 4.49914E-05
|
||||
TDDFPT| 4 9.52129 1.1297E-08 -4.7865E-08 8.3174E-01 1.61372E-01
|
||||
TDDFPT| 5 10.01790 -9.4987E-09 -4.8324E-01 -5.0387E-08 5.73140E-02
|
||||
TDDFPT| 6 10.86728 -1.6175E-08 -3.6799E-01 -7.5353E-09 3.60529E-02
|
||||
TDDFPT| 7 10.97656 -3.7898E-01 -1.0287E-08 -3.3941E-09 3.86231E-02
|
||||
TDDFPT| 8 11.21831 4.5569E-08 -4.2529E-09 1.9115E-08 6.76117E-16
|
||||
TDDFPT| 9 11.40817 2.7777E-08 -6.8033E-01 -3.7411E-08 1.29362E-01
|
||||
TDDFPT| 10 11.82525 -1.2576E-09 1.3562E-08 3.8592E-01 4.31486E-02
|
||||
```
|
||||
|
||||
It should be noted that it is possible to combine sTDA with the semi-empirical ground-state
|
||||
reference GFN1-xTB. However, it is then recommended to adjust all parameters [](#Grimme2016) and to
|
||||
apply corrections to shift the virtual KS orbital eigenvalues. A shift can be applied by adding the
|
||||
keyword [EV_SHIFT](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.EV_SHIFT) (for open-shell systems
|
||||
[EOS_SHIFT](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.EOS_SHIFT)).
|
||||
|
||||
### Periodic systems
|
||||
|
||||
Adjustments are required when switching to periodic boundary conditions. As already mentioned above,
|
||||
oscillator strengths should be calculated using the `BERRY` or `VELOCITY` formulation. When choosing
|
||||
the `sTDA` kernel, [DO_EWALD](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.STDA.DO_EWALD) has to be
|
||||
switched to true to activate Ewald summation for Coulomb contributions. When computing ES gradients
|
||||
using [KERNEL](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.KERNEL) `FULL` in combination with hybrid
|
||||
functionals and ADMM, only the ADMM2 method relying on basis projection is implemented in
|
||||
combination with the default for the exchange functional for the first-order GGA correction term.
|
||||
|
||||
```none
|
||||
&AUXILIARY_DENSITY_MATRIX_METHOD
|
||||
METHOD BASIS_PROJECTION
|
||||
ADMM_PURIFICATION_METHOD NONE
|
||||
EXCH_SCALING_MODEL NONE
|
||||
EXCH_CORRECTION_FUNC PBEX
|
||||
&END
|
||||
```
|
||||
|
||||
### Natural transition orbitals
|
||||
|
||||
Natural transition orbitals (NTOs) are printed when choosing `PRINT_LEVEL medium` in the `GLOBAL`
|
||||
section or when enabling the
|
||||
[NTO_ANALYSIS](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.PRINT.NTO_ANALYSIS) section. For this
|
||||
purpose it is required to generate unoccupied orbitals and the keyword
|
||||
[LUMO](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.NLUMO) enables to adjust the number of unoccupied
|
||||
orbitals. It is possible to print the NTOs as `CUBE_FILES` or in Molden format, with the latter
|
||||
being activated with the keyword
|
||||
[MOS_MOLDEN](#CP2K_INPUT.FORCE_EVAL.PROPERTIES.TDDFPT.PRINT.MOS_MOLDEN).
|
||||
|
||||
[hehn2022]: https://doi.org/10.1021/acs.jctc.2c00144
|
||||
[strand2019]: https://doi.org/10.1063/1.5078682
|
||||
Loading…
Add table
Add a link
Reference in a new issue