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2.3 Quantum Chemistry

2.3.1 Density Functional Theory

The density functional theory (DFT) is a remarkable theory that allows one to replace the complicated N-electron wave function by a much simpler electron density ρ(~r). The basis for DFT is the proof by Hohenberg and Kohn [81] that the ground-state electronic energy is determined completely by the electron density ρ(~r) [79, 80, 82, 83]. The Hohenberg-Kohn says that the molecular energy, the wave function and all other molecular properties can be computed from the ground state electron probability density. Even with the proof that every specific electron density gives a specific energy (for the ground state), the connection between the energy and the functional has not been discovered. The hypothetical functional can be divided into three parts: the kinetic energyT[ρ(~r)], the core-electron attractionEne[ρ(~r)], and the electron-electron repulsion Eee[ρ(~r)]. The electron-electron repulsion is usually divided into an exchange part K[ρ(~r)] and a Coulomb partJ[ρ(~r)]. The exact kinetic energy (T) for a

where Ψi are natural spin orbitals and ni their occupation number, 0 ≤ ni ≥ 1. For an interacting system, Eq. (2.55) contains an infinite number of terms, making an exact solution unattainable. Kohn and Sham [81] presented a formalism for treating the kinetic part of the energy.

In Hartree’s model [79, 80], the electrons move in an effective potentialυH(~r)created by the atomic cores and a mean field created by the other electrons is given as:

υH(~r) =−

wherearuns over all the nuclei,Za is the nuclear charge on atoma,R~a denotes the position of the nuclei andρ(~r)is the electron density.

In this approximation, a one-particle Schr¨odinger equation can be defined as:

−1

2∇2iH(~r)

Ψi=EiΨi (2.57)

whereEiis the energy of the system.

The mean density is given by

ρ(~r) =

N

X

i

i(~r)|2 (2.58)

For the ground state, a summation over the N spin orbitals with lowest eigenvalues is per-formed.

Eq. (2.56-2.58) are solved self-consistently. From a trial guess of the electron density, a potential is obtained by Eq. (2.56). This potential is used in Eq. (2.57). The one-electron orbitals obtained are put in to Eq. (2.58). The procedure is repeated until a set of converged one-electron orbitals are obtained. For a system of independent non-interacting electrons, the common one-body potential,υKS is assumed.

−1

2∇2iKS(~r)

Ψi=EiΨi (2.59)

The local one-body potential υKS gives, by definition, a non-interacting electron density that has the same form as Eq. (2.57).

On comparing Eq. (2.55) and Eq. (2.59), the expression for the kinetic energy of the non-interacting electrons (Ts[ρ]), becomes

Ts[ρ] =

N

X

i=1

i| −1

2∇2iii (2.60)

where the sumi again runs over all orbitals. The lower index s in Ts[ρ], denotes the single-electron equations. As the single-electrons do interact in reality, the expression is not exact, and the following inequality holds whereT[ρ]is the exact kinetic energy

Ts[ρ]≤T[ρ] (2.61)

The remaining part of the kinetic energy defines the correlation contribution:

Tc[ρ] =T[ρ]−Ts[ρ]≥0 (2.62)

where Tc is included in a exchange/correlation term Exc. The Kohn-Sham equations can be solved analogously to the Hartree equations, with the difference that the potential in Eq. (2.57),υH, is replaced by υef f:

υef f(~r) =υ(~r) +

Z ρ(~r0)

|~r−~r0 |d~r0xc(~r) (2.63)

where υxc(~r) denotes the local exchange/correlation potential and υ(~r) corresponds to the external potential.

Within the KS formalism, the energy of the ground state can be obtained from

EDF T[ρ] =X

i

Ei+Exc[ρ]− Z

υxc(~r)ρ(~r)dv−1 2

Z ρ(~r)ρ(~r0)

|~r−~r0 | (2.64)

or more generally, divided into its components:

EDF T[ρ(~r)] =Ts[ρ(~r)] +Ene[ρ(~r)] +J[ρ(~r)] +Exc[ρ(~r)] (2.65) An exact energy expression has been obtained from Eq. (2.65). The first term is the kinetic energy for the non-interacting electrons and the second term is the core-electron attraction and the third term represents the Coulombic repulsion functional, the electrostatic electron-electron repulsion and the final term is the exchange/correlation term. Except the last term exchange/correlation energy, all other terms are solved exactly. The new challenge was to find a solution toExc.

DIFFERENT DFTMODELS

Most DFT models differ in their expression for the exchange/correlation energy Exc. It is always split into separate exchange and correlation terms,ExandEc. The exchange energy is

“by definition” given as a sum of contributions fromαandβspin densities, as exchange energy only involves electrons of the same spin. The kinetic energy, the nuclear-electron attraction and Coulomb terms are trivially separable. The correlation energy contains contributions from the interactions between all electrons:

Ex(ρ) =Exαα) +Eβxβ) (2.66)

Ec(ρ) =Ecααα) +Ecβββ) +Ecαβα, ρβ) (2.67) Whereραandρβ are densities of theαandβspin. The total density is the sum of theαandβ contributions,ρ=ραβ the largest contribution toExccomes from the exchange partEx.

THE LOCAL DENSITY APPROXIMATION

In theLocal Density Approximation(LDA) it is assumed that the density can be treated locally as a uniform electron gas or the electron density is assumed to be slowly varying in space

ExcLDA[ρ] = Z

ρ(~r)εunifxc (ρ) (2.68)

εunifxc gives the exchange/correlation energy per electron in a uniform electron gas. The ana-lytical expression for the exchange energy can be obtained from the Dirac formula

ExcLDA[ρ] =−Cx

Z

ρ4/3(~r)d~r (2.69)

whereCx is given as:

Cx=3 4

3 π

1/3

In the more general case, whereα andβ densities are not equal, LDA has been replaced by theLocal Spin Density Approximation(LSDA).

ExcLSDA[ρ] =−21/3Cx

Z

ρ4/3α (~r) +ρ4/3β (~r)

d~r (2.70)

For the LDA correlation energy, no exact solution is known but it has been determined by Monte Carlo methods for a number of different densities. In order to use these results in DFT calculations, a suitable analytic interpolation formula is desirable. Vosko, Wilk and Nusari [84] fitted various data to obtain reliable analytic expressions for the LDA correlation energy and in general considered to be a very accurate fit. This exchange functional is used in the calculations.

THE GENERALIZED GRADIENT APPROXIMATION

The Generalized Gradient Approximation (GGA) [79, 80] is the improvement over the LSAD approach where the electron distribution is considered as a non-uniform electron gas. The idea behind this is not only considering the electron density, but also the gradient of the density, that is the change in the density at a given point.

The term GGA was probably first introduced in connection with the PW86 functional, devel-oped by Perdew and Wang in 1986 [85]. Perdew and Wang proposed modifying the LSDA exchange expression to that shown in Eq. (2.71)

ExP W86LDAx (1 +ax2+bx4+cx6)1/15 (2.71)

x= | ∇ρ|

ρ4/3 (2.72)

wherexis a dimensionless gradient variable, anda,bandcbeing suitable constant where the summation over equivalent expression forαandβ densities is implicitly assumed.

A general GGA functional has the form:

εGGAGGAα, ρβ,∇ρα,∇ρβ) (2.73)

Several GGA functionals, for both exchange and correlation, have been proposed in the liter-ature [85–90].

Becke [87] proposed a widely used correlation (B or B88) to the LSDA exchange energy:

εB88xLDAx + ∆εB88x (2.74)

∆εB88x =−βρ1/3 x2

1 + 6βxsinh−1x (2.75)

Theβ parameter is determined by fitting to known atomic data andxis defined in Eq. (2.72).

Perdew and Wang have proposed an exchange functional similar to B88 to be used in connec-tion with the PW91 correlaconnec-tion funcconnec-tional given below.

εP Wx 91LDAx 1 +xa1sinh−1(xa2) + (a3+a4e−bx2)x2 1 +xa1sinh−1(xa2) +a5x2

!

(2.76)

where ai and b are suitable constants and x is defined in Eq. (2.72). where x is given in Eq. (2.72) This GGA functional is used for the calculations.

HYBRID METHODS

The Kohn-Sham extensions revealed that improved expressions for electron exchange and correlation can lead to better wave functions and electronic energy. Therefore major attempts were carried out in the past to find improved and better electron exchange and correlation expressions.

Wave function theory (Hartree-Fock) can in principle provide the exact exchange energy.

ExHF =−1 2

n

X

i n

X

j

Z Z Ψi(~r1j(~r1i(~r2j(~r2)

|~r1−~r2| d~r1~r2 (2.77) It could be assumed that the ideal exchange/correlation energy would then be obtained from

Exc=ExHF +EcDF T (2.78)

In hybrid DFT methods in general, the exchange term of DFT is corrected by a contribu-tion from exact exchange energy. In the above, the DFT exchange has been replaced by HF exchange.

BECKE3 The most popular hybrid methods are based on Becke’s three functional B3[91]. It contains three adjustable parametersa0,ax andac:

ExcB3=a0ExHF + (1−a0)ExLSDA+ax∆ExB88+EcLSDA+ac∆EGGAc (2.79) Becke used PW91 for the correlation part [86, 88, 92]. The name of the functional , B3PW91, implies its use of a three-parameter scheme, as well as GGA exchange and correlation func-tionals B and PW91, respectively.

ExcB3LY P =a0ExHF + (1−a0)ExLSDA+ax∆ExB88+EcLSDA+ac∆EP Wc 91 (2.80)

THE BECKE 3 LEE, YANG AND PARR (B3LYP) HYBRID-FUNCTIONAL This is most frequently used in the quantum chemical computations. The DFT functional B3LYP comprises three different units: B stands exchange functional developed by A. Becke. The ‘3’ stands for the three adjustable parameters (see Eq. (2.79)), Stephens et al.,[93] modified LYP [90] correlation which was developed by Lee, Yang and Parr. Because LYP is designed to compute the full correlation energy and not a correction to LSDA. The B3LYP model is defined by

ExcB3=a0ExHF + (1−a0)ExLSDA+ax∆ExB+ (1−ac)EcLSDA+acELY Pc (2.81) Of all modern functionals, B3LYP has proved to be most popular to date. The B3LYP methods are used for the geometry optimization and solvation energy calculations.