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Next: Conclusions Up: Empirical Density Functionals.2 Previous: General Theory

Results

The BLYP functional is known to perform quite well on the G2 set [98,100,106], making it an ideal starting point for the optimizations. The results of modifying the BLYP parameters are listed in Table 4.1.


  
Table 4.1: Modified BLYP RMS deviations (kcal/mol)
Functional RMS deviation
B(0.0042)-LYP 5.290
B(0.0035)-LYP 5.069
B(0.0042) + 1.0431LYP 4.963
B-LYP(optimum) 4.848

The unmodified BLYP functional (with Becke's $\beta$ parameter of 0.0042 in the exchange part) gives an RMS error of 5.290 kcal/mol. The corresponding mean absolute deviation is 4.11 kcal/mol. Next, the Becke $\beta$ parameter was optimized, moving to 0.0035, giving an RMS deviation of 5.069 kcal/mol. Third, an optimal linear combination of the original Becke and LYP parts is found, lowering the RMS deviation to 4.963 kcal/mol. A final, fuller optimization only lowers the RMS error to 4.848 kcal/mol. (This has a Dirac coefficient of 1.0072 times the original, a $\beta$ value of 0.003705 and LYP parameters of a,b,c,d = 0.049,0.108,0.24,0.342.)

The next step is to see the effect of the different $\beta$ values through external mixing. By taking a combination of B(0.0035)-LYP, B(0.0042)-LYP, Hartree-Fock-Slater and Hartree-Fock-Becke theories the RMS deviation is lowered to 4.543 kcal/mol. Clearly the linear combination of two Becke functionals is a better exchange functional than either separately. The external optimization coefficients are
\begin{align}9.558\mathrm{B(0.0035)LYP} - 7.727\mathrm{B(0.0042)LYP} - 0.861\mathrm{HFS} + 0.743\mathrm{HFB(0.0042)}.
\end{align}
These coefficients were then refined via an internal optimization, along with a redetermination of the LYP parameters. The complete functional is then
\begin{align}\begin{split}
E_{xc} &= 1.030952 E_{x}^{D30} + 10.4017 \Delta E_{x}...
....0042) \\
& \quad + E_{c}^{LYP}(0.055,0.158,0.25,0.3505)
\end{split}\end{align}
where $\Delta E_{x}^{B88}$ represents the Becke correction, that is the B88 functional without the Dirac term. With this functional the RMS deviation is lowered to 4.237 kcal/mol and the mean absolute deviation is 3.215 kcal/mol. The non-LYP part of the above functional has been termed the double-Becke functional, while the complete functional is called `Empirical Density Functional 1' or EDF1.


  
Table 4.2: External linear mixing of Hartree-Fock (kcal/mol)
Functional Combination RMS deviation
BLYP + HFB(0.0042) + HFS 4.920
BLYP + HFB(0.0042) + HFS + HF 4.499
EDF1 + HFB(0.0042) + HFB(0.0035) + HFS + BLYP 4.211
EDF1 + HFB(0.0042) + HFB(0.0035) + HFS + BLYP + HF 4.211

The third step is to investigate the effect of adding a fraction of Fock exchange to EDF1. Table 4.2 gives the results of external mixing of Hartree-Fock with BLYP and EDF1 plus their components. Clearly, there is strong HF mixing with BLYP, but virtually none with EDF1. This is confirmed by trying to mix in HF with an internal optimization of the EDF1 components and Fock exchange. The HF coefficient is less than 0.001 and there is no significant lowering of the RMS error.

To asses the usefulness of EDF1 as a density functional it has been used to obtain the thermochemistry of the molecules in the G2 set, using the 6-31G* basis. The results are listed in Table 4.3 and Table 4.4. In addition, the BLYP and B3LYP functionals have been included for comparison. Perhaps surprisingly, B3LYP performs quite poorly, being inferior to both BLYP and EDF1. However, the parametization of the B3LYP functional was carried out using what is, in effect, an infinite basis. It is therefore not unreasonable to expect performance to improve if it was reoptimized for the 6-31G* basis. An internal reoptimization along these lines shows a decrease in the Fock exchange coefficient to about 5%, with an RMS error of 4.65 kcal/mol, still considerably inferior to EDF1.


  
Table 4.3: Deviations from experiment for various functionals
  Exp. Exp.-BLYP Exp.-B3LYP Exp.-EDF1
atomization energies (kcal/mol)
H2 103.3 -0.1 -0.6 -3.1
LiH 56.0 1.0 1.0 1.3
BeH 46.9 -7.0 -7.9 -7.2
CH 79.9 -0.3 0.3 -0.4
CH2 (3B1) 179.6 1.9 0.1 -2.3
CH2 (1A1) 170.6 4.0 3.8 2.2
CH3 289.2 1.5 -0.8 -3.7
CH4 392.5 3.9 0.6 -3.7
NH 79.0 -3.5 -1.6 -2.7
NH2 170.0 -2.6 -0.2 -2.6
NH3 276.7 2.6 4.4 -0.2
OH 101.3 0.7 2.8 0.4
OH2 219.3 7.6 10.3 4.6
FH 135.2 5.3 7.7 2.9
SiH2(1A1) 144.4 1.5 0.2 -0.6
SiH2(3B1) 144.4 1.5 0.2 -0.6
SiH3 214.0 4.4 1.0 -0.3
SiH4 302.8 6.0 1.0 0.7
PH2 144.7 -0.7 -1.0 -2.8
PH3 227.4 4.4 3.0 0.4
SH2 173.2 7.5 7.1 3.4
ClH 102.2 6.5 6.4 3.5
Li2 24.0 4.2 4.2 5.4
LiF 137.6 2.3 5.8 4.4
HCCH 388.9 8.4 11.3 4.1
H2CCH2 531.9 7.0 5.6 -1.3
H3CCH3 666.3 9.5 3.7 -3.0
CN 176.6 -3.7 7.8 -2.1
HCN 301.8 -2.1 6.6 -1.5


Table 4.3 (continued)
  Exp. Exp.-BLYP Exp.-B3LYP Exp.-EDF1
CO 256.2 2.5 10.5 2.4
HCO 270.3 -4.4 3.6 -6.3
H2CO 357.2 -1.0 4.9 -4.5
H3COH 480.8 6.9 7.8 -0.1
N2 225.1 -4.5 8.8 0.2
H2NNH2 405.4 -0.1 5.2 -2.4
NO 150.1 -8.5 3.6 -6.7
O2 118.0 -13.1 1.3 -13.9
HOOH 252.3 0.5 11.3 -0.2
F2 36.9 -9.1 3.8 -7.3
CO2 381.9 -2.8 11.9 -5.4
Na2 16.6 -0.7 -0.1 1.3
Si2 74.0 1.9 9.0 0.8
P2 116.1 2.5 10.4 3.7
S2 100.7 1.8 7.4 0.0
Cl2 57.2 7.7 10.9 6.6
NaCl 97.5 7.4 6.7 6.7
SiO 190.5 3.6 12.7 6.2
SC 169.5 3.6 10.8 2.6
SO 123.5 -1.1 9.0 -1.4
ClO 63.3 -3.5 5.8 -2.9
ClF 60.3 -0.9 6.1 -0.7
CH3Cl 371.0 7.1 5.1 -0.2
Si2H6 500.1 13.2 4.5 4.1
CH3SH 445.1 11.1 8.4 2.1
HOCl 156.3 4.1 10.8 3.0
SO2 254.0 16.3 35.9 15.3
ionization potentials (V)
H 13.60 0.12 0.08 0.06
He 24.59 -0.12 -0.19 -0.20


Table 4.3 (continued)
  Exp. Exp.-BLYP Exp.-B3LYP Exp.-EDF1
Li 5.39 -0.13 -0.15 -0.12
Be 9.32 0.33 0.29 0.36
B 8.30 -0.27 -0.30 -0.26
C 11.26 -0.13 -0.19 -0.18
N 14.54 -0.01 -0.09 -0.13
O 13.61 -0.54 -0.43 -0.31
F 17.42 -0.33 -0.26 -0.24
Ne 21.56 -0.22 -0.17 -0.28
Na 5.14 -0.19 -0.19 -0.07
Mg 7.65 0.02 0.00 0.14
Al 5.98 0.11 0.04 0.04
Si 8.15 0.20 0.11 0.12
P 10.49 0.29 0.17 0.16
S 10.36 -0.01 -0.05 0.01
Cl 12.97 0.07 0.00 0.04
Ar 15.76 0.11 0.01 0.00
CH4 12.62 0.13 0.00 0.07
NH3 10.18 0.19 0.20 0.13
OH 13.01 -0.11 -0.06 -0.04
OH2 12.62 0.17 0.19 0.11
FH 16.04 0.08 0.11 0.00
SiH4 11.00 0.21 0.02 0.18
PH 10.15 0.15 0.04 0.03
PH2 9.82 0.05 -0.05 -0.05
PH3 9.87 0.18 0.14 0.17
SH 10.37 0.09 0.03 0.08
SH2 10.47 0.24 0.16 0.18
ClH 12.75 0.19 0.10 0.10
HCCH 11.40 0.40 0.36 0.32
H2CCH2 10.51 0.35 0.35 0.28


Table 4.3 (continued)
  Exp. Exp.-BLYP Exp.-B3LYP Exp.-EDF1
CO 14.01 0.01 -0.12 0.07
N2 15.58 0.24 -0.15 0.21
O2 12.07 -0.47 -0.79 -0.53
P2 10.53 0.32 -0.36 0.20
S2 9.36 -0.02 -0.26 -0.13
Cl2 11.50 0.30 0.04 0.23
ClF 12.66 0.19 -0.02 0.16
SC 11.33 -0.06 -0.14 -0.05
electron affinities (eV)
C 1.26 -0.07 -0.02 -0.06
CH 1.24 -0.07 -0.02 -0.07
CH2 0.65 -0.07 0.05 0.05
CH3 0.08 0.14 0.24 0.21
CN 3.82 -0.06 -0.18 0.02
NH 0.38 -0.07 0.09 0.07
NH2 0.74 0.08 0.21 0.15
NO 0.02 -0.37 -0.36 -0.30
O 1.46 -0.26 -0.06 -0.11
OH 1.83 0.02 0.19 0.08
O2 0.44 -0.14 -0.11 0.07
F 3.40 -0.22 -0.02 -0.17
Si 1.38 0.19 0.13 0.18
SiH 1.28 0.14 0.09 0.13
SiH2 1.12 0.08 0.04 0.08
SiH3 1.44 0.11 0.11 0.17
P 0.75 -0.10 -0.07 -0.02
PH 1.00 0.01 0.02 0.08
PH2 1.26 0.12 0.11 0.16
PO 1.09 -0.05 -0.17 -0.06
S 2.08 -0.04 -0.03 0.02


Table 4.3 (continued)
  Exp. Exp.-BLYP Exp.-B3LYP Exp.-EDF1
SH 2.31 0.07 0.07 0.09
S2 1.66 0.07 -0.03 0.12
Cl 3.62 0.01 -0.01 0.00
Cl2 2.39 -0.69 -0.70 -0.56
proton affinities (kcal/mol)
H2 100.8 10.7 11.5 8.5
HCHH 152.3 0.5 -0.2 -2.5
NH3 202.5 1.1 -0.2 -1.7
H2O 165.1 5.3 4.1 2.9
SiH4 154.0 4.0 5.7 2.9
PH3 187.1 4.0 2.8 1.5
H2S 168.8 3.4 3.5 1.0
HCl 133.6 5.6 6.5 3.4


  
Table 4.4: RMS errors for functionals
RMS Errors (kcal/mol) Exp.-BLYP Exp.-B3LYP Exp.-EDF1
atomization energies 5.75 8.10 4.41
ionization potentials 5.14 5.05 4.34
electron affinities 4.39 4.40 3.79
proton affinities 5.23 5.51 3.77

The overall improvement in moving from B3LYP (or BLYP) to EDF1 is largely due to the better atomization energies and proton affinities. The electron addition and removal energies are only slightly superior. It is interesting that the worst EDF1 results (atomization energies of SO2 and O2, ionization energy of O2, electron affinity of Cl2, and proton affinity of H2) are also problematic cases for BLYP and B3LYP. This confirms the underlying similarity of each of the three functionals, that they are all made from essentially the same main components.

By writing density functionals in the form
\begin{align}E_{xc}[\rho] = \int \rho^{4/3}({\bf r}) g(x) \, d{\bf r}
\end{align}
the double-Becke functional can be compared with the original B88 form. The B88 g(x) is
\begin{align}g_{B88}(\beta,x) = C_{0} - \frac{\beta x^{2}}{1+6\beta x \sinh^{-1}(x)}
\end{align}
with $\beta = 0.0042$ and C0 is the coefficient of the Dirac functional. The new g(x) is
\begin{align}g_{doubleB}(x) = -0.922818 C_{0} + 10.4017 g_{B88}(0.0035,x) - 8.44793 g_{B88}(0.0042,x)
\end{align}
These two functions are plotted in Figure 4.1.


  
Figure 4.1: The g(x) functions for the B88 and double-Becke exchange functionals
xx LegA gB88(x) LegB gdoubleB(x) \includegraphics[scale=0.95]{edfplot1.epsf}

At x=0 the double-Becke value is slightly below that of the uniform electron gas. The double-Becke curve is also much flatter at the origin. This can be seen from the initial term in the Taylor expansion
\begin{align}g(x) = g(0) + \frac{1}{2}g''(0)x^{2}+ \ldots
\end{align}
which is g''(0) = -0.00184, compared with -0.0084 from the original B88 form. The double-Becke value is much closer to the Sham-Kleinman value of -0.00387 . Also, the double-Becke curve is below B88 until x=4 and the curves cross again at x=9.7 .


next up previous contents
Next: Conclusions Up: Empirical Density Functionals.2 Previous: General Theory
Ross D. Adamson
1999-01-27