# Correlation energies from TDDFT¶

The Random Phase Approximation (RPA) for correlation energies comprises a nice non-empirical expression for the correlation energy that can be naturally combined with exact exchange to calculate binding energies. Due to the non-local nature of the approximation, RPA gives a good account of dispersive forces and is the only xc approximation capable of describing intricate binding regimes where covalent and van der Waals interactions are equally important. However, RPA does not provide a very accurate description of strong covalent bonds and typically performs worse than standard GGA functionals for molecular atomization energies and cohesive energies of solids.

In general, the exact correlation energy can be expressed in terms of the exact response function as

and the RPA approximation for correlation energies is simply obtained from the RPA approximation for the response function. From the point of view of TDDFT, the response function can be expressed exactly in terms of the Kohn-Sham response function and the exchange-correlation kernel \(f_{xc}\):

The RPA is obtained by neglecting the exchange-correlation kernel and it should be possible to improve RPA by including simple approximations for this kernel. However, if one tries to use a simple adiabatic kernel, one encounters severe convergence problems and results become worse than RPA! The reason for this is that the locality of adiabatic kernels renders the pair-correlation function divergent. As it turns out, the adiabatic correlation hole can be renormalized by a simple non-empirical procedure, which results in a density-dependent non-locality in the kernel. This can be done for any adiabatic kernel and the method has implemented for LDA and PBE. We refer to these approximations as renormalized adiabatic LDA (rALDA) and renormalized adiabatic PBE (rAPBE). We only include the exchange part of the kernel, since this part is linear in \(\lambda\) and the kernel thus only needs to be evaluated for \(\lambda=1\).

For more details on the theory and implementation of RPA we refer to RPA correlation energy and the tutorial Calculating RPA correlation energies. The RPA tutorial should be studied before the present tutorial, which inherits much of the terminology from RPA. Details on the theory, implementation and benchmarking of the renormalized kernels can be found in Refs. 1, 2, and 3.

Below we give examples on how to calculate the correlation energy of a Hydrogen atom as well as the rAPBE atomization energy of a \(CO\) molecule and the rAPBE cohesive energy of diamond. Note that some of the calculations in this tutorial will need a lot of CPU time and are essentially not possible without a supercomputer.

Finally, we note that there is some freedom in deciding how to include the density dependence in the kernel. By default the kernel is constructed from a two-point average of the density. However as shown in Example 4 it is possible to instead use a reciprocal-space averaging procedure. Within this averaging scheme it is possible to explore different approximations for \(f_{xc}\), for instance a simple dynamical kernel, or a jellium-with-gap model, which displays a \(1/q^2\) divergence for small \(q\). More details can be found below and in 4.

## Example 1: Correlation energy of the Hydrogen atom¶

As a first demonstration of the deficiencies of RPA, we calculate the correlation energy of a Hydrogen atom. The exact correlation energy should vanish for any one-electron system. The calculations can be performed with the following scripts, starting with a standard DFT-LDA calculation:

```
from ase import Atoms
from ase.parallel import paropen
from gpaw import GPAW
from gpaw import PW
resultfile = paropen('H.ralda.DFT_corr_energies.txt', 'w')
resultfile.write('DFT Correlation energies for H atom\n')
H = Atoms('H', [(0, 0, 0)])
H.set_pbc(True)
H.center(vacuum=2.0)
calc = GPAW(mode=PW(300, force_complex_dtype=True),
parallel={'domain': 1},
hund=True,
txt='H.ralda_01_lda.output.txt',
xc='LDA')
H.calc = calc
E_lda = H.get_potential_energy()
E_c_lda = -calc.get_xc_difference('LDA_X')
resultfile.write(f'LDA correlation: {E_c_lda} eV')
resultfile.write('\n')
calc.diagonalize_full_hamiltonian()
calc.write('H.ralda.lda_wfcs.gpw', mode='all')
```

followed by an RPA calculation:

```
from gpaw.xc.rpa import RPACorrelation
rpa = RPACorrelation('H.ralda.lda_wfcs.gpw',
txt='H.ralda_02_rpa_at_lda.output.txt')
rpa.calculate(ecut=300)
```

and finally one using the rALDA kernel:

```
from gpaw.xc.fxc import FXCCorrelation
fxc = FXCCorrelation('H.ralda.lda_wfcs.gpw',
xc='rALDA', txt='H.ralda_03_ralda.output.txt')
fxc.calculate(ecut=300)
```

The analogous set of scripts for PBE/rAPBE are `H.ralda_04_pbe.py`

, `H.ralda_05_rpa_at_pbe.py`

and `H.ralda_06_rapbe.py`

.
The computationally heavy RPA/rALDA/rAPBE parts can be parallelized efficiently on multiple CPUs.
After running the scripts the LDA and PBE correlation energies may be found in the file `H.ralda.DFT_corr_energies.txt`

.
Note that a rather small unit cell is used and the results may not be completely converged with respect
to cutoff and unit cell. Also note that the correlation energy is calculated at different cutoff energies up to
300 eV and the values based on two-point extrapolation is printed at the end (see Calculating RPA correlation energies and RPA correlation energy for a
discussion on extrapolation). The results in eV are summarized below.

LDA |
RPA |
rALDA |
---|---|---|

-0.56 |
-0.55 |
-0.029 |

PBE |
RPA |
rAPBE |
---|---|---|

-0.16 |
-0.55 |
-0.007 |

The fact that RPA gives such a dramatic underestimation of the correlation energy is a general problem with the method, which is also seen for bulk systems. For example, for the homogeneous electron gas RPA underestimates the correlation energy by ~0.5 eV per electron for a wide range of densities.

## Example 2: Atomization energy of CO¶

Although RPA severely underestimates absolute correlation energies in general, energy differences are often of decent quality due to extended error cancellation. Nevertheless, RPA tends to underbind and performs slightly worse than PBE for atomization energies of molecules. The following example shows that rAPBE not only corrects the absolute correlation energies, but also performs better than RPA for atomization energies.

First we set up a ground state calculation with lots of unoccupied bands. This is done with the script:

```
from ase import Atoms
from ase.parallel import paropen
from gpaw import GPAW, FermiDirac
from gpaw.mixer import MixerSum
from gpaw.hybrids.energy import non_self_consistent_energy as nsc_energy
from gpaw import PW
# CO
CO = Atoms('CO', [(0, 0, 0), (0, 0, 1.1283)])
CO.set_pbc(True)
CO.center(vacuum=3.0)
calc = GPAW(mode=PW(600, force_complex_dtype=True),
parallel={'domain': 1},
xc='PBE',
txt='CO.ralda_01_CO_pbe.txt',
convergence={'density': 1.e-6})
CO.calc = calc
E0_pbe = CO.get_potential_energy()
E0_hf = nsc_energy(calc, 'EXX')
calc.diagonalize_full_hamiltonian()
calc.write('CO.ralda.pbe_wfcs_CO.gpw', mode='all')
# C
C = Atoms('C')
C.set_pbc(True)
C.set_cell(CO.cell)
C.center()
calc = GPAW(mode=PW(600, force_complex_dtype=True),
parallel={'domain': 1},
xc='PBE',
mixer=MixerSum(beta=0.1, nmaxold=5, weight=50.0),
hund=True,
occupations=FermiDirac(0.01, fixmagmom=True),
txt='CO.ralda_01_C_pbe.txt',
convergence={'density': 1.e-6})
C.calc = calc
E1_pbe = C.get_potential_energy()
E1_hf = nsc_energy(calc, 'EXX')
f = paropen('CO.ralda.PBE_HF_C.dat', 'w')
print(E1_pbe, E1_hf, file=f)
f.close()
calc.diagonalize_full_hamiltonian()
calc.write('CO.ralda.pbe_wfcs_C.gpw', mode='all')
# O
O = Atoms('O')
O.set_pbc(True)
O.set_cell(CO.cell)
O.center()
calc = GPAW(mode=PW(600, force_complex_dtype=True),
parallel={'domain': 1},
xc='PBE',
mixer=MixerSum(beta=0.1, nmaxold=5, weight=50.0),
hund=True,
txt='CO.ralda_01_O_pbe.txt',
convergence={'density': 1.e-6})
O.calc = calc
E2_pbe = O.get_potential_energy()
E2_hf = nsc_energy(calc, 'EXX')
calc.diagonalize_full_hamiltonian()
calc.write('CO.ralda.pbe_wfcs_O.gpw', mode='all')
f = paropen('CO.ralda.PBE_HF_CO.dat', 'w')
print('PBE: ', E0_pbe - E1_pbe - E2_pbe, file=f)
print('HF: ', E0_hf - E1_hf - E2_hf, file=f)
f.close()
```

which takes on the order of 6-7 CPU hours. The script generates three gpw files containing the wavefunctions,
which are the input to the rAPBE calculation. The PBE and non-selfconsistent Hartree-Fock atomization energies
are also calculated and written to the file `CO.ralda.PBE_HF_CO.dat`

.
Next we calculate the RPA and rAPBE energies for CO with the script

```
from ase.parallel import paropen
from ase.units import Hartree
from gpaw.xc.rpa import RPACorrelation
from gpaw.xc.fxc import FXCCorrelation
from gpaw.mpi import world
fxc0 = FXCCorrelation('CO.ralda.pbe_wfcs_CO.gpw',
xc='rAPBE',
txt='CO.ralda_02_CO_rapbe.txt',
wcomm=world.size)
E0_i = fxc0.calculate(ecut=400)
f = paropen('CO.ralda_rapbe_CO.dat', 'w')
for ecut, E0 in zip(fxc0.ecut_i, E0_i):
print(ecut * Hartree, E0, file=f)
f.close()
rpa0 = RPACorrelation('CO.ralda.pbe_wfcs_CO.gpw',
txt='CO.ralda_02_CO_rpa.txt',
wcomm=world.size)
E0_i = rpa0.calculate(ecut=400)
f = paropen('CO.ralda_rpa_CO.dat', 'w')
for ecut, E0 in zip(rpa0.ecut_i, E0_i):
print(ecut * Hartree, E0, file=f)
f.close()
```

The energies for C and O are obtained from the corresponding scripts
`CO.ralda_03_C_rapbe.py`

and `CO.ralda_04_O_rapbe.py`

.
The results for various cutoffs are written to the files like `CO.ralda_rpa_CO.dat`

and `CO.ralda_rapbe_CO.dat`

.
We also print the correlation energies of the C atom to be used in a tutorial below.
As in the case of RPA the converged result is obtained by extrapolation using the script

```
import numpy as np
from gpaw.utilities.extrapolate import extrapolate
CO_rpa = np.loadtxt('CO.ralda_rpa_CO.dat')
C_rpa = np.loadtxt('CO.ralda_rpa_C.dat')
O_rpa = np.loadtxt('CO.ralda_rpa_O.dat')
a = CO_rpa
a[:, 1] -= (C_rpa[:, 1] + O_rpa[:, 1])
ext, A, B, sigma = extrapolate(a[:, 0], a[:, 1], reg=3, plot=False)
CO_rapbe = np.loadtxt('CO.ralda_rapbe_CO.dat')
C_rapbe = np.loadtxt('CO.ralda_rapbe_C.dat')
O_rapbe = np.loadtxt('CO.ralda_rapbe_O.dat')
a = CO_rapbe
a[:, 1] -= (C_rapbe[:, 1] + O_rapbe[:, 1])
ext, A, B, sigma = extrapolate(a[:, 0], a[:, 1], reg=3, plot=False)
```

If pylab is installed, the plot=False can be change to plot=True to visualize the quality of the extrapolation. The final results are displayed below

PBE |
HF |
RPA |
rAPBE |
Experimental |
---|---|---|---|---|

11.71 |
7.36 |
10.60 |
11.31 |
11.23 |

## Example 3: Cohesive energy of diamond¶

The error cancellation in RPA works best when comparing systems with similar electronic structure. In the case of cohesive energies of solids where the bulk energy is compared to the energy of isolated atoms, RPA becomes even worse than for atomization energies of molecules. Here we illustrate this for the cohesive energy of diamond and show that the rAPBE approximation corrects the problem. The initial orbitals are obtained with the script

```
from ase import Atoms
from ase.build import bulk
from ase.dft import monkhorst_pack
from ase.parallel import paropen
from gpaw import GPAW, FermiDirac
from gpaw import PW
from gpaw.hybrids.energy import non_self_consistent_energy as nsc_energy
import numpy as np
# Monkhorst-Pack grid shifted to be gamma centered
k = 8
kpts = monkhorst_pack([k, k, k])
kpts += [1. / (2 * k), 1. / (2 * k), 1. / (2 * k)]
cell = bulk('C', 'fcc', a=3.553).get_cell()
a = Atoms('C2', cell=cell, pbc=True,
scaled_positions=((0, 0, 0), (0.25, 0.25, 0.25)))
calc = GPAW(mode=PW(600),
xc='PBE',
occupations=FermiDirac(width=0.01),
convergence={'density': 1.e-6},
kpts=kpts,
parallel={'domain': 1},
txt='diamond.ralda_01_pbe.txt')
a.calc = calc
E_pbe = a.get_potential_energy()
E_hf = nsc_energy(calc, 'ECC')
E_C = np.loadtxt('CO.ralda.PBE_HF_C.dat')
f = paropen('diamond.ralda.PBE_HF_diamond.dat', 'w')
print('PBE: ', E_pbe / 2 - E_C[0], file=f)
print('HF: ', E_hf / 2 - E_C[1], file=f)
f.close()
calc.diagonalize_full_hamiltonian()
calc.write('diamond.ralda.pbe_wfcs.gpw', mode='all')
```

which takes roughly 5 minutes. The script generates `diamond.ralda.pbe_wfcs.gpw`

and uses a previous calculation of the C atom to calculate the EXX and PBE cohesive
energies that are written to `diamond.ralda.PBE_HF_diamond.dat`

. The RPA and rAPBE
correlation energies are obtained with the script:

```
from ase.parallel import paropen
from ase.units import Hartree
from gpaw.xc.rpa import RPACorrelation
from gpaw.xc.fxc import FXCCorrelation
fxc = FXCCorrelation('diamond.ralda.pbe_wfcs.gpw', xc='rAPBE',
txt='diamond.ralda_02_rapbe.txt')
E_i = fxc.calculate(ecut=400)
f = paropen('diamond.ralda.rapbe.dat', 'w')
for ecut, E in zip(fxc.ecut_i, E_i):
print(ecut * Hartree, E, file=f)
f.close()
rpa = RPACorrelation('diamond.ralda.pbe_wfcs.gpw',
txt='diamond.ralda_02_rpa.txt')
E_i = rpa.calculate(ecut=400)
f = paropen('diamond.ralda.rpa.dat', 'w')
for ecut, E in zip(rpa.ecut_i, E_i):
print(ecut * Hartree, E, file=f)
f.close()
```

This takes on the order of 30 CPU hours, but can be parallelized efficiently. Finally the correlation part of the cohesive energies are obtained by extrapolation with the script

```
from gpaw.utilities.extrapolate import extrapolate
import numpy as np
a = np.loadtxt('diamond.ralda.rpa.dat')
b = np.loadtxt('CO.ralda_rpa_C.dat')
ext, A, B, sigma = extrapolate(a[:, 0], a[:, 1] / 2 - b[:, 1],
reg=3, plot=False)
a = np.loadtxt('diamond.ralda.rapbe.dat')
b = np.loadtxt('CO.ralda_rapbe_C.dat')
ext, A, B, sigma = extrapolate(a[:, 0], a[:, 1] / 2 - b[:, 1],
reg=3, plot=False)
```

The results are summarized below

PBE |
HF |
RPA |
rAPBE |
Experimental |
---|---|---|---|---|

7.75 |
5.17 |
7.04 |
7.61 |
7.55 |

As anticipated, RPA severely underestimates the cohesive energy, while PBE performs much better, and rAPBE comes very close to the experimental value.

## Example 4: Correlation energy of diamond with different kernels¶

Finally we provide an example where we try different exchange-correlation kernels. For illustrative purposes we use a basic computational setup - as a result these numbers should not be considered converged! As usual we start with a ground state calculation to get the electron density and wavefunctions for diamond:

```
from ase.build import bulk
from gpaw import GPAW, FermiDirac
from gpaw import PW
bulk_c = bulk('C', a=3.5454859)
calc = GPAW(mode=PW(600.0),
parallel={'domain': 1},
xc='LDA',
occupations=FermiDirac(width=0.01),
kpts={'size': (6, 6, 6), 'gamma': True},
txt='diam_kern.ralda_01_lda.txt')
bulk_c.calc = calc
E_lda = bulk_c.get_potential_energy()
calc.diagonalize_full_hamiltonian()
calc.write('diam_kern.ralda.lda_wfcs.gpw', mode='all')
```

The default method of constructing the kernel is to use a two-point density average. Therefore the following simple script gets the rALDA correlation energy within this averaging scheme:

```
from gpaw.xc.fxc import FXCCorrelation
fxc = FXCCorrelation('diam_kern.ralda.lda_wfcs.gpw', xc='rALDA',
txt='diam_kern.ralda_02_ralda_dens.txt')
E_i = fxc.calculate(ecut=[131.072])
```

However, an alternative method of constructing the kernel is to work in reciprocal space,
and average over wavevectors rather than density.
To use this averaging scheme, we add the flag `av_scheme='wavevector'`

:

```
from gpaw.xc.fxc import FXCCorrelation
from ase.parallel import paropen
fxc = FXCCorrelation('diam_kern.ralda.lda_wfcs.gpw', xc='rALDA',
txt='diam_kern.ralda_03_ralda_wave.txt',
av_scheme='wavevector')
E_i = fxc.calculate(ecut=[131.072])
resultfile = paropen('diam_kern.ralda_kernel_comparison.dat', 'w')
resultfile.write(str(E_i[-1]) + '\n')
resultfile.close()
```

Using this averaging scheme opens a few more possible choices for the kernel.
For example, we can include the correlation part of the ALDA which is left out of the rALDA
by setting `xc='rALDAc'`

:

```
from gpaw.xc.fxc import FXCCorrelation
from ase.parallel import paropen
fxc = FXCCorrelation('diam_kern.ralda.lda_wfcs.gpw', xc='rALDAc',
txt='diam_kern.ralda_04_raldac.txt',
av_scheme='wavevector')
E_i = fxc.calculate(ecut=[131.072])
resultfile = paropen('diam_kern.ralda_kernel_comparison.dat', 'a')
resultfile.write(str(E_i[-1]) + '\n')
resultfile.close()
```

Alternatively, we can look at more exotic kernels, such as a simplified version of the
jellium-with-gap kernel of Ref. 5 (JGMs).
This kernel diverges as \(1/q^2\) for small \(q\), with the strength of the divergence
depending on the size of the band gap.
To use this kernel, the gap must be specified as `Eg=X`

, where X is in eV:

```
from gpaw.xc.fxc import FXCCorrelation
from ase.parallel import paropen
fxc = FXCCorrelation('diam_kern.ralda.lda_wfcs.gpw', xc='JGMs',
txt='diam_kern.ralda_04_jgm.txt',
av_scheme='wavevector',
Eg=7.3)
E_i = fxc.calculate(ecut=[131.072])
resultfile = paropen('diam_kern.ralda_kernel_comparison.dat', 'a')
resultfile.write(str(E_i[-1]) + '\n')
resultfile.close()
```

Another interesting avenue is the simple dynamical kernel of Constantin and Pitarke (CP_dyn) 6:

```
from gpaw.xc.fxc import FXCCorrelation
from ase.parallel import paropen
fxc = FXCCorrelation('diam_kern.ralda.lda_wfcs.gpw', xc='CP_dyn',
txt='diam_kern.ralda_06_CP_dyn.txt',
av_scheme='wavevector')
E_i = fxc.calculate(ecut=[131.072])
resultfile = paropen('diam_kern.ralda_kernel_comparison.dat', 'a')
resultfile.write(str(E_i[-1]) + '\n')
resultfile.close()
```

Finally, for the enthusiast there is a basic implementation of the range-separated
RPA approach of Ref. 7. By separating the Coulomb interaction into long
and short-range parts and taking the short range part from the electron gas, one can
dramatically reduce the number of plane waves needed to converge the RPA energy.
In this approach it is necessary to specify a range-separation parameter `range_rc=Y`

, where
Y is in Bohr. It is important to bear in mind that this feature is relatively untested.

```
from gpaw.xc.fxc import FXCCorrelation
from ase.parallel import paropen
fxc = FXCCorrelation('diam_kern.ralda.lda_wfcs.gpw', xc='range_RPA',
txt='diam_kern.ralda_07_range_rpa.txt',
range_rc=2.0)
E_i = fxc.calculate(ecut=[131.072, 80.0])
resultfile = paropen('diam_kern.ralda_kernel_comparison.dat', 'a')
resultfile.write(str(E_i[-1]) + '\n')
resultfile.close()
```

For comparison, one can see that the RPA converges much more slowly:

```
from gpaw.xc.fxc import FXCCorrelation
from ase.parallel import paropen
fxc = FXCCorrelation('diam_kern.ralda.lda_wfcs.gpw', xc='RPA',
txt='diam_kern.ralda_08_rpa.txt')
E_i = fxc.calculate(ecut=[131.072, 80.0])
resultfile = paropen('diam_kern.ralda_kernel_comparison.dat', 'a')
resultfile.write(str(E_i[-1]) + '\n')
resultfile.close()
```

Here we summarize the above calculations and show the correlation energy/electron (in eV), obtained at an (unconverged) cutoff of 131 eV:

rALDA (dens. av.) |
rALDA (wave. av) |
rALDAc |
JGMs |
CP_dyn |
range separated RPA |
RPA |
---|---|---|---|---|---|---|

-1.161 |
-1.134 |
-1.127 |
-1.134 |
-1.069 |
-1.730 |
-1.396 |

Incidentally, a fully converged RPA calculation gives a correlation energy of -1.781 eV per electron.

We conclude with some practical points. The wavevector-averaging scheme is less intuitive than the density-average, but avoids some difficulties such as having to describe the \(1/r\) divergence of the Coulomb interaction in real space. It also provides a natural framework to construct the JGMs kernel, and can be faster to construct for systems with many k points. However it is also worth remembering that kernels which scale linearly in the coupling constant (e.g rALDA) need only be constructed once per k point. Those that do not scale linearly (e.g. rALDAc) need to be constructed \(N_\lambda\) times, and the CP_dyn kernel must be constructed at each frequency point as well, i.e. \(N_\lambda N_\omega\) times. Assuming standard values of 8 and 16 for \(N_\lambda\) and \(N_\omega\) means there is a factor 100 cost in constructing and storing a dynamical kernel compared to rALDA. Finally we point out that the rALDA and rAPBE kernels are also special because they have explicit spin-polarized forms.

- 1
T. Olsen and K. S. Thygesen

*Phys. Rev. B***86**, 081103(R) (2012)- 2
T. Olsen and K. S. Thygesen

*Phys. Rev. B***88**, 115131 (2013)- 3
T. Olsen and K. S. Thygesen

*Phys. Rev. Lett***112**, 203001 (2014)- 4
C. E. Patrick and K. S. Thygesen

*J. Chem. Phys.***143**, 102802 (2015)- 5
P. E. Trevisanutto et al.

*Phys. Rev. B***87**, 205143 (2013)- 6
L. A. Constantin and J. M. Pitarke

*Phys. Rev. B***75**, 245127 (2007)- 7
F. Bruneval

*Phys. Rev. Lett***108**, 256403 (2012)