# Quasi harmonic approximation#

## Usage of `phonopy-qha`

#

Using phonopy results of thermal properties, thermal expansion and heat capacity
at constant pressure can be calculated under the quasi-harmonic approximation.
`phonopy-qha`

is the script to run fitting and calculation to perform it. Mind
that at leave 5 volume points are needed to run `phonopy-qha`

for fitting.

An example of the usage for `example/Si-QHA`

is as follows.

To watch selected plots:

```
% phonopy-qha -p e-v.dat thermal_properties.yaml-{-{5..1},{0..5}}
```

Without plots:

```
% phonopy-qha e-v.dat thermal_properties.yaml-{-{5..1},{0..5}}
```

The first argument is the filename of volume-energy data (in the above example,
`e-v.dat`

). The volumes and energies are given in \(\text{Angstrom}^3\) and
eV, respectively. Theses energies are only dependent on volume but not on
temperature unless using `--efe`

option. Therefore in the simplest case, these
are taken as the electronic total energies at 0K. An example of the
volume-energy file is:

```
# cell volume energy of cell other than phonon
140.030000 -42.132246
144.500000 -42.600974
149.060000 -42.949142
153.720000 -43.188162
158.470000 -43.326751
163.320000 -43.375124
168.270000 -43.339884
173.320000 -43.230619
178.470000 -43.054343
183.720000 -42.817825
189.070000 -42.527932
```

Lines starting with `#`

are ignored.

The following arguments of `phonopy-qha`

are the filenames of
`thermal_properties.yaml`

’s calculated at the volumes given in the volume-energy
file. These filenames have to be ordered in the same order as the volumes
written in the volume-energy file. Since the volume v.s. free energy fitting is
done at each temperature given in `thermal_properties.yaml`

, all
`thermal_properties.yaml`

’s have to be calculated in the same temperature ranges
and with the same temperature step. `phonopy-qha`

can calculate thermal
properties at constant pressure up to the temperature point that is one point
less than that in `thermal_properties.yaml`

because of the numerical
differentiation with respect to temperature points. Therefore
`thermal_properties.yaml`

has to be calculated up to higher temperatures than
that expected by `phonopy-qha`

.

Another example for Aluminum is found in the `example/Al-QHA`

directory.

If the condition under pressure is expected, \(PV\) terms may be included in
the energies, or equivalent effect is applied using `--pressure`

option.

Experimentally, temperature dependent energies are supported by `--efe`

option.
The usage is written at
phonopy/phonopy.

### Options#

`-h`

#

Show help. The available options are shown. Without any option, the results are saved into text files in simple data format.

`--tmax`

#

The maximum temperature calculated is specified. This temperature has to be
lower than the maximum temperature calculated in `thermal_properties.yaml`

to
let at least one temperature points fewer. The default value is `--tmax=1000`

.

`--pressure`

#

Pressure is specified in GPa. This corresponds to the \(pV\) term described in the following section Thermal properties in (T, p) space calculated under QHA. Note that bulk modulus obtained with this option than 0 GPa is incorrect.

`-b`

#

Fitting volume-energy data to an EOS, and show bulk modulus (without considering phonons). This is made by:

```
% phonopy-qha -b e-v.dat
```

`--eos`

#

EOS is chosen among `vinet`

, `birch_murnaghan`

, and `murnaghan`

. The default EOS
is `vinet`

.

```
% phonopy-qha --eos='birch_murnaghan' -b e-v.dat
```

`-p`

#

The fitting results, volume-temperature relation, and thermal expansion coefficient are plotted on the display.

`-s`

#

The calculated values are written into files.

`--sparse`

#

This is used with `-s`

or `-p`

to thin out the number of plots of the fitting
results at temperatures. For example with `--sparse=10`

, 1 in 10 temperature
curves is only plotted.

`--efe`

#

**Experimental**

Temperature dependent energies other than phonon free energy are included with this option. This is used such as:

```
% phonopy-qha -p --tmax=1300 --efe fe-v.dat e-v.dat thermal_properties.yaml-{00..10}
```

The temperature dependent energies are stored in `fe-v.dat`

. The file format is:

```
# volume: 43.08047896 43.97798894 44.87549882 45.77300889 46.67051887 47.56802885 48.46553883 49.36304881 50.26055878 51.15806876 52.05557874
# T(K) Free energies
0.0000 -17.27885993 -17.32227490 -17.34336569 -17.34479760 -17.32843604 -17.29673896 -17.25081954 -17.19263337 -17.12356816 -17.04467997 -16.95752155
10.0000 -17.27886659 -17.32228126 -17.34337279 -17.34481060 -17.32844885 -17.29675204 -17.25083261 -17.19264615 -17.12358094 -17.04469309 -16.95753464
20.0000 -17.27887453 -17.32228804 -17.34338499 -17.34482383 -17.32846353 -17.29676491 -17.25084547 -17.19265900 -17.12359399 -17.04470709 -16.95754774
...
```

The first column gives temperatures in K and the following columns give
electronic free energies in eV at temperatures and at unit (primitive) cell
volumes. The lines starting with `#`

are ignored. This file doesn’t contain the
information about cell volumes. Instead, the volumes are obtained from `e-v.dat`

file. The energies in `e-v.dat`

are not used when `--efe`

option is used. The
temperature points are expected to be the same as those in
`thermal_properties.yaml`

at least up to the maximum temperature specified for
`phonopy-qha`

.

An example is given in `example/Cu-QHA`

. The `fe-v.dat`

contains electronic free
energy calculated following, e.g., Eqs. (11) and (12) in the paper by Wolverton
and Zunger, Phys. Rev. B, **52**, 8813 (1994) (of course this paper is not the
first one that showed these equations):

with

and

where \(g\) is 1 or 2 for collinear spin polarized and non-spin polarized
systems, respectively. For VASP, a script to create `fe-v.dat`

and `e-v.dat`

by
these equations is prepared as `phonopy-vasp-efe`

, which is used as:

```
% phonopy-vasp-efe --tmax=1500 vasprun.xml-{00..10}
```

where `vasprun.xml-{00..10}`

have to be computed for the same unit cells as
those used for `thermal_properties.yaml`

. When `phonopy`

was run with
`PRIMITIVE_AXES`

or `--pa`

option, the unit cells for computing electronic
eigenvalues have to be carefully chosen to agree with those after applying
`PRIMITIVE_AXES`

, or energies are scaled a posteriori.

### Output files#

The physical units of V and T are \(\text{Angstrom}^3\) and K, respectively. The unit of eV for Helmholtz and Gibbs energies, J/K/mol for \(C_V\) and entropy, GPa for for bulk modulus and pressure are used.

Bulk modulus \(B_T\) (GPa) vs \(T\) (

`bulk_modulus-temperature.*`

)Gibbs free energy \(G\) (eV) vs \(T\) (

`gibbs-temperature.*`

)Heat capacity at constant pressure \(C_p\) (J/K/mol) vs \(T\) computed by \(-T\frac{\partial^2 G}{\partial T^2}\) from three \(G(T)\) points (

`Cp-temperature.*`

)Heat capacity at constant pressure \(C_p\) (J/K/mol) vs \(T\) computed by polynomial fittings of \(C_V(V)\) (

`Cv-volume.dat`

) and \(S(V)\) (`entropy-volume.dat`

) for \(\partial S/\partial V\) (`dsdv-temperature.dat`

) and numerical differentiation of \(\partial V/\partial T\), e.g., see Eq.(5) of PRB**81**, 174301 by Togo*et al.*(`Cp-temperature_polyfit.*`

). This may give smoother \(C_p\) than that from \(-T\frac{\partial^2 G}{\partial T^2}\).Volumetric thermal expansion coefficient \(\beta\) vs \(T\) computed by numerical differentiation (

`thermal_expansion.*`

)Volume vs \(T\) (

`volume-temperature.*`

)Thermodynamics Grüneisen parameter \(\gamma = V\beta B_T/C_V\) (no unit) vs \(T\) (

`gruneisen-temperature.dat`

)Helmholtz free energy (eV) vs volume (

`helmholtz-volume.*`

). When`--pressure`

option is specified, energy offset of \(pV\) is added. See also the following section (Thermal properties in (T, p) space calculated under QHA).

## Thermal properties in (*T*, *p*) space calculated under QHA#

Here the word ‘quasi-harmonic approximation’ is used for an approximation that introduces volume dependence of phonon frequencies as a part of anharmonic effect.

A part of temperature effect can be included into total energy of electronic
structure through phonon (Helmholtz) free energy at constant volume. But what we
want to know is thermal properties at constant pressure. We need some
transformation from function of *V* to function of *p*. Gibbs free energy is
defined at a constant pressure by the transformation:

where

means to find unique minimum value in the brackets by changing volume. Since volume dependencies of energies in electronic and phonon structures are different, volume giving the minimum value of the energy function in the square brackets shifts from the value calculated only from electronic structure even at 0 K. By increasing temperature, the volume dependence of phonon free energy changes, then the equilibrium volume at temperatures changes. This is considered as thermal expansion under this approximation.

`phonopy-qha`

collects the values at volumes and transforms into the thermal
properties at constant pressure.