# 2.3. Capabilities of WannierTools#

## 2.3.1. Bulk band calculation (points mode, line mode and plane mode)#

With the data read from the **hr.dat** file, which could be generated with the software **Wannier90**, we actually have hopping integrals of the Hamiltonian in real
space in Wannier function basis. In order to convert the
real-space Hamiltonian back to k-space, we need to do a Fourier Transformation.

where *R* is a lattice vector. To calculate band structure, we need to diagonalize H(k)

### Points mode#

You can calculate the energy bands with the given k points in the KPOINTS_3D KPOINTS_3D card.

#### Input#

Typical flags for this mode in the wt.in.

```
&CONTROL
BulkBand_points_calc = T
/
KPOINTS_3D
4 ! number of k points
Direct ! Direct or Cartesian
0.00000 0.00000 0.0000
0.00000 0.00000 0.5000
0.50000 0.50000 0.0000
0.00000 0.00000 0.0000
```

#### Output#

The outputs for this mode is **bulkek-pointsmode.dat**.
The structure for bulkek-pointsmode.dat

```
# No. of k point 1
# k1 k2 k3 kx ky kz
0.000000 0.000000 0.000000 0.000000 0.000000 0.000000
#band index Eigenvalue orbital weights (0-255)
1 1.7456780078 45 7 7 45 7 7 135 21 21 16 1 1 16 1 1 16 20 20 16 20 20 48 61 61 5 5 5 5 5 5
2 1.7456797993 16 20 20 16 20 20 48 61 61 5 5 5 5 5 5 45 7 7 45 7 7 135 21 21 16 1 1 16 1 1
```

The first line states which k point the following information belongs to. The second line specifies the vectors defined in k point and correspoinding values in the atomic basis. The remaining section is divided into several blocks, with each block containing the information for one band. Each block includes the band index, corresponding eigenvalue, and orbital weights for each projected orbital. Consequently, there are 30 weights (for Bi2Se3), one for each projectors.

### Line mode#

Calculate bulk energy band for a series k lines and project the selected orbitals onto the band structures. This is the basic calculation after the
construction of Wannier functions. You have to compare your Wannier interpolated bands
with the DFT bands. Those two bands should match well around the Fermi level.
This comparison can help verify the accuracy of the Wannier functions,
and ensure that they provide an appropriate description of the electronic structure of the system under study.
In order to obtain the parameter **NumOccupied**, you also need to calculate the bulk energy bands and plot it with
the software xmgrace.

In order to get the weight onto the projections, we need to set **SELECTED_WANNIERORBITALS** card. it
The orbital index is corresponding to the **PROJECTOS** card, nothing related to spin freedom. For example
In Bi2Se3, there are 30 Wannier functions in the hr.dat, however, there are only 15 projectors (orbitals).
So indices in **SELECTED_WANNIERORBITALS** are from 1 to 15.

#### Input#

Typical flags for bulk band calculation in the wt.in.

```
&CONTROL
BulkBand_calc = T
/
&PARAMETERS
Nk1 = 101 ! Number of k points for each k line
/
! get projected bands onto different orbitals, here we only consider orbital and omit the spin freedom
SELECTED_WANNIERORBITALS
2
1-6 ! Bi
7-15 ! Se
KPATH_BULK ! k point path
4 ! number of k lines only for bulk band
G 0.00000 0.00000 0.0000 Z 0.00000 0.00000 0.5000
Z 0.00000 0.00000 0.5000 F 0.50000 0.50000 0.0000
F 0.50000 0.50000 0.0000 G 0.00000 0.00000 0.0000
G 0.00000 0.00000 0.0000 L 0.50000 0.00000 0.0000
```

See CONTROL, PARAMETERS, KPATH_BULK

#### Output#

The outputs for bulk band calculation are **bulkek.dat** and **bulkek.gnu**. You can get the band plot by running

```
gnuplot bulkek.gnu
```

or

```
xmgrace bulkek.dat
```

to get a band stucture plot.

The data structure for **bulkek.dat**

```
0.000000000 -2.673821992 119 80 80 119 80 80 205 138 138 70 40 40 70 40 40 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
0.016453872 -2.681536808 118 78 78 118 78 78 203 134 134 82 41 41 82 41 41 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
```

The 1st column represents k points for the given kpath (KPATH_BULK)

The 2nd column is the energy level

From the 3rd to the n’th column are the projected weight of the wave function at each k point and each band onto each wannier orbitals. Those weights are normalized to 255 for the color plot convinence.

The subrotine for this feature is ek_bulk.f90 .

#### Examples#

Two examples Bi2Se3 and Graphene were prepared:

Strong topological insulator Bi2Se3 (in order to get the fat-band plot, you need to modify bulkek.gnu following the instruction inside)

```
$ cd examples/Bi2Se3
$ cp wt.in-bands wt.in
$ ../../bin/wt.x
$ gnuplot bulkek.gnu
```

2D Dirac semimetal Graphene

```
$ cd examples/Graphene
$ cp wt.in-bands wt.in
$ ../../bin/wt.x
$ gnuplot bulkek.gnu
```

The band plots of Bi2Se3 and Graphene should be like this

Note

In order to get the latex symbol \(\Gamma\) in gnuplot, you need to replace **“G”** to **“{/Symbol G}”** in the bulkek.gnu like this

set xtics (“M “ 0.00000,”K “ 0.84848, **“{/Symbol G}”** 2.54543,”M “ 4.01504)

### Plane mode#

Calculate band structure in a k slice(plane) specified by KPLANE_BULK card.
The mode is very useful to visualize the Dirac/Weyl cone. You have to set the following necessary tags in **wt.in**

```
!> bulk band structure calculation flag
&CONTROL
BulkBand_plane_calc = T
/
&SYSTEM
NumOccupied = 1 ! only write out 4 bands around NumOccpuied
SOC = 0 ! soc
E_FERMI = -1.2533 ! e-fermi
/
&PARAMETERS
Nk1 = 201 ! number k points
Nk2 = 201 ! number k points
/
KPLANE_BULK ! fractional coordinates
0.333333 0.333333 0.000000 ! Middle point for a k slice(plane) in 3D BZ. Usually, the position of Dirac points.
0.100000 0.000000 0.000000 ! The first vector to define k plane(slice) in 3D BZ
0.000000 0.100000 0.000000 ! The second vector to define k plane(slice) in 3D BZ
```

The output file is **bulkek_plane.dat**, **bulkek_plane-matlab.dat** and **bulkek_plane.gnu**. You can get
**bulkek_plane.png** with

```
$ gnuplot bulkek_plane.gnu
```

The **bulkek_plane-matlab.dat** is in MATLAB data format. You can plot the Dirac cone with matlab.

The format of **bulkek_plane.dat** is as follows:

```
# kx ky kz k1 k2 k3 E(Numoccupied-1) E(Numoccupied) E(Numoccupied+1) E(Numoccupied+2)
-0.299354337 -0.518496963 0.180167841 -0.518496936 -0.299354384 0.180167841 -1.311721381 -1.311705191 0.588683811 0.588872215
-0.299354337 -0.504670376 0.180167841 -0.511583643 -0.287380208 0.180167841 -1.294078082 -1.293904952 0.586780093 0.587249790
...
```

Column 1-3rd are k points in cartesian coordinates. Column 4-6th are k points in a rotated cartesian coordinates
where the x and y direction are line in the k plane and the z direction is perpendicular to the k plane you specified.
Column 7-10th are energies at each k point. Here we only print out 4 energy bands around the fermilevel. It depends on **NumOccupied**.
Usually, I choose column 4th and 5th as k coordinates and choose 8 and 9 as energy bands to show the Dirac cone shown below.

#### Example#

There is one example in the examples/Graphene

```
$ cd examples/Graphene
$ cp wt.in-bands-plane wt.in
$ ../../bin/wt.x
$ gnuplot bulkek_plane.gnu
```

The output is bulkek_plane.png and should like this

Note

Sometimes, you need to modify bulkek_plane.gnu to get correct plot. For example, in Graphene, there a only 2 bands in total. So you need to change the last two lines to

splot ‘bulkek_plane.dat’ u 4:5:

7w pm3d, ‘bulkek_plane.dat’ u 4:5:8w pm3d

## 2.3.2. 3D Fermi surface calculation#

Fermi surface calculation of the bulk system.

When calculating systems with SOC=0, meaning no spin-orbit coupling,
WannierTools computes 12 bands from the **NumOccupied-5** to **NumOccupied+6** energy levels.
However, when calculating systems with SOC=1, meaning spin-orbit coupling is present,
WannierTools computes 16 bands from the **NumOccupied-7** to **NumOccupied+8** energy levels.

Note

1. In order to reduce the storage of the Fermi surface, we only write out few energy bands around NumOccupied’th bands.
If SOC=0, then we write out about 12 bands [Numoccupied- 5, Numoccupied+ 6]. If SOC=1, then we write out about 16 bands
[Numoccupied- 7, Numoccupied+ 8]. So please set **NumOccupied** to be the band index of the band crossing the Fermi level.
for more information about **Numoccpuied**, please refer to SYSTEM. If you want to write out more bands, please
modify the source code at src/fermisurface.f90 around line 31-37 of subroutine fermisurface3D. And you have to
recompile the code after the modification.

2. The first numerical line of KCUBE_BULK should be (0, 0, 0) in order to get right plots in xcrysden. You should not set it to other values unless you use other software to visualize the Fermi surfaces or you know what you are doing.

### Input#

You should specify the number of k points for each three reciprocal vectors Nk1, Nk2, Nk3 in NAMELISTS PARAMETERS

```
&CONTROL
BulkFS_calc = T
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
Nk2 = 101 ! No. of slices for the 2nd reciprocal vector
Nk3 = 101 ! No. of slices for the 3rd reciprocal vector
/
KCUBE_BULK
0.00 0.00 0.00 ! Original point for 3D k plane, For BulkFS_calc, this should be always be 0 0 0
1.00 0.00 0.00 ! The first vector to define 3d k space plane
0.00 1.00 0.00 ! The second vector to define 3d k space plane
0.00 0.00 1.00 ! The third vector to define 3d k cube
```

See CONTROL, PARAMETERS

### Output#

The outputs for this function are **FS3D.bxsf**.
You can plot the FS with xcrysden run

```
$ xcrysden --bxsf FS3D.bxsf
```

or using FermiSurfer (version larger than 2.0.0)

```
$ fermisurfer FS3D.bxsf
```

By the way, Bulk band and BulkFS calculations were already implemented in Wannier90 code.

### Example#

There is one example in the examples/TiB2

```
$ cd examples/TiB2/
$ cp wt.in-3dfs wt.in
$ mpiexec -np 8 ../../bin/wt.x
$ xcrysden --bxsf FS3D.bxsf
$ fermisurfer FS3D.bxsf
```

## 2.3.3. A cross-section of the Fermi surface#

Bulk Fermi surface in a fixed k plane specified by **KPLANE_BULK** and at a fixed energy specified by **E_arc**.
The Fermi surface in a k-plane is calculated by the Green’s function. The spectral function can be
expressed by advanced Green’s function.

where the fixed energy \(\omega\) = **E_arc** and a Fermi broadening factor \(\eta\) = **Eta_arc**

### Input#

You should specify the number of k points for each three reciprocal vectors Nk1, Nk2 in NAMELISTS PARAMETERS

```
&CONTROL
BulkFS_plane_calc = T
Translate_to_WS_calc = F ! if True, then only write out the spectrum in the 1st BZ
/
&SYSTEM
SOC = 0 ! without
E_FERMI = 6.3906 ! e-fermi in the hr.dat
/
&PARAMETERS
Eta_arc = 0.02 ! infinite small value, like brodening
E_arc = 0.0 ! energy for calculate Fermi Arc
Nk1 = 201 ! number k points odd number would be better
Nk2 = 201 ! number k points odd number would be better
/
KPLANE_BULK ! unit is the reciprocal lattice vectors
0.00 0.00 0.00 ! center point for 3D k plane
2.00 0.00 0.00 ! The first vector to define 3d k space plane
0.00 2.00 0.00 ! The second vector to define 3d k space plane
```

See CONTROL, PARAMETERS

### Output#

The outputs for this function are **fs_kplane.dat, fs_kplane.gnu**.

gnuplot fs_kplane.gnu

to get the plot.

### Example#

There is one example in the examples/TiB2

```
$ cd examples/TiB2/
$ cp wt.in-fs_kplane wt.in
$ mpiexec -np 8 ../../bin/wt.x
$ gnuplot fs_kplane.gnu
```

## 2.3.4. Bulk spin texture calculations#

Calculate spin texture for bulk system that with vacuum or without inversion symmetry. For the bulk system with vacuum, you can calculate the surface projected spin texture. This is useful for comparing with the ARPES experiments. if you cut a slab system from a periodic tight binding model, then there is no charge relaxation on the surface which would change the surface state a lot. In this case, you have to do the first-principle calculations for a finite thickness slab system that with vacuum. Then you can construct Wannier functions for this system and use WannierTools to get the iso-energy plot of the Fermi surface (BulkFS_plane_calc =T) and get the surface projected spin texture (Bulkspintext_calc=T).

There is one example in the examples/Bi2Se3-6Qlayers.

The spin texture can be obtained with

\(\sigma\) stands for Pauli matrix.

There is one example in the examples/Bi2Se3-6Qlayers.

You should specify E_arc, eta_arc, Nk1, Nk2, NSLAB, E_FERMI in **wt.x** file

```
&CONTROL
BulkSpintexture_calc = T
/
&SYSTEM
NSLAB = 1 ! for thin film system
NumOccupied = 144 ! NumOccupied
E_FERMI = 2.5519
SOC = 1
/
&PARAMETERS
Nk1 = 21 ! number k points odd number would be better
Nk2 = 21 ! number k points odd number would be better
E_arc = 0.3 ! iso-energy
eta_arc = 0.001 ! infinite small value, like broadening
/
SELECTED_ATOMS ! projection only onto the selected atoms
2 ! number groups of selected atoms
6 12 18 24 30 ! top surface's atoms
1 7 13 19 25 ! bottom surface's atoms
```

The outfiles include **bulkspintext.dat** and **bulkspintext.gnu**.

The format of bulkspintext.dat

```
# kx ky kz kp1 kp2 kp3 | A(k,E) total |group 1: A sx sy sz |group 2: A sx sy sz |group
#column 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15
0.00000000 0.17533097 -0.04387697 -0.09243483 -0.15531240 0.00000000 1.99551113 0.30759819 -0.00000000 -0.00000000 0.00000000 0.30844716 -0.00000000 -0.00000000 0.00000000
0.00303682 0.17357766 -0.04343820 -0.09412010 -0.15220615 0.00000000 2.01557956 0.31199054 -0.00000000 -0.00000000 0.00000000 0.31294339 -0.00000000 -0.00000000 0.00000000
0.00607364 0.17182435 -0.04299943 -0.09580537 -0.14909990 0.00000000 2.02732969 0.31554459 -0.00000000 -0.00000000 0.00000000 0.31659405 -0.00000000 -0.00000000 0.00000000
0.00911047 0.17007104 -0.04256066 -0.09749063 -0.14599365 0.00000000 2.03080158 0.31822130 -0.00000000 -0.00000000
```

plot the data with

```
gnuplot bulkspintext.gnu
```

## 2.3.5. Density state(DOS) calculations#

The formula is

```
.. math:: DOS(\omega) = \frac{1}{N_k} \sum_k \delta(\omega-E(k))
.. math:: \delta(x)= e^{-x^2/\eta/\eta/2d0}/\sqrt(2\pi)/\eta
```

Calculation density of state for the bulk system. The typical setup in **wt.in**:

```
&CONTROL
DOS_calc = T
/
&PARAMETERS
Eta_Arc = 0.01 ! Fermi broadening
OmegaNum = 601 ! number of slices of energy
OmegaMin = -1.0 ! erergy range for DOS
OmegaMax = 1.0
Nk1 = 51 ! No. of slices for the 1st reciprocal vector
Nk2 = 51 ! No. of slices for the 2nd reciprocal vector
Nk3 = 51 ! No. of slices for the 3nd reciprocal vector
/
KCUBE_BULK
0.00 0.00 0.00 ! Original point for 3D k plane
1.00 0.00 0.00 ! The first vector to define 3d k space plane
0.00 1.00 0.00 ! The second vector to define 3d k space plane
0.00 0.00 1.00 ! The third vector to define 3d k cube
```

Outputs are **dos.dat** and **dos.gnu**. **dos.pdf** will be obtained with

```
gnuplot dos.gnu
```

The dos.dat looks like this

```
# Density of state of bulk system
# E(eV) DOS(E) (1/eV)
#Broadening \eta (meV): 0.10 0.20 0.40 0.80 1.00 2.00 4.00 8.00 10.00
-0.600000 4.486787 4.468209 4.532150 4.465199 4.428096 4.376913 4.436603 4.552139 4.601164
-0.596321 4.980748 4.941778 4.783586 4.599825 4.521006 4.344811 4.404406 4.534348 4.582083
```

Note

On input, we only set one broadening parameter **Eta_arc**, however, on output, we will generate 9 DOSs with
9 different broadenings. Eta= Eta_arc* [0.1, 0.2, 0.4, 0.8, 1.0, 2, 4, 8, 10].

You should select the one that is smooth and has small broadening.

The first column specifies the energy and the other columns list the DOS respect to different energy broadening(i.e \(\sigma\) in Gaussian distribution)

Here is one example about DOS calculation of Graphene. See examples/Graphene/wt.in-dos

## 2.3.6. Energy gap calculations (plane and cube mode)#

We support two modes for energy gap calculations.The formula is \(gap(k)= E_{NumOccupied+1}(k)- E_{NumOccpuied}(k)\)

### Gap_plane mode#

Calculate the energy gap for the k points in the KPLANE_BULK. This is useful to show Weyl points and nodal line structure.

#### Input#

Typical input parameters for BulkGap_plane calculation

```
&CONTROL
BulkGap_Plane_calc = T
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
Nk2 = 101 ! No. of slices for the 2nd reciprocal vector
/
KPLANE_BULK
0.00 0.00 0.00 ! Original point for 3D k plane
1.00 0.00 0.00 ! The first vector to define 3d k space plane(slice)
0.00 0.50 0.00 ! The second vector to define 3d k space plane(slice)
```

See CONTROL, PARAMETERS, KPATH_BULK

#### Output#

The outputs for Gap_plane mode are **GapPlane.dat**, **GapPlane.gnu**. The **GapPlane.png** will get by

```
gnuplot GapPlane.gnu
```

The head of **GapPlane.dat**

```
kx ky kz gap Ev4 Ev3 Ev2 Ev1 Ec1 Ec2 Ec3 Ec4 k1 k2 k3
0.00000000 0.00000000 0.00000000 0.45569845 -0.69109275 -0.69109055 -0.29654328 -0.29654073 0.15915772 0.15915871 1.24348171 1.24348457 0.00000000 0.00000000 0.00000000
0.03796028 -0.02191637 0.00548462 0.43770730 -0.77636510 -0.77598312 -0.26035113 -0.26027881 0.17742849 0.17771545 1.29499437 1.29505298 0.00000000 0.02500000 0.00000000
```

Column 1-3 are the Cartesian coordinates of the k points in the KPLANE_BULK, in unit of \(\frac{1}{Angstrom}\)

Column 4 is the energy gap

Column 5-12 are the energy value for valence and conduction bands close to the Fermi level. There are 4 conduction bands and 4 valence bands.

Column 13-15 are the Direct coordinates of the k points in the KPLANE_BULK

### Gap_Cube mode#

This helps us to find Weyl points and nodal line structure in the 3D BZ.

#### Input#

Typical input parameters for BulkGap_cube calculation

```
&CONTROL
BulkGap_Cube_calc = T
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
Nk2 = 101 ! No. of slices for the 2nd reciprocal vector
Nk3 = 101 ! No. of slices for the 3rd reciprocal vector
/
KCUBE_BULK
-0.50 -0.50 -0.50 ! Original point for 3D k plane
1.00 0.00 0.00 ! The 1st vector to define 3d k cube
0.00 1.00 0.00 ! The 2nd vector to define 3d k cube
0.00 0.00 1.00 ! The 3rd vector to define 3d k cube
```

See CONTROL, PARAMETERS, KCUBE_BULK

#### Output#

The outputs for Gap_plane mode are **GapCube.dat**, **GapCube.gnu**. The **GapCube.png** will get by

```
gnuplot GapCube.gnu
```

The head of **GapCube.dat** are

```
kx (1/A) ky (1/A) kz (1/A) Energy gap Ev Ec k1 (2pi/a) k2 (2pi/b) k3 (2pi/c)
0.00000000 0.87665487 -0.54846229 0.79075142 -0.34827281 0.44247861 -0.50000000 -0.50000000 -0.50000000
0.00000000 0.87665487 -0.51555455 0.86792416 -0.38635069 0.48157346 -0.50000000 -0.50000000 -0.45000000
```

Column 1-3 are the Cartesian coordinates of the k points where energy gap is small than Gap_threshold, in unit of \(\frac{1}{Angstrom}\)

Column 4 is the energy gap. Those values are smaller than Gap_threshold, see PARAMETERS

Column 5-6 are the energy value for valence and conduction bands close to the Fermi level. There are 4 conduction bands and 4 valence bands.

Column 7-9 are the Direct coordinates of the k points.

## 2.3.7. Find Nodes calculation#

Beside by using GapCube and GapPlane to find Weyl/Dirac nodes or node lines, we can directly using FindNodes function. \(gap(k)= E_{NumOccupied+1}(k)- E_{NumOccpuied}(k)\)

### Input#

Typical input parameters for FindNodes_cube calculation

```
&CONTROL
FindNodes_calc = T
/
&PARAMETERS
Nk1 = 8 ! No. of slices for the 1st reciprocal vector
Nk2 = 8 ! No. of slices for the 2nd reciprocal vector
Nk3 = 8 ! No. of slices for the 3rd reciprocal vector
Gap_threshold = 0.0001 ! a value to determine which point should be identified as a node
/
KCUBE_BULK
-0.50 -0.50 -0.50 ! Original point for 3D k plane
1.00 0.00 0.00 ! The 1st vector to define 3d k cube
0.00 1.00 0.00 ! The 2nd vector to define 3d k cube
0.00 0.00 1.00 ! The 3rd vector to define 3d k cube
```

Note

Please don’t set Nk1, Nk2, Nk3 too large. Otherwise, it will become very time consuming. Usually, 15*15*15 is enough to get converged number of Weyl/Dirac points.

### Output#

Outputs are **Nodes.dat** and **Nodes.gnu**. Nodes.png will be obtained by

```
gnuplot Nodes.gnu
```

Here are heads of output for WTe2 **Nodes.dat**

```
# local minimal position and the related energy gap
# kx ky kz gap E k1 k2 k3
0.219436 -0.045611 -0.000001 0.000000 0.056688 0.121432 -0.045363 -0.000003
-0.219515 -0.045063 -0.000001 0.000000 0.056461 -0.121476 -0.044818 -0.000002
0.220195 -0.038682 -0.000002 0.000000 0.051264 0.121852 -0.038472 -0.000003
-0.220183 -0.038936 -0.000001 0.000000 0.051618 -0.121845 -0.038724 -0.000003
0.219514 0.045063 0.000001 0.000000 0.056459 0.121475 0.044818 0.000003
-0.219434 0.045620 0.000002 0.000000 0.056692 -0.121431 0.045371 0.000004
-0.220194 0.038678 0.000000 0.000000 0.051259 -0.121851 0.038468 0.000001
0.220181 0.038941 0.000000 0.000000 0.051620 0.121844 0.038729 0.000001
```

You will find that there are 8 Weyl points in the BZ as expected.

## 2.3.8. Weyl Chirality calculation#

After you identify the positions of Weyl points, you could use this function to calculate the chirality, which tells you whether a Weyl point is a sink or a source of the Berry Curvature.

### Input#

Typical input parameters for WeylChirality_calc calculation

```
&CONTROL
WeylChirality_calc = T
/
&PARAMETERS
Nk1 = 41 ! No. of slices for the 1st reciprocal vector, berry phase integration direction
Nk2 = 21 ! No. of slices for the 2nd reciprocal vector
/
WEYL_CHIRALITY
8 ! Num_Weyls
Cartesian ! Direct or Cartesian coordinate
0.004 ! Radius of the ball surround a Weyl point
0.219436 -0.045611 -0.000000 ! Positions of Weyl points, No. of lines should larger than Num_weyls
-0.219515 -0.045063 -0.000000
0.220195 -0.038682 -0.000000
-0.220183 -0.038936 -0.000000
0.219514 0.045063 0.000000
-0.219434 0.045620 0.000000
-0.220194 0.038678 0.000000
0.220181 0.038941 0.000000
```

### Output#

Outputs are **wanniercenter3D_Weyl.dat** and **wanniercenter3D_Weyl_i.gnu**. wanniercenter3D_Weyl.png will be obtained by

```
gnuplot wanniercenter3D_Weyl_i.gnu
for ((i=1; i<9; i++)); do gnuplot wanniercenter3D_Weyl_$i.gnu;done
```

Note

i is an integer from 1 to Num_weyls

Here are heads of output for WTe2 **wanniercenter3D_Weyl.dat**

```
# Chirality -1 1 1 -1 1 -1 1 -1
# k phase phase phase phase phase phase phase phase
0.00000000 0.99970932 0.00005854 0.00004671 0.99975139 0.00005851 0.99970861 0.00004736 0.99975087
0.05000000 0.89229069 0.08696587 0.08941971 0.90855415 0.08723118 0.89170870 0.09022452 0.90795187
0.10000000 0.79659821 0.16589558 0.17112299 0.82248889 0.16697194 0.79511289 0.17279423 0.82108022
```

The first line shows the chiralities of each Weyl point. The first column is k point. From the 2nd to the last column show the Wannier charge center phase. In total, there are Num_weyls columns.

## 2.3.9. Slab band calculation#

Before using iterative green’s function to get the surface state spectrum for semi-infinite system. We also can just construct a finite thickness slab system and calculate the band structure for it.

Note

For slab calculations, please read carefully the input card SURFACE

### Input#

```
&CONTROL
SlabBand_calc = T
/
&SYSTEM
NSLAB = 10
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
/
KPATH_SLAB
2 ! numker of k line for 2D case
K 0.33 0.67 G 0.0 0.0 ! k path for 2D case
G 0.0 0.0 M 0.5 0.5
```

See CONTROL, SYSTEM PARAMETERS, KPATH_SLAB

### Output#

Outputs are **slabek.dat** and **slabek.gnu**

The heads of **slabek.dat** are

```
0.0000000 -4.9575466 240
0.0508687 -5.0110528 226
0.1017373 -5.0566963 221
0.1526060 -5.0671994 220
...
```

The 1st column are k points in the KPATH_SLAB

The 2nd column are energy values.

The 3rd column represent the surface weight, which is normalized to 255.

The colorfull plot **slabek.png** of the slab energy bands can be obtained by

```
gnuplot slabek.gnu
```

## 2.3.10. Nanowire/nanoribbon band calculation#

Band calculation for wire system. Only one direction is periodic, the other two directions are confined.

### Input#

You don’t have to set the k path, because it only has one direction.

```
&CONTROL
WireBand_calc = T
/
&SYSTEM
NSLAB1 = 4
NSLAB2 = 4
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
/
```

See CONTROL, SYSTEM PARAMETERS

### Output#

Outputs are **ribbonek.dat** and **ribbonek.gnu**. The data format of **ribbonek.dat** is the same as
**slabek.dat**. Get plot ribbonek.png with

```
gnuplot ribbonek.gnu
```

## 2.3.11. Surface state ARPES calculation#

One important feature for topological materials is the surface state. The bulk-edge correspondence tells us, if the topological property of the bulk system is nontrivial, then there will be nontrivial states on the surface. Nowadays, there are several method to detect the surface states. One direct way is the angle resolved photoemission spectroscopy (ARPES). Such spectrum can be obtained by the iterative Green’s function.

Note

For slab calculations, please read carefully the input card SURFACE

### Input#

```
&CONTROL
SlabSS_calc = T
/
&PARAMETERS
OmegaNum = 101
OmegaMin = -1.0
OmegaMax = 1.0
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
NP = 2 ! principle layer
/
KPATH_SLAB
2 ! numker of k line for 2D case
K 0.33 0.67 G 0.0 0.0 ! k path for 2D case
G 0.0 0.0 M 0.5 0.5
```

See CONTROL, PARAMETERS, KPATH_SLAB

NP : integer valued, Number of principle layers, see details related to iterative green’s function. Used if SlabSS_calc= T, SlabArc_calc=T, SlabSpintexture_calc=T. Default value is 2. You need to do a convergence test by setting Np= 1, Np=2, Np=3, and check the surface state spectrum. Basically, the value of Np depends on the spread of Wannier functions you constructed. One thing should be mentioned is that the computational time grows cubically of Np.

### Output#

The output files are **surfdos_l.dat**, **surfdos_r.dat**, **surfdos_l.gnu**, **surfdos_r.gnu**. You could get the the spectral function
plots with

```
gnuplot surfdos_l.gnu
gnuplot surfdos_r.gnu
```

**_l** and **_r** means the top and bottom surface.

## 2.3.12. Surface state QPI calculation#

Settings for this feature are almost the same as Fermi arc calculation. Only difference is that you should set

```
# please set SlabQPI_kplane_calc = T from V2.4.2
&CONTROL
SlabQPI_kplane_calc = T
/
```

### Output#

- There are a lot of outputs for QPI calculation. including
arc.dat_l, arc.dat_r, arc_l.gnu, arc_r.gnu, arc.jdat_l, arc.jdat_r, arc.jsdat_l, arc.jsdat_r, arc_l_jdos.gnu, arc_l_jsdos.gnu, arc_r_jdos.gnu, arc_r_jsdos.gnu.

The gnu script with ‘only’ means we only plot the spectrum with the surface contribution, exclude the bulk contribution. (we remove file arc_l_only.gnu after v2.4.1 for the reason of misleading) jdat_l is the QPI data without consideration of spin scattering. jsdat_l is the QPI data in consideration of spin scattering.

Note

This is a note

## 2.3.13. Fermi arc calculation#

Surface state spectrum at fixed energy level E_arc set in NAMELISTS PARAMETERS . Set SlabArc_calc=T,
and set Nk1, Nk2, in NAMELISTS PARAMETERS, set k plane in KPLANE_SLAB CARD.
Get the plots with “gnuplot arc_l.gnu”, “gnuplot arc_r.gnu”. **_l** and **_r** means the top and bottom surface.

## 2.3.14. Spin texture calculation#

Spin texture calculation at a fixed energy level E_arc set in NAMELISTS PARAMETERS . Set Slabspintexture_calc=T, and set Nk1, Nk2, in NAMELISTS PARAMETERS, set k plane in KPLANE_SLAB CARD. Get the plots with “gnuplot spintext_l.gnu”, “gnuplot spintext_r.gnu”.

Note

Here we asumme that the tight-binding basis are pure spin up or pure spin down, which means that the spin up and spin down are not mixed in the basis. This could be realized if you don’t do the maximal-localized step by setting num_iter=0 in wannier90.win and select the projectors, disentanglement windown properly. If your Wannier functions are the maximal localized ones, then this feature doesn’t work. I suggest you using Wannier90 to get spin-texture which needs information from the first-principle calculations.

## 2.3.15. Berry phase calculation#

Calculate Berry phase of a closed k path in 3D BZ. This is useful in a nodal line system. It is demonstrated that the Berry phase around a closed mirror symmetric k loop is either 0 or pi for a mirror protect nodal line system.

In WannierTools, you can specify a k path by a serials k points. Here we take the WC example, which has two nodal lines around K point.

### Input#

```
&CONTROL
BerryPhase_calc = T
/
&SYSTEM
NumOccupied = 10 ! Number of occupied Wannier orbitals
/
&PARAMETERS
Nk1 = 21 ! No. of slices for the 1st reciprocal vector
/
KPATH_BERRY
11
Direct
0.3 0.333 -0.2
0.3 0.333 -0.1
0.3 0.333 -0.0
0.3 0.333 0.1
0.3 0.333 0.2
0.33 0.333 0.2
0.33 0.333 0.1
0.33 0.333 0.0
0.33 0.333 -0.1
0.33 0.333 -0.2
0.3 0.333 -0.2
```

### Output#

The value of Berry phase can be found in the **WT.out**.

Note

1. In principlely, the Berry phase for around a nodal line should be interger. However, the MLWF-TB model usally is not symmetric. So the value of Berry phase is close to zero or one.

The first and the last kpoints in the KPATH_BERRY should be the same to form a loop.

## 2.3.16. Berry curvature calculation for 3D bulk case#

Calculate Berry curvature at a fixed k plane in 3D BZ. Set BerryCurvature_calc=T, and set Nk1, Nk2, in NAMELISTS PARAMETERS, set k plane in KPLANE_BULK CARD. Get the plot with “gnuplot Berrycurvature.gnu”.

please set NumOccpuied correctly. It represents the “occpuied” wannier bands, not the total number of electrons. In this application, the Berrycurvature is the summation over NumOccupied bands.

A typical input (take ZrTe as an example):

```
&CONTROL
BerryCurvature_calc=T
/
&SYSTEM
NumOccupied = 8 ! Number of occupied Wannier orbitals
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
Nk2 = 101 ! No. of slices for the 2st reciprocal vector
/
KPLANE_BULK
0.00 0.00 0.00 ! Central point for 3D k slice k3=0
1.00 0.00 0.00 ! The first vector. Integrate along this direction to get WCC
0.00 1.00 0.00 ! WCC along this direction, for Z2, usually half of the reciprocal lattice vector
```

## 2.3.17. Berry curvature calculation for slab system#

Note

Not well tested.. Use it carefully.

A typical input:

```
&CONTROL
BerryCurvature_slab_calc=T
/
&SYSTEM
NumOccupied = 8 ! Number of occupied Wannier orbitals of the unit cell
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
Nk2 = 101 ! No. of slices for the 2st reciprocal vector
/
KPLANE_SLAB
0.00 0.00 ! Central point for 3D k slice k3=0
1.00 0.00 ! The first vector. Integrate along this direction to get WCC
0.00 1.00 ! WCC along this direction, for Z2, usually half of the reciprocal lattice vector
```

## 2.3.18. Anomalous Hall conductivity (AHC)#

Calculate AHC in the energy range [OmegaMin, OmegaMax]. AHC is in unit of (Ohm*cm)^-1.

Relevant inputs are

```
&CONTROL
AHC_calc=T
/
&PARAMETERS
OmegaNum = 601 ! number of slices of energy
OmegaMin = -1.0 ! erergy range for AHC
OmegaMax = 1.0
Nk1 = 51 ! No. of slices for the 1st reciprocal vector
Nk2 = 51 ! No. of slices for the 2nd reciprocal vector
Nk3 = 51 ! No. of slices for the 3nd reciprocal vector
/
KCUBE_BULK
0.00 0.00 0.00 ! Original point for 3D k plane
1.00 0.00 0.00 ! The first vector to define 3d k space plane
0.00 1.00 0.00 ! The second vector to define 3d k space plane
0.00 0.00 1.00 ! The third vector to define 3d k cube
```

Output is **sigma_ahe.txt**.

## 2.3.19. Wannier charge center/Wilson loop calculation#

Wannier charge center, which is sometimes called Wilson loop can be calculated by set WannierCenter_calc=T and set KPLANE_BULK CARD, set number of k points for two vectors is Nk1, Nk2 in NAMELISTS PARAMETERS. Notice: You should notice that the first vector in KPLANE_BULK CARD is the integration direction, this vector should be equal to one primitive reciprocal lattice vector. If you want to calculate the Z2 number, Please set the second vector to be half of the reciprocal lattice vector. You can get the Wannier charge center along the second k line. See more details In the paper written by Alexey. Soluyanov (2011). If you want to calculate the Chern number, Please set the second vector to be one primitive reciprocal lattice vector.

Note

Important: please set **NumOccpuied** correctly. It represents the “occpuied” wannier bands, not the total number of electrons.
In this application, the Wilson loop is the trace of NumOccupied bands. If you want to study the topology between the 8th and the 9th band,
then set NumOccupied=8.

### Output#

Outputs are **wcc.dat** and **wcc.gnu**, the format of **wcc.dat** is:

```
# k largestgap sum(wcc(:,ik)) wcc(i, ik)(i=1, NumOccupied)
0.00000000 0.60940556 0.99998388 0.00000850 0.07701431 0.07702018 0.19328973 0.19329593 0.28118760 0.28119336 0.49998615 0.50000060 0.71881052 0.71881646 0.80675987 0.80676424 0.92297767 0.92298328 0.99993530 0.99994085 0.99999935
0.00312500 0.61256609 0.99998716 0.00030351 0.00082300 0.07688154 0.07709302 0.19117885 0.19525313 0.27952027 0.28297172 0.49188658 0.50810192 0.71703027 0.72048573 0.80480135 0.80887751 0.92290159 0.92311931 0.99908212 0.99967575
0.00625000 0.61569946 0.99999557 0.00061525 0.00168708 0.07668131 0.07711296 0.18887026 0.19709893 0.27796336 0.28485788 0.48373617 0.51625672 0.71514220 0.72204447 0.80295562 0.81118878 0.92287871 0.92332259 0.99821913 0.99936414
......
```

The second column is the position of the largest gap of WCC. It is used for drawing a line to calculate the Z2 number (see A. Soluyanov 2011), From the fourth column to the last column, they are wcc for the occupied bands specified with “NumOccupied”. The third line is the summation of the WCC over all the “occupied” bands. It’s usefull for telling the Chern number.

### Example#

Take Bi2Se3 for example, we calculate the Wilson loop (WCC) at k3=0 plane, where k1, k2, k3 is in unit of reciprocal lattice vector. The you should set the particular inputs like this

```
&CONTROL
WannierCenter_calc=T
/
&SYSTEM
NumOccupied = 10 ! Number of occupied Wannier orbitals
/
&PARAMETERS
Nk1 = 41 ! No. of slices for the 1st reciprocal vector
Nk2 = 41 ! No. of slices for the 2st reciprocal vector
/
KPLANE_BULK
0.00 0.00 0.00 ! Original point for 3D k slice k3=0
1.00 0.00 0.00 ! The first vector. Integrate along this direction to get WCC
0.00 0.50 0.00 ! WCC along this direction, for Z2, usually half of the reciprocal lattice vector
```

For 2D materials stacked along z direction, you could think it as a 3D material with weak coupling along z direction. You can use this function to get the Z2 value at k3=0 plane to characterize the topology.

Use “gnuplot wcc.gnu” to get “wcc.eps” plot.

Here is an example.

## 2.3.20. Mirror Chern number calculation#

At present, We can only calculate mirror Chern number for the simplest case (1. There is only one atom per atom’s type in the unit cell e.g. ZrTe. 2. kz=0 is the mirror plane we concern). For the more complex case, you can modify the source code by setting the mirror operator properly. Define your own mirror operator based on the atomic like Wannier functions in the symmetry.f90 and change the subroutine wanniercenter_mirror in wanniercenter.f90.

After properly setting of the mirror operator, you can run WannierTools with the basic parameters and the following additional parameters (Here we take ZrTe at kz=0 plane as an example)

```
&CONTROL
MirrorChern_calc=T
/
&SYSTEM
NumOccupied = 8 ! Number of occupied Wannier orbitals
/
&PARAMETERS
Nk1 = 101 ! No. of slices for the 1st reciprocal vector
Nk2 = 101 ! No. of slices for the 2st reciprocal vector
/
KPLANE_BULK
0.00 0.00 0.00 ! Original point for 3D k slice k3=0
1.00 0.00 0.00 ! The first vector. Integrate along this direction to get WCC, should be a close path
0.00 1.00 0.00 ! WCC along this direction, for Chern, usually one reciprocal lattice vector
```

### Output#

The mirror Chern number can be found in the WT.out. The WCC/Wilson loop is included in the files
**wcc-mirrorminus.dat** and **wcc-mirrorplus.dat**. The gnuplot script is **wcc-mirrorchernnumber.gnu**. The format of **wcc-mirrorplus.dat** is:

```
# k sum(wcc(:,ik)) wcc(:, ik)
0.00000000 0.93401098 0.26748313 0.33122324 0.37761566 0.95768895
0.01000000 0.93458410 0.26776394 0.33149191 0.37747362 0.95785463
0.02000000 0.93515725 0.26806334 0.33205065 0.37717770 0.95786557
0.03000000 0.93572256 0.26838206 0.33288980 0.37673021 0.95772050
...
```

The first column is k=i/Nk2 (i=0, Nk2), we take the second vector defined in KPLANE_BULK as unit of 1. The second line is the summation of the WCC over all the “occupied/2” bands. It’s usefull for telling the Chern number. From the third column to the last column, they are wcc for the occupied/2 bands specified with “NumOccupied”.

## 2.3.21. Z2 number for 3D bulk materials#

We can get Z2 topological index (v0, v1v2v3) from the z2 calculations of six time reversal invariant planes, i.e. (a) k1=0.0; (b) k1=0.5; (c) k2=0.0; (d) k2=0.5; (e) k3=0.0; (f) k3=0.5; Usually, you can call “Wannier charge center calculation for a plane” six times. Here we packed them up to get another function. You can set the input file like the following.

### Input#

The necessary tags that you should set in the wt.in

```
&CONTROL
Z2_3D_calc = T
/
&PARAMETERS
NumOccpuied = 18 ! No. of occupied wannier bands
Nk1 = 41 ! No. of slices of the k points for WCCs
Nk2 = 41 ! No. of slices of the k points for WCCs
/
```

### Output#

Outputs are **wanniercenter3D_Z2_1.dat, wanniercenter3D_Z2_2.dat, wanniercenter3D_Z2_3.dat, wanniercenter3D_Z2_4.dat, wanniercenter3D_Z2_5.dat, wanniercenter3D_Z2_6.dat**
and **wanniercenter3D_Z2.gnu**. The z2 value can be found in the WT.out by searching “z2 number for 6 planes”.
The WCC (Wilson loop) plots **wanniercenter3D_Z2.eps** can be got with:

```
gnuplot wanniercenter3D_Z2.gnu
```

Note

Important: please set **NumOccpuied** correctly. It represents the “occpuied” wannier bands, not the total number of electrons.
In this application, the Wilson loop is the trace of NumOccupied bands. If you want to study the topology between the 8th and the 9th band,
then set NumOccupied=8.

About the Z2 index for 3D system.

v0= (z2(ki=0)+z2(ki=0.5))mod 2

vi= z2(ki=0.5)

For the 2D system, if you set the Z axis as the stack axis, please only take the Z2 number at k3=0 plane.

## 2.3.22. Chern number for 3D bulk materials#

- Basically, you can calculate the Chern number for a closed manifold, for example, a 2D torus. For this purpose, I would suggest you using
WannierCenter_calc=T in the calculation.

We can get Chern number of six k planes, i.e. k1=0.0; k1=0.5; k2=0.0; k2=0.5; k3=0.0; k3=0.5; where k1, k2, k3 is in fractional units. Usually, you can call “Wannier charge center calculation for a plane” six times. Here we packed them up to get another function. You can set the input file like the following.

Basically, the method used here is very similar to the one used in the Z2 number calculations. We also use the Wilson loop method. However, for Z2 calculation, you only take half of the size of a time reversal invariant slice. For Chern number calculation, you need a closed momentum surface. For example, for the k1=0.0 plane, half of the time reversal invariant slice would be defined like this:

```
k2 is in [0, 0.5]
k3 is in [0, 1]
```

The full closed momentum surface would defined like this

```
k2 is in [0, 1]
k3 is in [0, 1]
```

### Input#

The necessary tags that you should set in the wt.in

```
&CONTROL
Chern_3D_calc = T
/
&PARAMETERS
NumOccpuied = 18 ! No. of occupied wannier bands
Nk1 = 41 ! No. of slices of the k points for WCCs
Nk2 = 41 ! No. of slices of the k points for WCCs
/
```

### Output#

Outputs are **wanniercenter3D_Chern.dat**
and **wanniercenter3D_Chern.gnu**. The Chern number can be found in the WT.out by searching “Chern number for 6 planes”.
The WCC (Wilson loop) plots **wanniercenter3D_Chern.eps** can be got with:

```
gnuplot wanniercenter3D_Chern.gnu
```

Note

Important: please set **NumOccpuied** correctly. It represents the “occpuied” wannier bands, not the total number of electrons.
In this application, the Wilson loop is the trace of NumOccupied bands. If you want to study the topology between the 8th and the 9th band,
then set NumOccupied=8.

For the 2D system, if you set the Z axis as the stack axis, please only take the Chern number at k3=0 plane.

## 2.3.23. Landau level calculations#

**This functionality is under testing, not released yet. Developed by QSWu and YFGuan**

By applying the uniform magnetic field along one lattice vector, the Landau level spectrum can be calculated by the Peierls substitution.

Here we put one example of Graphene. The input file wt.in is like this

```
&TB_FILE
Hrfile = 'wannier90_hr.dat'
/
!> bulk band structure calculation flag
&CONTROL
BulkBand_calc = T
Hof_Butt_calc = T
LandauLevel_k_calc = T
LandauLevel_wavefunction_calc = F
/
&SYSTEM
NSLAB = 200 ! the size of magnetic supercell
NumOccupied = 1 ! NumOccupied
SOC = 0 ! soc
E_FERMI = -1.2533 ! e-fermi
/
&PARAMETERS
E_arc = 0.00 ! energy for calculate Fermi Arc
OmegaNum = 201 ! number of eigenvalues to calculate the Landau levels
Nk1 = 100 ! number k points for each line in the kpath_bulk
/
LATTICE
Angstrom
2.1377110 -1.2342080 0.0000000
0.0000000 2.4684160 0.0000000
0.0000000 0.0000000 10.000000
!> used when you want to study the projections on the orbital for each band
SELECTEDORBITALS
1 ! NumberofSelectedOrbitals without spin degeneracy
1 ! SelectedOrbitals indices without spin degeneracy
ATOM_POSITIONS
2 ! number of atoms for projectors
Direct ! Direct or Cartisen coordinate
C 0.333333 0.666667 0.500000 C
C 0.666667 0.333333 0.500000 C
PROJECTORS
1 1 ! number of projectors
C pz
C pz
SURFACE
0 0 1 ! magnetic field direction in units of lattice vectors
1 0 0
KPATH_BULK ! k point path
1 ! number of k line only for bulk band
M 0.50000 0.00000 0.00000 G 0.00000 0.00000 0.00000
WANNIER_CENTRES
Cartesian
0.712570 1.234209 5.000000
1.425141 -0.000001 5.000000
```

We can calculate the Hofstader butterfly plot by setting **Hof_Butt_calc = T**. **Nslab** is the size of the supercell. The corresponding
magnetic field strength can be found in the output WT.out.

Since the calculation for magnetic supercell is very heavy, we have two versions of eigenvalue solvers. One is direct diagonalization, the other one is the ARPACK solver, which is based on the sparse matrix. So you have to install the ARPACK package, and specify the library in the Makefile. You don’t have to choose the solvers. It is automatically chosen according to the matrix dimensionality. If the dimensionality of the Hamiltonian matrix of the magnetic supercell is larger than 1600, WannierTools will call the sparse matrix solver.

Once the sparse matrix solver is chosen. You have to set **E_arc** and **OmegaNum**, which means you are going to calculate
2*OmegaNum+1 Landau energy levels around **E_arc** respect to the Fermi level.

The magnetic field is along the first vector specified in the SURFACE card.

## 2.3.24. Ordinary magnetoresistance calculations#

After version 2.6.0, WannierTools is able to calculate magnetoresistance of a non-magnetic metal or semimetal which has Fermi surfaces. The theory part was described in Phys. Rev. B 99, 035142 (2019).

With control tag **Boltz_OHE_calc=T** and **Symmetry_Import_calc = T**, we can get the conductivity tensor
for a given magnetic direction specified by **Btheta** and **Bphi**.

Here we put one example of Cu. The input file wt.in is like this

```
&TB_FILE
Hrfile = 'wannier90_hr.dat_nsymm48' ! Here we symmetrized the TB model
/
&CONTROL
Boltz_OHE_calc = T ! calculate ordinary magnetoresistance
Symmetry_Import_calc = T ! please set it to be true for magnetoresistance calculation
/
&SYSTEM
SOC = 0 ! There is no SOC in the hr file : SOC=0; with soc : SOC=1
E_FERMI = 7.7083 ! e-fermi in eV
Btheta= 0, Bphi= 90 ! magnetic field direction, Btheta is the angle with z axial, Bphi is the angle with respect to x axial in the x-y plane
NumOccupied = 6 ! set it anyway even don't use it. Usually, It's the valance band maximum band index.
/
&PARAMETERS
OmegaNum = 1 ! omega number
OmegaMin = 0.0 ! energy interval
OmegaMax = 0.0 ! energy interval chemical potential \mu_i=OmegaMin+ (i-1)/(OmegaNum-1)*(OmegaMax-OmegaMin)
Nk1 =61 ! Kmesh(1) for KCUBE_BULK
Nk2 =61 ! Kmesh(2) for KCUBE_BULK
Nk3 =61 ! Kmesh(3) for KCUBE_BULK
BTauNum= 100 ! Number of B*tau we calculate
BTauMax = 40.0 ! The maximum B*tau, starting from Btau=0.
Tmin = 30 ! Temperature in Kelvin
Tmax = 330 ! Temperature in Kelvin
NumT = 11 ! number temperature we calculate. T_i=Tmin+(Tmax-Tmin)/(NumT-1)*(i-1)
/
LATTICE
Angstrom ! Unit of length: Angstrom or Bohr
0.0000000 1.8075000 1.8075000
1.8075000 0.0000000 1.8075000
1.8075000 1.8075000 0.0000000
ATOM_POSITIONS
1 ! number of atoms for projectors
Cartisen ! Direct or Cartisen coordinate
Cu 0.000000 0.000000 0.000000
PROJECTORS
9 ! number of projectors
Cu s pz px py dz2 dxz dyz dx2-y2 dxy
SELECTEDBANDS
1
6 ! the 6'th band is crossing the Fermi level.
KCUBE_BULK ! in unit of primitive reciprocal lattice vectors.
0.00 0.00 0.00 ! Original point for 3D k plane
1.00 0.00 0.00 ! The first vector to define 3d k space plane
0.00 1.00 0.00 ! The second vector to define 3d k space plane
0.00 0.00 1.00 ! The third vector to define 3d k cube
```

The above input file indicates that 1). The magnetic field is along z direction (Btheta=0). 2). The chemical potential is set to Zero. by OmegaNum=1; OmegaMin=Omegamax=0. 3). The temperature is set as an arrary from 30K to 330K with 30 as interval by Tmin=30; Tmax=330; NumT=11. 4). The magnetic field strenth is set as B*tau= (0, 40) with 100 points by BTauMax=40; BTauNum=100. 5). The k-mesh is set as 61*61*61.

On output, the conductivity tensor sigma/tau as a function of B*Tau for each band n, each chemical potential mu and each temperature T are presented in file sigma_band_${n}_mu_${mu}eV_T_${T}K.dat

If there are serveral band, you should write a script to add up all the conductivity tensor for all the bands, then take an inverse of it to get the resistivity tensor.

On output, there are also resistivity tensor files for each band, each chemical potential and each temperature. It’s usfull to get general information for each band.

For more illustration of example Cu, you can visit https://www.wanniertools.org/examples/ordinary-magnetoresistance-of-cu/

Note

If you obtained negative magnetoresistance at large Btau, then please increase NSlice_Btau_Max such that the negative magnetoresistance vanishes. The Lorentz force will only give us positive magnetoresistance.