Fermi surface

The Fermi surface is visualized by XCrySDen [66]. When you perform calculations of the density of states by the following keywords:

  Dos.fileout                  on        # on|off, default=off
  Dos.Erange              -20.0  20.0    # default = -20 20 
  Dos.Kgrid                 61 61 61     # default = Kgrid1 Kgrid2 Kgrid3
you will obtain a file 'System.Name.FermiSurf0.bxsf', where 'System.Name' is 'System.Name', and the file can be visualized by XCrySDen [66]. As well as 'Dos.Fileout', 'DosGauss.fileout' can be also used for the purpose. In case of spin-polarized calculations, two files are generated as 'System.Name.FermiSurf0.bxs' and 'System.Name.FermiSurf1.bxs' for spin-up and spin-down states, respectively. In case of non-collinear calculations, a file 'System.Name.FermiSurf.bxs' is generated. It is noted that a large number of k-points should be used in order to obtain a smooth Fermi surface. As an example, Fermi surfaces of the fcc Ca bulk are shown in Fig. 54. The input file used for the calculation is 'Cafcc_FS.dat' in the directory 'work'.

Figure 54: Fermi surfaces of the fcc Ca bulk visualized by XCrySDen [66]. Since two sorts of bands intersect with the Fermi energy (chemical potential), two Fermi surfaces are shown in (a) and (b). The input file used for the calculation is 'Cafcc_FS.dat' in the directory 'work'.
\begin{figure}\begin{center}
\epsfig{file=FermiSurface.eps,width=16.0cm}
\end{center}
\end{figure}

2016-04-03