Last Modified 17 December 1999

The ``Static'' Tight-Binding Program: Example IX

Constructing the Density of States (DOS)

On the previous page we used static to produce a QLMT file to be used to construct a Density of States for hcp Ruthenium. This page shows how to convert this particular QLMT file into an approximate electronic density of states.

There are accurate ways to construct the DOS, most notably the tetrahedron method, and then there is my way. My way uses the program qdos.f, which produces a ``quick and dirty'' DOS using the implicit formula for the DOS defined by our method of doing eigenvalue-energy sums. A somewhat more detailed explanation of this is contained in the comments within the source code.

Compile qdos.f and place the executable somewhere in your path. Then go to your working directory and run the code.

$ ./qdos 0.005 -0.389 0.500 0.0002 < QLMT > dos_0.0050

Let's take a quick look at the output file dos_0.0050. The first few lines look like this:

     -.38900      .00067      .10740  1.3784E+01     -.00026
     -.38880      .00069      .11017  1.3964E+01     -.00026
     -.38860      .00072      .11298  1.4140E+01     -.00027
     -.38840      .00074      .11583  1.4309E+01     -.00028
     -.38820      .00076      .11871  1.4473E+01     -.00029
     -.38800      .00079      .12162  1.4631E+01     -.00030
     -.38780      .00081      .12456  1.4783E+01     -.00031
     -.38760      .00084      .12753  1.4928E+01     -.00032
     -.38740      .00086      .13053  1.5067E+01     -.00033
     -.38720      .00089      .13355  1.5199E+01     -.00034

On each line,

We can now plot out the DOS for Ruthenium using a gnuplot script:

DOS of TB Ru at T = 5 mRy

We can compare this result with the First-principles calculation from NRL's Electronic Structures Database:

First principles DOS of Ru

Aside from the arbitrary shift in energy, these curves are in pretty close agreement.

Temperature Dependence of the DOS

We'll now consider the behavior of the DOS as a function of the Fermi temperature used in Gillan's method. We can guess that if the temperature is too small the DOS plot will degenerate into a series of spikes, and we'll have to have a very fine grid to see them at all. On the other hand, when the temperature is too large everything gets smeared out.

The following script calculates the DOS at every temperature on its command line, assuming the temperatures are in Rydbergs:

#!/bin/sh
for temp
do
./qdos $temp -0.389 0.5001 0.0005 < QLMT > dos_$temp
done

We'll run this for a few representative temperatures:

tscript 0.0010 0.0025 0.0100

and plot them and our original data using this script:

Temperature Dependent DOS of Ru

Our predictions are correct, but over the rather broad range 1 mRy<T<10 mRy this ``Quick and Dirty'' DOS remains fairly consistent.


Now back to the DOS setup page.

Look at other examples.

Get other parameters from the Tight-binding periodic table.


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