| Differences between revisions 2 and 23 (spanning 21 versions) | Back to page |
|
Size: 84
Comment:
|
Size: 2919
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 1: | Line 1: |
| [[ Matlab and Python | Here is some base-line discussion for Matlab and Python. ]] | === Here is some discussion of the programming part of Homework #4. === [[ Matlab and Python | First, here is some base-line discussion for Matlab and Python that you might find useful]]. Please read it, or at least run a quick scan through it. Now, for this homework, you basically need to calculate some functions and plot up the results. Example 2.3 of the textbook is a pretty good "template" for this task, and so I will discuss that example here. '''Here is the Matlab code for Example 2.3.''' This code is somewhat different from the code in the text book, but does the same thing. {{{#!highlight matlab %E2.3: Fermi Function Calculation, f(E-EF,T) %Initialization clear close %Constant %25.85 meV for 300 K is an equivalent way to remember it. k=8.617e-5; %Google for "Matlab linspace", to find out what linspace does! dE=linspace(-0.2,0.2); for ii=1:4; T=100*ii; kT=k*T; f(ii,:)=1./(1+exp(dE./kT)); end %Plotting result close plot(dE,f); grid; xlabel('E - E_F (eV)'); ylabel('f (E)'); text(.05,.22,'T=400K'); text(-.03,.12,'T=100K'); %Comment these out for batch mode %print -djpeg E2p3.jpg %print -depsc E2p3.eps %print -dpng E2p3.png %exit }}} The obtained images by Matlab and Octave are as follows (click to see full images). <<lia(E2.3.jpg)>> <<lia(E2.3.oct.jpg)>> To run the above code with Matlab in batch mode (after commenting out at least one of the print lines): {{{ matlab -nosplash -nodesktop -minimize -r E2p3 }}} To run the above code with Octave in batch mode (after commenting out at least one of the print lines): {{{ octave E2p3.m }}} Of course, for this command to run successfully, octave must be in the path (which is ''not'' the case by default for Windows installation! -- I had to add the Octave bin directory to path manually!), and E2p3.m must be the file name for the above code. '''Here is the Python code for Example 2.3.''' {{{#!highlight python # E2.3: Fermi Function Calculation, f(E-EF,T) # pylab is part of matplotlib, a matlab like environment in python. # http://matplotlib.sourceforge.net/index.html # Lots of names are imported by this (numpy, scipy, matplotlib, I think). from pylab import * # 25.85 meV for 300 K is an equivalent way to remember it. k = 8.617e-5 # linspace defaults to 50 points -- I want 100 (like in matlab). dE = linspace (-0.2, 0.2, 100) Ts = [100, 200, 300, 400] for T in Ts: plot (dE, 1./(1 + exp (dE / (k * T)))) grid () # matplotlib comes with its own LaTeX parser -- cool! xlabel (r'E - E$_\mathrm{F}$ (eV)') ylabel ('f (E)') text (.05,.22,'T=400K') text (-.04,.12,'T=100K') # after showing, it is possible to save the plot as an image. show () }}} You should get an image like this (click to see the full image), when you save the image from the interactive window that pops up on "show ()". <<lia(E2.3.png)>> |
Here is some discussion of the programming part of Homework #4.
First, here is some base-line discussion for Matlab and Python that you might find useful. Please read it, or at least run a quick scan through it.
Now, for this homework, you basically need to calculate some functions and plot up the results. Example 2.3 of the textbook is a pretty good "template" for this task, and so I will discuss that example here.
Here is the Matlab code for Example 2.3. This code is somewhat different from the code in the text book, but does the same thing.
%E2.3: Fermi Function Calculation, f(E-EF,T)
%Initialization
clear
close
%Constant
%25.85 meV for 300 K is an equivalent way to remember it.
k=8.617e-5;
%Google for "Matlab linspace", to find out what linspace does!
dE=linspace(-0.2,0.2);
for ii=1:4;
T=100*ii;
kT=k*T;
f(ii,:)=1./(1+exp(dE./kT));
end
%Plotting result
close
plot(dE,f); grid;
xlabel('E - E_F (eV)'); ylabel('f (E)');
text(.05,.22,'T=400K'); text(-.03,.12,'T=100K');
%Comment these out for batch mode
%print -djpeg E2p3.jpg
%print -depsc E2p3.eps
%print -dpng E2p3.png
%exit
The obtained images by Matlab and Octave are as follows (click to see full images).
To run the above code with Matlab in batch mode (after commenting out at least one of the print lines):
matlab -nosplash -nodesktop -minimize -r E2p3
To run the above code with Octave in batch mode (after commenting out at least one of the print lines):
octave E2p3.m
Of course, for this command to run successfully, octave must be in the path (which is not the case by default for Windows installation! -- I had to add the Octave bin directory to path manually!), and E2p3.m must be the file name for the above code.
Here is the Python code for Example 2.3.
# E2.3: Fermi Function Calculation, f(E-EF,T)
# pylab is part of matplotlib, a matlab like environment in python.
# http://matplotlib.sourceforge.net/index.html
# Lots of names are imported by this (numpy, scipy, matplotlib, I think).
from pylab import *
# 25.85 meV for 300 K is an equivalent way to remember it.
k = 8.617e-5
# linspace defaults to 50 points -- I want 100 (like in matlab).
dE = linspace (-0.2, 0.2, 100)
Ts = [100, 200, 300, 400]
for T in Ts:
plot (dE, 1./(1 + exp (dE / (k * T))))
grid ()
# matplotlib comes with its own LaTeX parser -- cool!
xlabel (r'E - E$_\mathrm{F}$ (eV)')
ylabel ('f (E)')
text (.05,.22,'T=400K')
text (-.04,.12,'T=100K')
# after showing, it is possible to save the plot as an image.
show ()
You should get an image like this (click to see the full image), when you save the image from the interactive window that pops up on "show ()".


