27.12.2014 Views

Problem Set 9 Solutions

Problem Set 9 Solutions

Problem Set 9 Solutions

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

5<br />

4. a.) Continued<br />

0.6<br />

0.5<br />

G1(x)<br />

G2(x)<br />

G3(x)<br />

0.4<br />

G(x)<br />

0.3<br />

0.2<br />

0.1<br />

0<br />

0 1 2 3 4<br />

x (angstroms)<br />

b.) Plot the atomic orbital f (r) as a function of x.<br />

orbital s(r) with the form<br />

Compare this to a Slater type atomic<br />

€<br />

€<br />

s(r) = ζ 3 1/ 2<br />

⎛⎛ ⎞⎞<br />

⎜⎜<br />

⎜⎜<br />

⎟⎟<br />

⎝⎝ π ⎟⎟ e −ζ r ,<br />

⎠⎠<br />

with the orbital exponent ζ set to 1.<br />

€<br />

The functions are plotted below. Note that the only significant difference is near the origin, where the<br />

Slater type orbital has € a cusp.<br />

0.6<br />

0.5<br />

s(x)<br />

f(x)<br />

0.4<br />

s(x), f(x)<br />

0.3<br />

0.2<br />

0.1<br />

0<br />

0 1 2 3 4<br />

x (angstroms)

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!