Perturbation of a 3-dimensional infinite cubical well
Karl Patrick S. Casas
Consider a three-dimensional infinite cubical well


The stationary states are

and the allowed ground state energy is given by

.
The first excited state is triply degenerate,

and we denote each degenerate state as

Now, we introduce the perturbation
(shown in the figure above),

We can get the first-order correction to the ground state energy by


Using the integral formula,
.
And so, solving each integral,
![\int_0^{a/2}\sin^2\left(\frac{\pi}{a}x\right)dx=\left[\frac{x}{2}-\frac{\sin2\pi x/a}{4\pi/a}\right]_0^{a/2}=\frac{x}{2}\left|_0^{a/2}=\frac{a}{4}](http://www.quantumsciencephilippines.com/wp-content/uploads/eq_39cebb17fd5390c891fb347d30cf71eb.png)
![\int_{a/2}^{a}\sin^2\left(\frac{\pi}{a}y\right)dy=\left[\frac{y}{2}-\frac{\sin2\pi y/a}{4\pi/a}\right]_{a/2}^a=\frac{y}{2}\left|_{a/2}^a=\frac{a}{4}](http://www.quantumsciencephilippines.com/wp-content/uploads/eq_4dac18cd77f21efd54ec4ab56b5207d6.png)
![\int_0^{a}\sin^2\left(\frac{\pi}{a}z\right)dz=\left[\frac{z}{2}-\frac{\sin2\pi z/a}{4\pi/a}\right]_0^{a}=\frac{z}{2}\left|_0^{a}=\frac{a}{2}](http://www.quantumsciencephilippines.com/wp-content/uploads/eq_7ca3de357bb1efd61dcfcdff1a9ff629.png)
Thus,
.
To solve for the eigenvalue
, we consider the components of

where we can then solve the corresponding eigenvalue equation,


Solving for the components,


we already have the first and second integral. Now, consider the z-part
![\int_0^a\sin^2(2\pi z/a )dz=\left[\frac{z}{2}-\frac{\sin2\left(2\pi/a\right)z}{4\left(2\pi/a\right)}\right]_0^a=\frac{z}{2}\left|_0^a=\frac{a}{2}](http://www.quantumsciencephilippines.com/wp-content/uploads/eq_170844710c3e2f1d24ffdefb1a1e1da4.png)
hence,

Now,


solving the y-integral

.
So,
.
And then,

.
Considering the x-part,
![\int_{a/2}^{a}\sin^2\left(\frac{2\pi}{a}x\right)dx=\frac{x}{2}-\frac{\sin2\left(2\pi/a\right)x}{4\left(2\pi/a\right)}\left]_0^a=\frac{x}{2}\left|_{a/2}^a =\frac{a}{2}-\frac{a}{4}=\frac{a}{4}](http://www.quantumsciencephilippines.com/wp-content/uploads/eq_366242dd2d97ec0406f225689818c34a.png)
Thus,

Next,


Here, it’s different from the previous. So we use the following integral,

Solving for the y- and z- integrals,




Hence,

Moving on,


We have seen in the previous section that the z-part is zero, and so

Lastly,


Solving for the x-integral,


Therefore,

,
where 
Finally,

We can now solve for the characteristic equation given by

![= \left(\frac{V_0}{4}-\lambda\right)\left[\left(\frac{V_0}{4}-\lambda\right)^2-\left(-\kappa\frac{V_0}{4}\right)^2\right]=0](http://www.quantumsciencephilippines.com/wp-content/uploads/eq_8d2e8f83cec041fd4a64a29db01e4be3.png)



Therefore,

This result is exactly the same as in the sample problem related to this given in Grifftihs “Introduction to quantum mechanics”.
About the author: Karl Patrick S. Casas is a masters student of Mindanao State University-Iligan Institute of Technology. He hopes to finish his degree as soon as possible.


























