Infinite square well centered at the origin

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Homework Help Overview

The problem involves solving the time-independent Schrödinger Equation for an infinite square well centered at the origin. The original poster seeks to demonstrate that the energy levels remain consistent with those of a well defined between x=0 and x=L, and to derive the wave function solutions based on boundary conditions.

Discussion Character

  • Exploratory, Assumption checking, Problem interpretation

Approaches and Questions Raised

  • Participants discuss the implications of boundary conditions on the constants A and B in the wave function. Questions arise regarding the assumptions made about these constants and the conditions under which they can be zero. There is exploration of the consequences of different values of k and their relation to energy levels.

Discussion Status

The discussion is ongoing, with participants exploring various interpretations of the constants in the wave function and their normalization. Some guidance has been offered regarding the relationship between the constants and the boundary conditions, but no consensus has been reached on the final form of the wave function.

Contextual Notes

Participants note the need for normalization of the wave function and the implications of the boundary conditions on the values of A and B. There is an acknowledgment of the original poster's struggle with the problem and a suggestion to persist despite the challenges faced.

  • #31
I probably shoudn't do this, because it might confuse the issue ... but, here is another way to do this problem assuming the solution for a well from ##x=0## to ##x=L## is known. Use translation of functions, i.e., stuff like ##g\left(x\right) = f\left(x-a\right)## and ##h\left(x\right) = f\left(x+a\right)##.
 
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  • #32
That's great. Then you can also show that this of course doesn't change anything concerning the physics, since it's just a different choice of where you set the 0 point of your (spatial) reference frame. This "change of description" is formally given by a corresponding unitary transformation (a translation, which is a fundamental symmetry of Galilean spacetime), and thus indeed nothing is changed physicswise, just our description has changed :-).
 
  • #33
George Jones said:
I probably shoudn't do this, because it might confuse the issue ... but, here is another way to do this problem assuming the solution for a well from ##x=0## to ##x=L## is known. Use translation of functions, i.e., stuff like ##g\left(x\right) = f\left(x-a\right)## and ##h\left(x\right) = f\left(x+a\right)##.
This sounds interesting! Can you please elaborate how to get the solution of centered well from the normal one?

Exactly where do I substitute these new limits?
 
  • #34
Kaguro said:
This sounds interesting! Can you please elaborate how to get the solution of centered well from the normal one?

Exactly where do I substitute these new limits?

Sometimes the square well is taken to be from ##0## to ##L## and in this case the solution comes out slightly more easily than it does in the cases of ##-L/2## to ##L/2##.

Since you now have the solution for a well from ##-L/2## to ##L/2##, you can get the solutions for a well from ##0## to ##L## using a change of coordinates.

Can you see how to do that?
 
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  • #35
PeroK said:
Sometimes the square well is taken to be from ##0## to ##L## and in this case the solution comes out slightly more easily than it does in the cases of ##-L/2## to ##L/2##.

Since you now have the solution for a well from ##-L/2## to ##L/2##, you can get the solutions for a well from ##0## to ##L## using a change of coordinates.

Can you see how to do that?
I have ##\psi= \sqrt{\frac{2}{L}} cos(n\pi x/L) ## if n is odd and
##\psi= \sqrt{\frac{2}{L}} sin(n\pi x/L) ## if n is even

To get solution for well from 0 to L ,I should make the transformation x ##\to ## x+L/2

There for odd n:
##\psi= \sqrt{\frac{2}{L}} cos(n\pi (x+L/2)/L) ##
##= \sqrt{\frac{2}{L}} cos(n\pi x/L)cos(n\pi /2) - sin(n\pi x/L)sin(n\pi /2) ##
##=-\sqrt{\frac{2}{L}}sin(n\pi x/L) ##

For even n:
##\psi= \sqrt{\frac{2}{L}} sin(n\pi (x+L/2)/L) ##
##= \sqrt{\frac{2}{L}} (sin(n\pi x/L)cos(n\pi /2) + cos(n\pi x/L)sin(n\pi /2) )##
##= \sqrt{\frac{2}{L}}(-1)^{n/2} sin(n\pi x/L)##

How to combine them?
 
  • #36
Kaguro said:
To get solution for well from 0 to L ,I should make the transformation x →\to x+L/2

You must be careful with this technique. Which ##x## is which?

In fact, you ended up with them the wrong way round. Instead, try:

##x' = x + L/2##

Where ##x'## is the new variable that runs from ##0## to ##L##.

(Note that this means that ##x = x' - L/2##. Which is not what you did.)
 
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  • #37
Also note that phase factors don't play any role. Defining the system to live in ##[0,L]## the boundary value at ##x=0## tells you ##\psi(0)=0##, which leads to the ansatz ##\psi(x)=A \sin(k x)## for the energy eigenfunctions, then the other boundary condition tells you
$$\psi(L)=A \sin(k L)=0,$$
from which you get ##k \in \pi \mathbb{N}/L##. Thus the complete set of eigenfunctions is
$$\psi_n(L)=A \sin \left(\frac{n \pi x}{L} \right).$$
The factors ##(-1)^j## are phase factors which you can simply neglect, because they have no physical significance.
 
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  • #38
vanhees71 said:
The factors (−1)j(-1)^j are phase factors which you can simply neglect, because they have no physical significance.
Yes, after understanding that x = x' - L/2 will be the correct transformation, I tried it again and got everything correct except this ##(-1)^{n/2}##. Now if you say that it carries no significance and can be neglected, I have arrived at the correct answer! Thank you!
 
  • #39
Kaguro said:
Yes, after understanding that x = x' - L/2 will be the correct transformation, I tried it again and got everything correct except this ##(-1)^{n/2}##. Now if you say that it carries no significance and can be neglected, I have arrived at the correct answer! Thank you!
To explain this a bit more.

What you got was a specific case of:

##\psi(x') = \alpha_n \sqrt{\frac{L}{2}} \sin (\frac{n\pi x'}{L})##

Where ##\alpha_n## is a complex number of unit modulus (sometimes called the phase factor). In this case, you had ##\alpha_n = \pm 1##, depending on ##n##.

This is perfectly valid for a set of eigenfunctions. But, you are free to choose the phase factor to be simply ##1## in each case. Hence, you have the simplest set of solutions:

##\psi(x') = \sqrt{\frac{L}{2}} \sin (\frac{n\pi x'}{L})##:

Note that can always do the opposite as well, and add any phase factors you want. For example, we could take your original solution:

Kaguro said:
##\psi (x) =\begin{cases} \sqrt{ \frac{2}{L}}cos(n\pi x/L) & \text{if n is odd} \\ \sqrt{ \frac{2}{L}}sin(n\pi x/L) & \text{if n is even} \end{cases} ##

And, we could replace this with an alternative, equally valid set of eigenfunctions:

##\psi (x) =\begin{cases} i\sqrt{ \frac{2}{L}}cos(n\pi x/L) & \text{if n is odd} \\ (e^{i\theta_n})\sqrt{ \frac{2}{L}}sin(n\pi x/L) & \text{if n is even} \end{cases} ##

This has all the same properties as your original solution. The only different is that we've added a phase factor to every function.

This is an important point, because when you have a set of eigenfunctions it can be very useful to choose a phase factor in a particular way. Often that some arbitrary complex number is real.

In any case, the point to remember is that you did not find the only possible unique set of solutions. You found a set of solutions, unique only up to the phase factor. You are free, therefore, to simplify or complicate your solution by changing the phase factors any way you like.
 
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  • #40
Thanks to you guys I was having exactly same doubt.
 

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