Variance of a harmonic motion particle

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Homework Help Overview

The discussion revolves around a particle in a harmonic potential, specifically analyzing its energy eigenvalues, wave functions, and properties such as variance. Participants explore classical motion limits, probability integrals, and the calculation of variance in quantum mechanics.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants discuss the classical turning points for a particle in a harmonic potential and the implications of the wave function on probability calculations. There are attempts to compute the variance and clarify the use of integrals related to the wave function.

Discussion Status

Some participants have provided corrections regarding the wave function and its properties, while others are exploring the implications of these corrections on the calculations of expectation values. There is ongoing exploration of integral techniques and their applications to the problem.

Contextual Notes

Participants are working within the constraints of homework rules, which may limit the information they can share. There is a focus on ensuring the accuracy of the wave function and its implications for the calculations being performed.

TFM
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Homework Statement



Consider a particle in the harmonic potential [tex]V(x)= \frac{m\omega^2 x^2}{2}[/tex]. Its lowest energy eigenvalue is [tex]E_0=\hbar \omega/2[/tex] and the eigenfunction associated with this energy, ie the ground-state wave function, is

[tex]\phi_0(x) = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{(m\omega/2\hbar)x^2}[/tex]


a)

Determine the limits of the classical motion in this potential (the “classical turning points”), ie the smallest and the largest values of x that a classical particle can reach if it has the total energy E0.

b)

Assume that the wave function of the particle is the stationary state [tex]\phi_0(x) = e^{-iE_0t/\hbar}[/tex]. Determine the probability (in the form of an integral) of finding the particle outside the region where classical motion can occur. By making an appropriate change of variable in the integral you obtain, show that the answer is independent of m, [tex]\omega[/tex], and [tex]\hbar[/tex].

c)

Calculate the variance [tex]\Delta \hat{x}[/tex] in the ground-state of the system and compare it to the limits of the classical motion.

useful integral:

[tex]\int^{\infty}_{-\infty} z^2 e^{-\alpha z^2} dz = \frac{1}{2}\sqrt{\frac{\pi}{a^3}}[/tex]


Homework Equations



Variance = [tex]\sqrt{<x^2> - <x>^2}[/tex]

[tex]<x^2> = \int \phi^* x^2 \phi[/tex]

[tex]<x> = \int \phi^* x \phi[/tex]

The Attempt at a Solution



I have done all but the location of reflection for (a), and I have done (b), but I am slightly stuck for (c)

I have used the formulas given above, with:

[tex]\phi_0(x) = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{(m\omega/2\hbar)x^2}[/tex]


[tex]\phi_0(x)^* = \left(\frac{m^*\omega^*}{\pi \hbar^*}\right)^{1/4}e^{-(m\omega/2\hbar)x^2}[/tex]

however when I put them in the variance formula, because it is e^x x e^-x, they cancel,so I am just left with:

[tex]<x> = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}\left(\frac{m^*\omega^*}{\pi \hbar^*}\right)^{1/4}x[/tex]

and

[tex]<x^2> = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}\left(\frac{m^*\omega^*}{\pi \hbar^*}\right)^{1/4}x^2[/tex]

This doesn't seem to coincide with the useful integer given...?

Have I gone wrong somewhere?

Many Thanks,

TFM
 
Last edited:
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first of all, the wavefunction does not seem to be correct.

http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/hosc5.html

so your suggestion:
[tex] \phi_0(x) = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{(m\omega/2\hbar)x^2} [/tex]
is wrong, it should be;
[tex] \phi_0(x) = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{-(m\omega/2\hbar)x^2} [/tex]

And now taking the complex conjugate of this one.. can you please tell me what the complex conjugate of a real number is? Then can you tell me if the ground state function is a real function?! ;-)
 
The complex conjugate of a real number is just the real number.

there is no i's, so it is real...

this means

[tex]\phi_0(x) = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{-(m\omega/2\hbar)x^2}[/tex]

and

[tex]\phi_0(x)^* = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{-(m\omega/2\hbar)x^2}[/tex]

so:


[tex]<x> = \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{-(m\omega/2\hbar)x^2}\left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{-(m\omega/2\hbar)x^2} x[/tex]

giving:

[tex]<x> = \int^{\infty}_{infty}\left(\frac{m\omega}{\pi \hbar}\right)^{1/2}e^{-2(m\omega/2\hbar)x^2} x dx[/tex]

this looks lot better, but how would you use the integral

[tex]\int^{\infty}_{-\infty} z^2 e^{-\alpha z^2} dz = \frac{1}{2}\sqrt{\frac{\pi}{a^3}}[/tex]

for this one to solve? Would you use a substitiution?
 
no for this integral you only need to do x^2 = y, and take y as integration variable.

Haven't you done calculus? :S
 
Okay, so

[tex]<x> = \int^{\infty}_{infty}\left(\frac{m\omega}{\pi \hbar}\right)^{1/2}e^{-2(m\omega/2\hbar)x^2} x dx[/tex]

take constants outside of integral

[tex]<x> = \left(\frac{m\omega}{\pi \hbar}\right)^{1/2}\int^{\infty}_{infty}xe^{-2(m\omega/2\hbar)x^2} dx[/tex]

make

2(m\omega/2\hbar a constant, \alpha

[tex]<x> = \left(\frac{m\omega}{\pi \hbar}\right)^{1/2}\int^{\infty}_{infty}xe^{-\alpha x^2} dx[/tex]

[tex]x^2 = y, x = \sqrt{y}[/tex]

[tex]<x> = \left(\frac{m\omega}{\pi \hbar}\right)^{1/2}\int^{\infty}_{infty}\sqrt{y}e^{-\alpha y} dy[/tex]

use integration by parts:

[tex]\int^{\infty}_{infty}\sqrt{y}e^{-\alpha y} dy[/tex]

f(x) g'(x) = f(x)g(x) - \int{f'(x) g(x)}

f(x) = e^-ax
g'(x) = y

f'(x) = -(1/a)e^-ax
g(x) = 1

[tex]f(x) g'(x) = e^{-ax}1 - \int{-(1/a)e^-ax 1}[/tex]

[tex]f(x) g'(x) = e^{-ax} - \int{-(1/a)e^-ax}[/tex]

[tex]f(x) g'(x) = e^{-ax} - e^-ax}[/tex]

[tex]f(x) g'(x) = e^{-ax} - e^-ax} = 0[/tex]

Does this look right?
 
no!

if x^2 = y, then xdx = (1/2)dy !

Now I can give you one more approach, what is the integral over an odd function over an even interval? (can you use that in this situation?)
 
what is the integral over an odd function over an even interval? (can you use that in this situation?)

0

Also,

[tex]= \left(\frac{m\omega}{\pi \hbar}\right)^{1/2}\int^{\infty}_{infty}xe^{-\alpha x^2} dx[/tex]

using the substitution, gives:

[tex]\int^{\infty}_{infty}e^{-\alpha y} \frac{1}{2}dy[/tex]

which is:

[tex]\frac{1}{2}\left[-\frac{1}{\alpha}e^{-\alpha y}\right]^{\infty}_{infty}[/tex]

which is 0 from infinty to -infinty
 
Last edited:
yes, good!
but you can also see that it is 0 from the fact that xe^(-x^2) is an odd function.

Ok, let's do the x^2e^(-x^2) integral using that integral relation which was given to you.
 
Okay, so:

[tex]<x^2> = \int \phi^* x^2 \phi[/tex]

insert phi and phi*:


[tex]<x^2> = \int \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{(m\omega/2\hbar)x^2} x^2 \left(\frac{m\omega}{\pi \hbar}\right)^{1/4}e^{(m\omega/2\hbar)x^2}[/tex]

giving:

[tex]<x^2> = \int \left(\frac{m\omega}{\pi \hbar}\right)^{1/2}e^{-(m\omega/\hbar)x^2} x^2[/tex]

take out constants:


[tex]<x^2> = \left(\frac{m\omega}{\pi \hbar}\right)^{1/2} \int^{\infty}_{-\infty} e^{-(m\omega/\hbar)x^2} x^2[/tex]

use:

[tex]\alpha = \frac{m\omega}{\hbar}[/tex]

[tex]<x^2> = \left(\frac{\alpha}{\pi} \right)^{1/2} \int^{\infty}_{-\infty} e^{-\alpha x^2} x^2[/tex]

use given integral:

[tex]<x^2> = \left(\frac{\alpha}{\pi} \right)^{1/2} \left[ \frac{1}{2}\sqrt{\frac{\pi}{\alpha}}\right][/tex]

insert alpha:

[tex]<x^2> = \left(\frac{m\omega}{\hbar\pi} \right)^{1/2} \left[ \frac{1}{2}\sqrt{\frac{\pi}{\frac{m\omega}{\hbar}}}\right][/tex]

okay so far?
 
  • #10
no check the identity again

[tex] = \left(\frac{\alpha}{\pi} \right)^{1/2} \left[ \frac{1}{2}\sqrt{\frac{\pi}{\alpha}}\right] [/tex]

is wrong, it should be:

[tex] = \left(\frac{\alpha}{\pi} \right)^{1/2} \left[ \frac{1}{2}\sqrt{\frac{\pi}{\alpha ^3}}\right] [/tex]

Slow down, don't hurry
 
  • #11
Okay so:

[tex]= \left(\frac{m\omega}{\hbar\pi} \right)^{1/2} \left[ \frac{1}{2}\sqrt{\frac{\pi}{\left(\frac{m\omega}{\hbar}\right)^{3}} }\right] [/tex]
 
  • #12
simplify
 
  • #13
Okay,

[tex]= \left(\frac{m\omega}{\hbar\pi} \right)^{1/2} \left[ \frac{1}{2}\sqrt{\frac{\pi}{\left(\frac{m\omega}{\ hbar}\right)^{3}} }\right][/tex]


[tex]= \frac{1}{2}\sqrt{\frac{\frac{m\omega}{\hbar\pi}\pi}{\left(\frac{m\omega}{\hbar}\right)^{3}}[/tex]

[tex]= \frac{1}{2}\sqrt{\frac{\frac{m\omega}{\hbar}}{\left(\frac{m\omega}{\hbar}\right)^{3}}[/tex]


[tex]= \frac{1}{2}\sqrt{\frac{1}{\left(\frac{m\omega}{\hbar}\right)^{2}}[/tex]

Would this go to:

[tex]= \frac{1}{2}\sqrt{\left(\frac{\hbar}{m\omega}\right)^{2}[/tex]

?
 
  • #14
what is square root of quadratic?
 
  • #15
well x^2 square rooted is, so:

[tex]\frac{1}{2}\sqrt{\left(\frac{\hbar}{m\omega}\right )^{2}[/tex]

can cancel to:

[tex]\frac{\hbar}{2m\omega}[/tex]
 
  • #16
Okay, so now, if I put this into the variance:

[tex]\Delta \bar{x} = \sqrt{<x^2> - <x>^2}[/tex]

[tex]\Delta \bar{x} = \sqrt{\frac{\hbar}{2m\omega} - 0^2}[/tex]

[tex]\Delta \bar{x} = \sqrt{\frac{\hbar}{2m\omega}}[/tex]

Which is very similar to the limits of the classical motion, which were

[tex]\sqrt{\frac{\hbar}{m\omega}}[/tex]
 

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