Solving Ground State of Hydrogen Atom QM Problem

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Homework Help Overview

The discussion revolves around the calculations related to the ground state wavefunction of the hydrogen atom in quantum mechanics. Participants are examining the properties of the wavefunction, particularly its real nature and implications for probability calculations.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the nature of the wavefunction, questioning why it lacks a complex component and how this affects calculations of expectation values and probabilities. There are attempts to evaluate integrals related to the probability of finding the electron in specific regions, with some participants suggesting the need for volume integration in three dimensions.

Discussion Status

The discussion is active, with participants providing insights and corrections regarding the integration process and the nature of the wavefunction. Some participants express confusion over the proper setup of integrals and the implications of using a real wavefunction. There is a recognition of the need to consider volume elements in spherical coordinates, and while some participants are clarifying concepts, there is no explicit consensus on the calculations being discussed.

Contextual Notes

Participants are grappling with the definitions and calculations of probabilities in quantum mechanics, particularly in the context of the hydrogen atom. There are mentions of homework constraints and the challenge of integrating over three-dimensional space, which adds complexity to the problem.

  • #31
It should be -sin \theta.du since the derivative of cos is -sine. Right? Thats what I was trying to right, but I didn't account for the other sine. So should it be sin^2 instead of sine in the above integral? And can I treat this as a constant when integrating wrt u. If not I'm unsure how to proceed since I'll have two variables then?
 
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  • #32
If du = - \sin{\theta} d\theta then you have precisely du in the bottom of your integral already, right? I'm not sure where you are getting this \sin^2{\theta} idea from. The whole point of the substitution is that you transform one seemingly complicated integral over \theta into something like a simple exponential integral in terms of u.
 
  • #33
Sorry my brain burped. :blushing: Integratiuon by substitution is probably my weakest point in calculus.

Anyway, let me show you how it is as I get it, and maybe you can let me know where I'm going wrong.

The tricky theta integral is

\int^\pi_0 {e^(\frac{-ipCos\theta}{\hbar})Sin\theta}.d\theta

If we make the substitution z = Cos\theta

Then \frac{dz}{d\theta} = -Sin\theta

Now as I understand the integration by substitution process, we need to sub d\theta in terms of dz i.e

d\theta = \frac{-dz}{Sin\theta}

This makes our integral.

\int^\pi_0 {e^(\frac{-ip.z}{\hbar})Sin\theta}.\frac{dz}{Sin\theta}

Now would the Sine terms cancel leaving?

\int^\pi_0 {e^(\frac{-ip.z}{\hbar})dz

Which I can integrate, but not 100% sure about the method? Any bugs in the system?
 
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  • #34
You are almost there, you need to write the limits in terms of the new variable. Also, you lost a minus sign somewhere.
 
  • #35
-\int^{-1}_{1} {e^(\frac{-ip.z}{\hbar})}.dz
Right?
However, I was wondering, if I had made the same substitution but the Sine terms had not canceled (so ther was still a sine theta in there). Could I have proceeded because I'd now have a a substituted variable and the old variable that need integrating? Could I have treated the theta terms as constant despite theta being the variable of interest?
 
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  • #36
Right so I solved the theta integral, leaving my r integral as (subbing k for p/h and alpha for 1/a):

\phi(p) = \frac{2A}{(2\pi/\hbar)^{3/2}}\frac{2\pi}{k}\int^\infty_0{rSin(kr)e^{-\alpha r}}.dr

I tried to solve the integral by parts by subbing u =r and using the standard integrals.

\int{e^{ax} Sin(bx).dx = \frac{e^{ax}}{a^2+b^2}(aSin(bx)-bCos(bx)

and

\int{e^{ax} Cos(bx).dx = \frac{e^{ax}}{a^2+b^2}(bSin(bx)+aCos(bx)

Which I'm not sure about. I get (after fiddling with the constants)

\frac{2\sqrt{2}}{\pi k(\hbar^3a^3)^{1/2}}[\frac{k\alpha}{(k^2-\alpha^2)^2}]

Does this sound about right. Can anyone suggest a way to simplify this more?

Whats the forum stand on checking working? I tried the earlier expectation for the kinetic energy of the hydrogen ground state problem and am very close, except I'm a factor of 2 out and can't see where I lost it.
 
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  • #37
The Fourier transform of the ground state goes like \frac{1}{(k^2 + a^{-2}_0)^2}, so unfortunately you have made an error in your integration. Quite apart from anything else, your formula can't be right because it is singular at k = \alpha where as the real space wavefunction is non-singular and very well behaved (in other words, you shouldn't get in a singularity in the Fourier transform).
 
  • #38
Right, well the k in the constant and the numerator cancel. So my problem must be the extra alpha. I'll take a look at the working again. However can you tell me if there is anything wrong with using that standard integral to do the transform in r?
 
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  • #39
Nope still have that pesky alpha, and I feel like I'm so close too.:cry:

Can anyone see where I'm going wrong?

Starting with

\phi(p) = \frac{2A}{(2\pi/\hbar)^{3/2}}\frac{2\pi}{k}\int^\infty_0{rSin(kr)e^{-\alpha r}}.dr

Concentrating on the integral, I used by parts making the allocating the following.

\frac{dv}{dr} = e^{-\alpha r}Sin(kr) thus using the standard integral I mentioned I get v = \frac{e^{-\alpha r}}{k^2-\alpha^2}(- \alpha Sin(kr)-kCos(kr))

u = r thus \frac{du}{dr} = 1

Subbing this into the by parts formula I get.

[\frac{re^{-\alpha r}}{k^2-\alpha^2}(-\alpha Sin(kr) - kCos(kr))] - \frac{- \alpha}{k^2- \alpha^2}\int{e^{-\alpha r}Sin(kr)}.dr -\frac{k}{k^2-\alpha^2}\int{e^{-\alpha r}Cos(kr)}.dr

Making the integration gives me three terms, again, using the standard integrals.

[\frac{re^{-\alpha r}}{k^2-\alpha^2}(-\alpha Sin(kr) - kCos(kr))] - [\frac{- \alpha}{k^2-\alpha^2}}(-\alpha Sin(kr) - kCos(kr))] - [\frac{k}{k^2 - \alpha^2}(-\alpha Cos(kr) + kSin(kr))]

The terms have limits between zero and infinity. The infinity terms cancel as exp(-infinity) is zero. So only the zero substitutions count. As r = 0 the first term is canceled to zero. And as Sin zero is zero only the cos terms have anny significance. The Cos reduced to 1 and so I'm left with.

\frac{- \alpha}{k^2- \alpha^2}(\frac{k}{k^2-\alpha^2}) - \frac{k}{k^2-\alpha^2}({\frac{\alpha}{k^2 -\alpha^2})

Leaving me with \frac{2k \alpha}{(k^2-\alpha^2)^2}

And thus the same answer as before. The 2 belongs and the k cancels, its just the alpha that shouldn't be there that I can see. I can't see my error (I'm terrible at finding mistakes) can any of you guys (Assuming what I've written makes sense).

Thanks:biggrin:
 
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  • #40
Anyone see my error, this needs to be in tomorrow

Thanks
 
  • #41
hey who started this thread coz i have a piece of work exactly the same question that i am stuck on. I am studying at loughborough uni my name is owen!
 
  • #42
Beer-monster, you've got the wrong value for the integral, it should be k^2 + \alpha^2 in the denominator, how did you get -\alpha^2?

You might try to evaluate the integral by breaking the \sin{kr} up into its exponential parts. You should have two integrals to do, one involves e^{ikr-r/a_0} and the other involves e^{-ik-r/a_0} with an important relative minus sign. Each of these integrals is easy to do as it is a standard exponential integration. Once you've done each integral (be very careful with your minus signs), find a common denominator. The form I gave should pop right out.
 
  • #43
beer monkey

if you are doing prof alexanderovs questions for question 1b i get 0.65 (2dp)but I am unsure if that is correct everything seemed to fold out nicely but not sure
 
  • #44
I've solved the integrals but I get an addition of two (ik- \alpha)^2. I'm nnot how I can combine these into the form you described monkey? It's late and my brain has fallen asleep
 
  • #45
Got there in the end. I'd like to thank everyone on the forum who tried to help me with this problem. You've been a huge help in this and hopefully QM more generally.
 
  • #46
you made a error integrating, i do it by my self and the result is:

<br /> \phi(p) = \frac{4\pi}{(2\pi\hbar)^{3/2}}\frac{1}{\pi a^3}\frac{2a^3 \hbar ^4}{\left(\hbar ^2 + a^2 p^2 \right)^2}<br />
<br /> \phi(k) = \frac{4\pi}{(2\pi\hbar)^{3/2}}\frac{1}{\pi a^3}\frac{2a^3 \hbar ^4}{\left(\hbar ^2 +\hbar ^2 a^2 k^2 \right)^2}<br />
 
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