Deriving potential energy of an electron inside a nucleus

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SUMMARY

The discussion centers on deriving the potential energy of an electron within a uniformly charged nucleus, represented by the equation V'(r) = (-Ze²/4πε₀R)(3/2 - (1/2)(r/R)²). Participants emphasize the importance of definite integrals in calculating the potential energy, particularly when integrating from infinity to a point inside the sphere. The user mafisco initially struggles with the integration limits and the derivation of the 3/2 term but receives guidance on the correct approach to definite integrals, ultimately resolving the issue.

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mafisco
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Homework Statement



Derive equation below. It is the potential energy of an electron inside a nucleus assumed to be a uniformly charged sphere of R.

Homework Equations



V'(r) =( -Ze2/4∏ε0R)(3/2 - (1/2)(r/R)^2)

The Attempt at a Solution



So I understand that I need to find the

∫ from infinity to a point A (A exists inside the uniformly charged sphere)

I did this by splitting it between infinity to B(on surface of sphere) and A to B.

I did get the (-Ze^2/4∏ε0R)(1/2)(r/R)^2, but I just am lost for the 3/2. Any help would be wonderful.

Thanks!
 
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Hello, mafisco. Welcome to PF.

Sounds like you have the right idea. Can you show more detail of your calculation for each part of the split?
 
Hey, thanks! I'm going to be here for a while I believe, taking on a nuclear physics class and it's been a while since I've done physics.

Alright, so I know that

E*dA= (Qenc/(ε0*Volume(4/3∏R3))) * new volume(4/3∏r3)

for the limit integral of A to B.

Taking Qenc = Ze2 and dA = 4∏r2,

I get E = Ze2r/(4∏ε0R3)

With integration, it becomes E = (Ze2r2)/(8∏ε0R3)

That's the right hand part of what I need, but the left hand part (which I thought would be easy) appears to not give me the 3/2 I need.

What I tried :-
E*dA = Qenc/ε0. dA = 4∏r2, Qenc = Ze2.

I would end up with E = (Ze2)/(4∏ε0r2) which doesn't really give me the result I need after integration.

Let me know what I can do! Thanks!
 
Last edited:
You should be doing definite integrals. So, you need to substitute in the limits of integration corresponding to points B and A.

Likewise for the integration outside the sphere from infinity to B.

(I actually prefer to switch the order of the limits and make up for it by changing the overall sign of the integrals. That way I'm always integrating from small to larger values of r and my lower limits on the integrals are less than the upper limits. So, inside the sphere, I integrate from A to B (on surface) and then outside I integrate from B to infinity. If I don't do it this way I invariably get some signs wrong. :redface:)
 
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Wonderful.

That did the trick my man, thank you very much. It seems as if I had forgotten definite integrals quite sadly.

Hope to see more people like you around, thanks again!
 
I don't get the integration limits! Can you please show how you evaluated when applying the limits?
 

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