Charge density for a given potential

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The discussion centers on calculating charge density and electric field from a given electric potential. The charge density is specified as ρ = ε₀A(4πδ³(r) - λ²e^(-λr)/r). The user successfully derived the electric field E = Ae^(-λr)(1 + λr)/r², but struggled with the divergence of E, particularly at r = 0, where standard expressions do not apply. Clarification was provided regarding the use of divergence and gradient in spherical coordinates, emphasizing that the second term does not involve a divergence but rather a gradient. Understanding these vector calculus identities is crucial for correctly applying the equations in this context.
Silviu
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Homework Statement


Given the electric potential ##V(r)=A\frac{e^{-\lambda r}}{r}## calculate the charge density ##\rho(r)## and the electric field ##E(r)##.
They specify the answer for charge density should be: ##\rho = \epsilon_0 A(4\pi \delta^3(r)-\lambda^2e^{-\lambda r}/r)##

Homework Equations


##E=-\nabla V##
##\nabla E = \frac{\rho}{\epsilon_o}##

The Attempt at a Solution


For the electric field I got: ##E = Ae^{-\lambda r}(1+\lambda r)/r^2##, pointing in the r direction and this is the same as their answer. Then I tried to take the divergence of E, and in spherical coordinates this would be ##\nabla E = \frac{1}{r^2}\frac{\partial r^2 E}{\partial r} = \frac{1}{r^2}\frac{\partial (Ae^{-\lambda r}(1+\lambda r))}{\partial r} ## . However this doesn't give me a delta function so I am not sure where I did something wrong.
 
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Your expression for the divergence is only valid for ##r\ne 0##. You need to consider what's happening at ##r=0## in another way.
 
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vela said:
Your expression for the divergence is only valid for ##r\ne 0##. You need to consider what's happening at ##r=0## in another way.
Thank you! So I found a solution online to this problem but I am still a bit confused. I attached their solution. So i understand how they obtain the delta function but when they apply the divergence to the other term, they use ##\frac{\partial}{\partial r}##. Shouldn't they use the divergence in spherical coordinates which is ##\frac{1}{r^2}\frac{\partial (r^2 E')}{\partial r}##, with E' being the term that remained to be acted on?
 

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Silviu said:
So i understand how they obtain the delta function but when they apply the divergence to the other term, they use ##\frac{\partial}{\partial r}##. Shouldn't they use the divergence in spherical coordinates ...?
They are using the identity
upload_2017-2-19_16-56-10.png

where ##\psi## is a scalar function.

(See https://en.wikipedia.org/wiki/Vector_calculus_identities#Product_of_a_scalar_and_a_vector)

The second term on the right does not involve a divergence. It involves a gradient.
 

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