What is the impact of a source point just at the field point in Coulomb's Law?

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The discussion centers on the application of Coulomb's Law to determine the electric field at a point inside a uniformly charged sphere. There is concern about the contribution from a source point located at the same position as the field point, as this could imply an infinite contribution due to zero distance. The conversation highlights that while Coulomb's Law is an approximation, it can be derived from Maxwell's Equations, which may provide a more rigorous framework. Additionally, for interactions at very small distances, Quantum Electrodynamics (QED) would be necessary for accurate analysis. The complexities of these concepts underline the limitations of classical electrostatics in certain scenarios.
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Hi there,

I have a question about Coulomb's Law. Assume there is a uniform sphere charge distribution RHO and I want to know the electric field at some point inside the sphere. I can simply apply Coulomb's Law to find it. However, I worry about the contribution from source point that is "just" at the field point. Based on Coulomb's Law, the distance between the source point and field point now is zero and the contribution might become infinity. Although the charge there is infinitesimal, the contribution from it is still unspecified. After all, no rigorous mathematical proof says that the contribution is zero. Can anyone give me an explanation about this point?
 
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Coulomb's Law is an approximation and can be derived from the more general, yet still classical, Maxwell's Equations, which will probably be better to deal with this. To really answer a question about interactions between charged particles at extremely small distances you'd need to use QED (Quantum Electrodynamics).
 
It may be shown from the equations of electromagnetism, by James Clerk Maxwell in the 1860’s, that the speed of light in the vacuum of free space is related to electric permittivity (ϵ) and magnetic permeability (μ) by the equation: c=1/√( μ ϵ ) . This value is a constant for the vacuum of free space and is independent of the motion of the observer. It was this fact, in part, that led Albert Einstein to Special Relativity.

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