Equivalence of Integral and Differential Forms of Gauss's Law?

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SUMMARY

The discussion centers on the equivalence of integral and differential forms of Gauss's Law, specifically for a sphere with charge density ρ = k·r. The integral form yields an electric field E = (k·r²)/(4ε) inside the sphere, while the divergence of E calculated using the differential form results in ∇·E = (k·r)/(2ε), which is half of the expected value. The discrepancy arises from the application of differential operators in curvilinear coordinates versus Cartesian coordinates. The correct electrostatic potential is derived as φ(r) = -(k/12)r³, leading to the consistent result for the divergence of E.

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A sphere has charge density \rho=k\cdot r. Using the integral form of Gauss's Law, one easily finds that the electric field is E=\frac{k\cdot r^2}{4\epsilon} anywhere inside the sphere. However, \nabla\cdot E=\frac{k\cdot r}{2\epsilon}, which is half of what should be expected from the differential form of Gauss's Law, since \frac{\rho}{\epsilon}=\frac{k\cdot r}{\epsilon}. Why is this?
 
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In Heaviside-Lorentz units, the equation for the electrostatic potential reads

\Delta \phi(\vec{x})=-\rho(\vec{x}).

In spherical coordinates, for a radially symmetric charge distribution, this equation simplifies to the ode,

\frac{1}{r} \mathrm{d}_r^2 (r \phi)=:\frac{1}{r} (r \phi)''=-\rho(r).

Here, r=|\vec{x}|. In your case we have

(r \phi)''=-k r^2.

This you can integrate up successively:

(r \phi)'=-\frac{k}{3} r^3+C_1, \quad r \phi=-\frac{k}{12} r^4 + C_1 r+C_2

or, finally,

\phi(r)=-\frac{k}{12} r^3 + C_1 + \frac{C_2}{r}.

The integration constants, C_1 and C_2, are determined by appropriate boundary conditions, where C_1 is physically irrelevant since the electric field is the observable quantity, which is given by the gradient of the potential. So I set C_1=0 Further, since the charge distribution is continuous at the origin, we must have C_2=0. So finally we get

\phi(r)=-\frac{k}{12} r^3, \quad \vec{E}=-\vec{\nabla} \phi = \frac{k}{4} r^2 \vec{e}_r = \frac{k}{4} r \vec{x}.

To check this result, we take the divergence, which for our case of \vec{E}=E_r(r) \vec{e}_r simplifies to

\vec{\nabla} \cdot \vec{E}=\frac{1}{r^2} (r^2 E_r)'=\frac{1}{r^2} \left (\frac{k r^4}{4} \right )'=k r=\rho

as it should be since Maxwell's equations for the electrostatic case read

\vec{\nabla} \times \vec{E}=0, \quad \vec{\nabla} \cdot \vec{E}=\rho.

I guess, your confusion comes from forgetting that the differential operators look different in curvilinear coordinates compared to the expressions in cartesian ones.

Of course, you can calculate the divergence also in Cartesian coordinates. Although this is a bit more inconvenient in your case of spherical symmetry, you must get the same result. Indeed using the Cartesian form

\vec{E}=\frac{k}{4} \sqrt{x^2+y^2+z^2} \vec{x}

you get again

\vec{\nabla} \cdot \vec{E}=\partial_x E_x+\partial_y E_y+\partial_z E_z=\frac{k}{4} \left (\frac{2 x^2+y^2+z^2}{r}+\frac{x^2+2y^2+z^2}{r}+\frac{x^2+y^2+2 z^2}{r} \right) =\frac{k}{4} \frac{4(x^2+y^2+z^2)}{r}=k r.
 
Thank you. I did take the divergence incorrectly.
 

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