Electric Field Problem 2.46 Griffiths

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SUMMARY

The electric field configuration described in Problem 2.46 of Griffiths' "Introduction to Electrodynamics" is represented by the potential function V(r) = a (e^(λr)/r). The charge density ρ(r) is derived as ρ = ε₀ A (4π δ³(r) - (λ² e^(-λr))/r). The total charge Q is calculated by integrating the charge density over all space, which requires careful consideration of the Dirac delta function and spherical coordinates. The correct approach involves integrating from 0 to infinity for r, and the resulting total charge is Q = -4π ε₀ A.

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  • Knowledge of spherical coordinates and volume integrals
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  • Review Griffiths' "Introduction to Electrodynamics" Chapter 1 for foundational concepts
  • Explore advanced integration techniques in calculus, focusing on improper integrals
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Problem 2.46 Griffiths EM
The electric field of some configuration is given by the expression
[tex]V(\vec{r}) = a \frac{e^{\lambda r}}{r}[/tex]

where A and lambda are constants. Find the electric field E(r) , charge density rho (r) and the total charge Q

i can easily find the E and rho
in fact rho is given by
[tex]\rho = \epsilon_{0} A (4 \pi \delta^3(\vec{r}) - \frac{\lambda^2 e^{-\lambda r}}{r})[/tex]

now there's the part of finding the total charge Q

i have to integrate roh over all space.. but wait.. the potential will blow up to negative infinity if we included negative value for r. But what about the part with the dirac delta function?? Is it integrated over all space or just the part for which r is valid. On my assignment i integrated the dirac delta from 0 to r and the resulting integral was zero

so my integral looks like

[tex]Q = \epsilon_{0} A \left( 4 \pi \int_{0}^{\infty} \delta^3 (\vec{r}) d\vec{r} - \int_{0}^{\infty} \frac{\lambda^2 e^{-\lambda r}}{r} dr \right) = - 4\pi \epsilon_{0} A[/tex]

but my prof says that the integral for the delta function should for all values of r that is -infty to +infty. But that would yield an answer of zero for Q. how can there be zero charge enclosed??
 
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For your Q you should be doing a volume integral over the entire space. This means that, in spherical coordinates, you need to integrate over r from 0 to infinity, theta from 0 to pi, and phi from 0 to 2pi. And don't forget to include the differential volume element in spherical coordinates as well (see inside front cover of Griffiths and Griffiths Chapter 1).
 

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