Total charge from charge density (spherical coordinates)

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SUMMARY

The discussion focuses on calculating charge density and total charge within a sphere using Gauss' law in spherical coordinates. The electric field is defined as \(\vec{E} = k r^2 \hat{r}\). In part (a), the charge density \(\rho(\vec{r})\) is derived as \(\rho = \frac{r}{\pi}\) using the differential form of Gauss' law. In part (b), the total charge \(Q_e\) contained in a sphere of radius \(R\) is calculated to be \(R^4\) through the integral form of Gauss' law. Part (c) involves integrating the charge density over the volume, but the user encounters confusion regarding the integration in spherical coordinates, leading to a mismatch with the result from part (b).

PREREQUISITES
  • Understanding of Gauss' law (both differential and integral forms)
  • Familiarity with spherical coordinates and volume integration
  • Knowledge of electric fields and charge density concepts
  • Proficiency in using the del operator (\(\nabla\)) in vector calculus
NEXT STEPS
  • Study the application of Gauss' law in various symmetrical charge distributions
  • Learn about spherical coordinate integration techniques for volume calculations
  • Explore the relationship between charge density and electric field in electrostatics
  • Review vector calculus, focusing on the del operator and its applications in physics
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Students of electromagnetism, physicists, and educators seeking to deepen their understanding of charge density calculations and the application of Gauss' law in spherical coordinates.

bfusco
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Homework Statement


In some region of space, the electric field is \vec{E} =k r^2 \hat{r}, in spherical coordinates, where k is a constant.
(a) Use Gauss' law (differential form) to find the charge density \rho (\vec{r}).

(b) Use Gauss' law (integral form) to find the total charge containted in a sphere of radius R, centered at r=0

(c) Find the total charge contained in a sphere of radius R, centered at r=0 by direct integration of your result for \rho (\vec{r}) in (a). Does the answer agree with that in (b)?

The Attempt at a Solution


NOTE: IM USING \Delta as the del operator

Im pretty sure my problems only arise on part (c), but if any error is noticed in the other parts please tell me. Thank you

(a)using \vec{ \Delta} \bullet \vec{E} = \frac{\rho}{\epsilon_0}
rearranging it to solve for \rho i get \rho = \epsilon( \vec{\Delta} \bullet \vec{E}) where \epsilon( \vec{\Delta} \bullet \vec{E}) = \frac{\epsilon_0}{r^2} \frac{d(r^2 k r^2)}{dr} which reduces to \frac{r}{\pi}

(b) using \oint \Delta \bullet d\vec{a} = \frac{Q_e}{\epsilon_0} and rearranging to solve for Q_e i get Q_e=\epsilon_0 \oint \vec{E} \bullet d\vec{a}, which since the sphere is symmetric about the origin i can do \epsilon_0 \oint |\vec{E}| d\vec{a}, which equals \epsilon_0 k r^2 4\pi R^2 which reduces to R^4 (note: i replaced r^2 with R^2)

(c) knowing \rho = \frac{dq}{dV} and reorganizing to solve for dq i get \int dq = \int \rho(\vec{r}) dV at this point I am a little confused on how to take the integral with respect to dV in spherical coordinates. I am pretty sure i have to add an r^2 in the integrand but I am not sure.
 
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dV = r^2 \sin(\theta) dr d\theta d\phi
 
bfusco said:
1
NOTE: IM USING \Delta as the del operator


Don't! To most people,
\Delta = \nabla^2

Since you're using tex, just use \nabla for the del operator.
 
phyzguy said:
Don't! To most people,
\Delta = \nabla^2

Since you're using tex, just use \nabla for the del operator.

lol ok, i didnt know that

test \nabla
 
Bryson said:
dV = r^2 \sin(\theta) dr d\theta d\phi

alright so since non of these variables have any unit vector other than \hat{r} the r^2 sin\theta =0 ?? at which point the integral will be \oint \frac{r}{\pi} dr
which is \frac{r^2}{2\pi} which doesn't match part (b), and therefore i am incorrect somewhere.
 

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