Differences
This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision Next revision | Previous revision | ||
| 184_notes:examples:week5_flux_two_radii [2017/09/18 13:28] – [Solution] tallpaul | 184_notes:examples:week5_flux_two_radii [2021/06/04 00:47] (current) – schram45 | ||
|---|---|---|---|
| Line 1: | Line 1: | ||
| + | [[184_notes: | ||
| + | |||
| =====Example: | =====Example: | ||
| Suppose you have a point charge with value $1 \mu\text{C}$. What are the fluxes through two spherical shells centered at the point charge, one with radius $3 \text{ cm}$ and the other with radius $6 \text{ cm}$? | Suppose you have a point charge with value $1 \mu\text{C}$. What are the fluxes through two spherical shells centered at the point charge, one with radius $3 \text{ cm}$ and the other with radius $6 \text{ cm}$? | ||
| Line 9: | Line 11: | ||
| * $\Phi_e$ for each sphere | * $\Phi_e$ for each sphere | ||
| * $\text{d}\vec{A}$ or $\vec{A}$, if necessary | * $\text{d}\vec{A}$ or $\vec{A}$, if necessary | ||
| - | |||
| - | ===Approximations & Assumptions=== | ||
| - | * There are no other charges that contribute appreciably to the flux calculation. | ||
| - | * There is no background electric field. | ||
| - | * The electric fluxes through the spherical shells are due only to the point charge. | ||
| ===Representations=== | ===Representations=== | ||
| Line 21: | Line 18: | ||
| $$\vec{E}=\frac{1}{4\pi\epsilon_0}\frac{q}{r^2}\hat{r}$$ | $$\vec{E}=\frac{1}{4\pi\epsilon_0}\frac{q}{r^2}\hat{r}$$ | ||
| * We represent the situation with the following diagram. Note that the circles are indeed spherical shells, not rings as they appear. | * We represent the situation with the following diagram. Note that the circles are indeed spherical shells, not rings as they appear. | ||
| - | {{ 184_notes: | + | [{{ 184_notes: |
| + | |||
| + | <WRAP TIP> | ||
| + | ===Approximations & Assumptions=== | ||
| + | There are a few approximations and assumptions we should make in order to simplify our model. | ||
| + | * There are no other charges that contribute appreciably to the flux calculation. | ||
| + | * There is no background electric field. | ||
| + | * The electric fluxes through the spherical shells are due only to the point charge. | ||
| + | The first three assumptions ensure that there is nothing else contributing or affecting the flux through our spheres in the model. | ||
| + | * Perfect spheres: This will simplify our area vectors and allows us to use geometric equations for spheres in our calculations. | ||
| + | * Constant charge for the point charge: Ensures that the point charge is not charging or discharging with time. | ||
| + | </ | ||
| ====Solution==== | ====Solution==== | ||
| - | Before we dive into calculations, | + | Before we dive into calculations, |
| + | |||
| + | [{{ 184_notes: | ||
| - | Since $\vec{E}$ is constant with respect | + | Since the shell is a fixed distance from the point charge, the electric field has constant magnitude on the shell. |
| $$\Phi_e=\int\vec{E}\bullet \text{d}\vec{A} = E\int\text{d}A$$ | $$\Phi_e=\int\vec{E}\bullet \text{d}\vec{A} = E\int\text{d}A$$ | ||
| - | We can rewrite | + | Note that $E$ is a scalar value representing $\vec{E}$ as a magnitude, |
| $$E = \frac{1}{4\pi\epsilon_0}\frac{q}{r^2}\left|\hat{r}\right| = \frac{1}{4\pi\epsilon_0}\frac{q}{r^2}$$ | $$E = \frac{1}{4\pi\epsilon_0}\frac{q}{r^2}\left|\hat{r}\right| = \frac{1}{4\pi\epsilon_0}\frac{q}{r^2}$$ | ||
| - | We can plug in values for $q$ and $r$ for each spherical shell, using what we listed in the facts. For the smaller shell, we have $E=1.0\cdot 10^7 \text{ N/C}$. For the larger shell, we have $E=2.5\cdot 10^6 \text{ N/C}$. | + | We can plug in values for $q$ and $r$ for each spherical shell, using what we listed in the facts. For the smaller shell, we find $E=1.0\cdot 10^7 \text{ N/C}$. For the larger shell, we find $E=2.5\cdot 10^6 \text{ N/C}$. |
| To figure out the area integral, notice that the magnitude of the area-vector is just the area. This means that our integrand is the area occupied by $\text{d}A$. Since we are integrating this little piece over the entire shell, we end up with the area of the shell' | To figure out the area integral, notice that the magnitude of the area-vector is just the area. This means that our integrand is the area occupied by $\text{d}A$. Since we are integrating this little piece over the entire shell, we end up with the area of the shell' | ||