please solve this problem step by stepA disk of radius a lies in the x-y plane, with the z axis through its center. Surface
charge of uniform density pg C/m? lies on the disk, which rotates about the z axis at
angular velocity w rad/s. Express the magnetic field intensity H at any point on the
z axis. (Hint: Just like ] = p,¥ on P8 of L_17 Slides, K = ps)
Question:
please solve this problem step by stepA disk of radius a lies in the x-y plane, with the z axis through its center. Surface
charge of uniform density pg C/m? lies on the disk, which rotates about the z axis at
angular velocity w rad/s. Express the magnetic field intensity H at any point on the
z axis. (Hint: Just like ] = p,¥ on P8 of L_17 Slides, K = ps)
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Asked by: Mohin
Created at: 2025-10-18 11:17:33
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Let's solve the problem step by step.
---
## **Step 1: Understanding the Problem**
- **Disk of radius** \( a \) **in the \(xy\)-plane**
- **Uniform surface charge density:** \( \rho_s \) (C/m\(^2\))
- **Disk rotates about \(z\)-axis** at angular velocity \( \omega \) (rad/s)
- **Find:** Magnetic field intensity \( \vec{H} \) at any point on the \(z\)-axis
---
## **Step 2: Surface Current Density**
When charged disk rotates, each point at radius \( r \) has velocity
\[
\vec{v} = \omega r \, \hat{\phi}
\]
The **surface current density** is:
\[
\vec{K} = \rho_s \vec{v} = \rho_s \omega r \, \hat{\phi}
\]
---
## **Step 3: Magnetic Field on the \(z\)-axis**
By **symmetry**, the field on the \(z\)-axis points along \( \hat{z} \).
We can use the **Biot-Savart Law** for surface currents:
\[
\vec{H} = \frac{1}{4\pi} \int_S \frac{\vec{K} \times \vec{R}}{R^3} dS
\]
where:
- \(\vec{R}\) is the vector from the surface element to the field point (on z-axis at \(z\))
---
## **Step 4: Setting Up the Integral**
Let a surface element on the disk be at \( (r', \phi', ) \).
Let the field point be at \( (, , z) \).
\[
\vec{R} = (,,z) - (r'\cos\phi', r'\sin\phi', ) = (-r'\cos\phi', -r'\sin\phi', z)
\]
\[
R = \sqrt{r'^2 + z^2}
\]
\[
\vec{K} = \rho_s \omega r' \hat{\phi}'
\]
where \( \hat{\phi}' = -\sin\phi' \hat{x} + \cos\phi' \hat{y} \)
---
## **Step 5: Cross Product**
\[
\vec{K} \times \vec{R}
\]
Let's write out:
\[
\vec{K} = \rho_s \omega r' (-\sin\phi' \hat{x} + \cos\phi' \hat{y})
\]
\[
\vec{R} = -r'\cos\phi' \hat{x} - r'\sin\phi' \hat{y} + z \hat{z}
\]
Now, cross each term:
- \( (-\sin\phi' \hat{x}) \times (-r'\cos\phi' \hat{x}) = \)
- \( (-\sin\phi' \hat{x}) \times (-r'\sin\phi' \hat{y}) = -\sin\phi' \hat{x} \times -r'\sin\phi' \hat{y} = r' \sin^2\phi' \hat{z} \)
- \( (-\sin\phi' \hat{x}) \times (z \hat{z}) = -z\sin\phi' (\hat{x} \times \hat{z}) = -z\sin\phi' (-\hat{y}) = z\sin\phi' \hat{y} \)
- \( (\cos\phi' \hat{y}) \times (-r'\cos\phi' \hat{x}) = -r'\cos\phi' \cos\phi' (\hat{y} \times \hat{x}) = -r'\cos^2\phi' (-\hat{z}) = r'\cos^2\phi' \hat{z} \)
- \( (\cos\phi' \hat{y}) \times (-r'\sin\phi' \hat{y}) = \)
- \( (\cos\phi' \hat{y}) \times (z \hat{z}) = z\cos\phi' (\hat{y} \times \hat{z}) = z\cos\phi' \hat{x} \)
Sum all z-components:
\[
(r'\sin^2\phi' + r'\cos^2\phi') \hat{z} = r'(\sin^2\phi' + \cos^2\phi') \hat{z} = r' \hat{z}
\]
Sum all x and y components:
- x: \( z\cos\phi' \)
- y: \( z\sin\phi' \)
So,
\[
\vec{K} \times \vec{R} = \rho_s \omega r' \left[ z\cos\phi' \hat{x} + z\sin\phi' \hat{y} + r' \hat{z} \right]
\]
---
## **Step 6: Integrate Over the Disk**
Only the \( \hat{z} \) component survives when integrating over \( \phi' \) from to \( 2\pi \):
\[
\vec{H}(,,z) = \frac{1}{4\pi} \int_^a \int_^{2\pi} \frac{\rho_s \omega r' \cdot r' \hat{z}}{(r'^2 + z^2)^{3/2}} r' d\phi' dr'
\]
(Area element: \( dS = r' d\phi' dr' \))
\[
\vec{H}(,,z) = \frac{\rho_s \omega}{4\pi} \hat{z} \int_^a \int_^{2\pi} \frac{r'^2}{(r'^2 + z^2)^{3/2}} d\phi' dr'
\]
\[
\int_^{2\pi} d\phi' = 2\pi
\]
\[
\vec{H}(,,z) = \frac{\rho_s \omega}{2} \hat{z} \int_^a \frac{r'^2}{(r'^2 + z^2)^{3/2}} dr'
\]
---
## **Step 7: Solve the Integral**
Let’s solve:
\[
I = \int_^a \frac{r'^2}{(r'^2 + z^2)^{3/2}} dr'
\]
Let \( u = r'^2 + z^2 \implies du = 2r' dr' \implies dr' = \frac{du}{2r'} \)
When \( r' = , u = z^2 \); when \( r' = a, u = a^2 + z^2 \)
But let's use substitution:
Let’s use \( r' = z \tan\theta \implies dr' = z \sec^2\theta d\theta \)
Then \( r'^2 + z^2 = z^2 \sec^2\theta \), \( r'^2 = z^2 \tan^2\theta \)
So:
\[
I = \int_{\theta=}^{\arctan(a/z)} \frac{z^2 \tan^2\theta}{(z^2 \sec^2\theta)^{3/2}} z \sec^2\theta d\theta
\]
\[
= \int_^{\arctan(a/z)} \frac{z^2 \tan^2\theta}{z^3 \sec^3\theta} z \sec^2\theta d\theta
\]
\[
= \int_^{\arctan(a/z)} \frac{z^3 \tan^2\theta \sec^2\theta}{z^3 \sec^3\theta} d\theta
\]
\[
= \int_^{\arctan(a/z)} \tan^2\theta \frac{1}{\sec\theta} d\theta
= \int_^{\arctan(a/z)} \tan^2\theta \cos\theta d\theta
\]
Let’s use \( \tan^2\theta = \sec^2\theta - 1 \):
\[
= \int (\sec^2\theta - 1) \cos\theta d\theta
= \int \sec^2\theta \cos\theta d\theta - \int \cos\theta d\theta
\]
\[
\int \sec^2\theta \cos\theta d\theta = \int \frac{1}{\cos^2\theta} \cos\theta d\theta = \int \frac{1}{\cos\theta} d\theta = \int \sec\theta d\theta
\]
So,
\[
I = \int \sec\theta d\theta - \int \cos\theta d\theta
= \ln|\sec\theta + \tan\theta| - \sin\theta
\]
Back to the limits:
When \( r' = \), \( \tan\theta = \rightarrow \theta = \)
When \( r' = a \), \( \tan\theta = a/z \rightarrow \theta = \arctan(a/z) \)
So,
\[
I = \left[\ln|\sec\theta + \tan\theta| - \sin\theta \right]_^{\arctan(a/z)}
\]
Compute at \( \theta = \arctan(a/z) \):
- \( \tan\theta = a/z \)
- \( \sec\theta = \sqrt{1 + \tan^2\theta} = \sqrt{1 + (a/z)^2} = \sqrt{z^2 + a^2}/z \)
- \( \sin\theta = \frac{\tan\theta}{\sqrt{1 + \tan^2\theta}} = \frac{a/z}{\sqrt{1 + (a/z)^2}} = \frac{a}{\sqrt{z^2 + a^2}} \)
At \( \theta = \):
- \( \tan = \), \( \sec = 1 \), \( \sin = \)
So,
\[
I = \left[ \ln\left( \frac{\sqrt{z^2 + a^2}}{z} + \frac{a}{z} \right) - \frac{a}{\sqrt{z^2 + a^2}} \right] - [\ln(1) - ]
\]
\[
= \ln\left( \frac{\sqrt{z^2 + a^2} + a}{z} \right) - \frac{a}{\sqrt{z^2 + a^2}}
\]
---
## **Step 8: Final Expression**
\[
\boxed{
\vec{H}(,,z) = \frac{\rho_s \omega}{2} \left[ \ln\left( \frac{\sqrt{z^2 + a^2} + a}{z} \right) - \frac{a}{\sqrt{z^2 + a^2}} \right] \hat{z}
}
\]
---
### **Summary**
- Compute surface current density: \( \vec{K} = \rho_s \omega r \hat{\phi} \)
- Use Biot-Savart law for surface currents
- Integrate over the disk and evaluate on the \(z\)-axis
- Result above gives the magnetic field intensity at any point on the \(z\)-axis due to the rotating charged disk
---
**Let me know if you need further clarification or a check for special cases (e.g., on the axis near the center or far away)!**
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