SUMMARY
The magnetic field on the axis of a circular current loop of radius a is given by the formula \mathbf{B}=\frac{\mu_0 I a^2}{2(a^2+z^2)^{\frac{3}{2}}} \mathbf{\hat{z}}, where I is the current and z is the distance from the center of the loop. For an insulating disc with uniform surface charge density \sigma rotating at angular velocity \omega, the surface current density is defined as \mathbf{K(r)}=\sigma \mathbf{\omega} \wedge \mathbf{r}. The contribution to the magnetic field from a ring of radius r is expressed as B_z = \frac{\mu_0}{2} \int_{0}^{a} \frac{\sigma \omega r^3 dr}{(r^2+z^2)^{\frac{3}{2}}}. As z approaches infinity, the magnetic field behaves as \mathbf{B}(z) \sim \frac{1}{8} \mu_0 \sigma \omega \frac{a^4}{z^3} \mathbf{\hat{z}}.
PREREQUISITES
- Understanding of magnetic fields and current loops
- Familiarity with surface charge density and current density concepts
- Knowledge of integration techniques, particularly for evaluating definite integrals
- Proficiency in applying the binomial expansion for limits
NEXT STEPS
- Learn advanced integration techniques for evaluating complex integrals in electromagnetism
- Study the derivation of magnetic fields from rotating charged bodies
- Explore the implications of the binomial expansion in physics problems
- Investigate the behavior of magnetic fields at infinity in various geometries
USEFUL FOR
Students and professionals in physics, particularly those focusing on electromagnetism, electrical engineering, and applied mathematics.