Conduction and displacement currents for a spherical solid

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SUMMARY

The discussion focuses on the cancellation of conduction and displacement currents in a spherical radioactive solid emitting charged particles radially. It highlights the relationship between radial conduction current density, ##j_r##, and charge density, ##\rho##, emphasizing local charge conservation principles. The displacement current density, ##j_d##, is linked to the time derivative of the electric displacement field, ##\dot{\mathbf{D}}##. The problem requires understanding Maxwell's equations and the behavior of charged particles in a spherical geometry.

PREREQUISITES
  • Maxwell's equations
  • Current density (j) concepts
  • Displacement current density (jd) understanding
  • Charge conservation principles
NEXT STEPS
  • Study the derivation of local charge conservation from Maxwell's equations
  • Explore the relationship between electric displacement field (D) and charge density (ρ)
  • Investigate the implications of radioactive decay on charge distribution in materials
  • Learn about the mathematical treatment of conduction and displacement currents in spherical coordinates
USEFUL FOR

This discussion is beneficial for physics students, electrical engineers, and researchers interested in electromagnetic theory, particularly in the context of charge dynamics in spherical geometries.

Huan Nguyen
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Homework Statement


Show that the conduction and displacement currents cancel each other for a spherical radioactive solid emitting charged particles radially outwards

Homework Equations


Maxwell's equations
Current density (j)
Displacement current density (jd)

The Attempt at a Solution


I haven't made it very far into the problem. I think "the conduction" means i=dq/dt and "displacement current" id=jd*S with jd= ∂D/∂t. However, I am still struggling to understand the problem.
 
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Huan Nguyen said:
I am still struggling to understand the problem.
Hello, Huan. Welcome to PF!

Every volume element of the sphere will be continually emitting charged particles due to the radioactive decay. The emitted particles are assumed (unrealistically) to stream out radially without being reabsorbed anywhere in the sphere. So, as the sphere emits particles the sphere builds up charge. Charge must be conserved locally and this can be used to relate the radial conduction current density, ##j_r##, to the charge density, ##\rho##, of the sphere. There is a well known formula for local charge conservation.

As you noted, the displacement current, ##j_d##, is related to ##\dot{\mathbf{D}}##. You'll need to relate ##\mathbf{D}## to ##\rho##.
 

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