How to calculate the magnetic field generated by accelerating charges?

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SUMMARY

The discussion focuses on calculating the magnetic field generated by accelerating charges using Jefimenko's equations and Lienard-Wiechert potentials. Key methods include deriving the scalar potential (φ) and vector potential (A) through the equations E = -∇φ - ∂A/∂t and B = ∇×A. A significant challenge in this process is solving for the retarded time (tr), which accounts for the propagation of electromagnetic changes from the charge to the observation point. Relevant literature includes Griffiths chapters 10 and 11, as well as Heald and Marion chapters 8 and 9.

PREREQUISITES
  • Understanding of Jefimenko's equations
  • Familiarity with Lienard-Wiechert potentials
  • Knowledge of electromagnetic field equations (E and B fields)
  • Concept of retarded time in electromagnetic theory
NEXT STEPS
  • Study Griffiths chapters 10 and 11 for problem sets on electromagnetic fields
  • Explore Heald and Marion chapters 8 and 9 for further insights on accelerating charges
  • Research the quasistatic approximation and its applications
  • Learn about the physical implications of current density derivatives in electromagnetic theory
USEFUL FOR

Physicists, electrical engineers, and students studying electromagnetism, particularly those interested in the dynamics of accelerating charges and their effects on magnetic fields.

the_m-theorist
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my guess was Jefimenko's equations could be used, am i right? also are there any other relevant equations or methods? also what does the current density derivative in the equation (in terms of the acceleration) for the magnetic field physically mean? p.s. my first post on the internet!
 
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You just use the Lienard-Wiechert potentials to get the scalar potential ##\varphi## and vector potential ##\vec{A}## and use the definitions ##\vec{E} = -\vec{\nabla}\varphi - \partial_t \vec{A}## and ##\vec{B} = \vec{\nabla}\times \vec{A}##. The only hard part (and it is a really hard part) in the calculation is solving for the retarded time ##t_r## in terms of the actual time ##t## since the changes in the electromagnetic field carried by the particle have to propagate from the field point of the charge (with which ##t_r## is associated) to the observation point (with which ##t## is associated). See Griffiths chapters 10 and 11 for problem sets on this as well as on the ultra-important application to radiation fields.

EDIT: and also Heald and Marion chapters 8 and 9.
 
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