
Explore core electrodynamics concepts from Griffiths' Introduction to Electrodynamics, building on basic electromagnetism and Maxwell's equations through guided theory and solved exercises.
Investigate how time-dependent electromagnetism reshapes conservation, energy, and charge continuity. Explore electromagnetic momentum, Maxwell's stress tensor, and angular momentum, including its quantization, while solving exercises.
Define the poynting vector as the energy flux density, the power carried across a surface by electromagnetic fields, and relate it to energy conservation via its divergence.
Shows how Maxwell's stress tensor resolves apparent violations of Newton's third law by encoding electric and magnetic field momentum into a force as the divergence of the tensor.
Derive the force on charges via Maxwell's stress tensor, separating pressure and shear terms, in static cases, and compute Coulomb forces with boundary surface integrals.
Explore how to compute the net force on the northern hemisphere of a uniformly charged solid sphere using Maxwell's stress tensor, with boundary surfaces and spherical coordinates.
Learn momentum and angular momentum conservation in electromagnetic fields, derive the field momentum from E cross B, and apply the Maxwell stress tensor in a coaxial cable example.
Derive the electric and magnetic fields of an oscillating electric dipole from potentials using Maxwell's equations, then apply three approximations to obtain the radiation-zone field.
Derive the vector potential for an oscillating electric dipole and compute the electric and magnetic fields in the radiation zone, then obtain the pointing vector and the omega^4 power law.
Analyze magnetic dipole radiation from a circulating current loop, defining the magnetic dipole moment. Compare with electric dipole radiation and derive the vector potential in the static limit.
In this course we will work all the theory corresponding to the Electromagnetic laws but in a dynamic situation.
The normal way to teach EM is first building a theory where all the system is static. In that case, you can obtain basic physical laws and understand the nature of electromagnetic interactions.
Once that is done, its interesting go further and see what happens when the system is free to evolve in time. This is what we call Electrodynamics and will led us to interesting results.
Obviously, the new results that we will find here have to be consistent with the fundamental static theory. During the lectures, we will see that sometimes, we derive the static equations from the new dynamic ones just to verify that the math work was well done.
This is the way scientists have created new theories using the Scientific Method. One famous example of this is the General and Special Relativity introduced by Albert Einstein. These theories improve and go further than the previous laws of Gravitation intoduced by Isaac Newton.
So, the main goal of this course is to learn many concepts about Electrodynamics with the support of some lectures and examples presenting solved exercices.