Course |
Learning outcome (at course level) |
Learning and teaching strategies |
Assessment Strategies |
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Paper Code |
Paper Title |
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PHY 321 |
Classical Electrodynamics – II
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After the completion of this course the student will be able to:
CO 82: Apply Maxwell’s equations to a variety of problems. CO 83: Solve problems involving the propagation and scattering of electromagnetic waves in a variety of media. CO 84: Acquire a good understanding of Special Relativity, especially as applied to electrodynamics. CO 85: Demonstrate an understanding of the characteristics of electromagnetic radiation by moving charges. CO 86: Develop understanding of the covariant formulation of electrodynamics and the concept of retarded time for charges undergoing acceleration |
Approach in teaching: Interactive Lectures, Discussion, Tutorials, , Demonstration, Problem Solving
Learning activities for the students: Self learning assignments, Effective questions, Seminar presentation, Solving numerical Additional learning through online videos and MOOC courses |
Class test, Semester end examinations, Quiz, Solving problems , Assignments, Presentations |
Plane wave in a non-conducting medium. Frequency dispersion characteristics of dielectrics, conductors and plasma, waves in a conducting or dissipative medium, superposition of waves in one dimension, group velocity, causalty, connection between D and E, Kramers-Kroning relation.
Introduction and definitions, MHD equations, Magnetic diffusion, viscosity and pressure, Pinch effect, instabilities in pinched plasma column, Magneto hydrodynamics wave, Plasma oscillations, short wave length limit of plasma oscillations and Debye shielding distance.
(a)Covariant Form of Electrodynamic Equations: Mathematical properties of the space-time special relativity, Invariance of electric charge, covariance of electrodynamics, Transformation of electromagnetic field.
(b) Thomson scattering and radiation, Scattering by quasi-free charges, coherent and incoherent scattering, Cherenkov radiation.
Solution of inhomogeneous wave equation by Fourier analysis; Lienard-Wiechert Potential for a point charge, Total power radiated by an accelerated charge, Larmour's formula and its relativistic generalization, Angular distribution of radiation emitted by an accelerated charge, Radiation emitted by a charge in arbitrary extremely relativistic motion.
Introductory considerations, Radiative reaction force from conservation of energy, Abraham Lorentz evaluation of the self force, difficulties with Abraham Lorentz model, Integro-differential equation of motion including radiation damping, Line Breadth and level shift of an oscillator, Scattering and absorption of radiation by an oscillator.