Requirements/prerequisites:
prerequisite: MA2342
Duration: Michaelmas term, 11 weeks
Number of lectures per week: 3 lectures including tutorials per week
Assessment: Assignments will not contribute formally to the final result
except in bordeline cases.
ECTS credits: 5
End-of-year Examination:
This module will be examined jointly with MA3432
in a 3-hour examination in Trinity term,
except that those taking just one of the
two modules will have a 2 hour examination.
However there will be separate results for MA3431 and MA3432.
Description: Rationale and Aims The purpose of Module MA3431 is to outline the properties of a classical field theory that relate in particular to scalar and vector fields, to point out features of the tensor calculus suitable for the description of relativistic non-quantum field theories, and to indicate the importance of symmetry and invariance principles in the development of conservation laws for energy, momentum and other conserved quantities.
The module is mandatory for third year undergraduate students of theoretical physics but may optionally be taken by third or fourth year undergraduate students of mathematics. Postgraduate students from other institutions have taken the module in the past. The module forms an element of the undergraduate programme in theoretical physics being built upon prerequisite first and second year courses in classical dynamics and mathematics and leading to courses in the fourth and final year including quantum field theory.
From a teaching point of view, the intention of the lecturer is to indicate how powerful analytical and formal methods can be invoked to understand and solve many problems in mathematical physics. A further intention is to provide a sense of the important rôle played by field theories, particularly electrodynamics, in the development of theoretical physics and its applications.
Content
Classical Lagrangian for a discrete system, Lagrangian density for a field
Indicative textbooks:
Classical Electrodynamics, J. David Jackson, John Wiley (3rd edition) 1998
describe how to find the equation of motion for a scalar field using a given Lagrangian density