Lecturer: David Quigley
Weighting: 10 CATS
This module studies Newtonian mechanics and special relativity emphasizing the conservation laws inherent in the theory. These have a wider domain of applicability than just classical mechanics (for example they also apply in quantum mechanics). The module looks in particular at the mechanics of oscillations and of rotating bodies.
Einstein pointed out that Newton's laws were inconsistent with the theory of light waves: in mechanics objects only move relative to each other, whereas light appears to move relative to nothing at all (the vacuum). Einstein realised that Newtonian mechanics itself was the problem. He proposed that the laws of classical mechanics had to be consistent with just two postulates, namely that the speed of light is a constant and that all frames of reference are equivalent. These postulates forced Einstein to reject previous ideas of space and time and led directly to the special theory of relativity.
To revise A-level classical mechanics and to develop the theory using vector notation and calculus. To introduce special relativity. To cover material required for future physics modules.
At the end of the module, you should be
- Able to solve F =d p /dt for a variety of simple cases;
- Familiar with the concepts of potential and kinetic energy;
- Able to recognise and solve the equations of forced and damped harmonic motion;
- Able to solve problems involving torque and angular momentum;
- Able to explain the transformation between inertial frames of reference (Lorentz transformation) and to work through illustrative problems.
Forces, interactions and Newton's Laws of Motion
Applying Newton's Laws - equilibrium, dynamics of particles, friction and dynamics of circular motion Work and kinetic energy.
Potential energy and energy conservation.
Conservation of momentum, elastic collisions, centre of mass
Rotation of rigid bodies - angular velocity and acceleration, Dynamics of rotational motion, conservation of angular momentum
Hooke's law, equation of motion for a mass attached to a spring on a frictionless plane. Solutions for shm. Energy in shm. The pendulum, departures from shm for large amplitude. Complex notation. Damping: critical and under-/over-damping. Forced oscillations.
Motion as seen by different observers. Galilean Transformation of Velocities. Inertial frames of reference
The Michelson Morley experiment. The universality of the speed of light. The meaning of simultaneity.
Einstein's postulates: Lorentz transformation, Inverse Lorentz transformation and invariants. Length Contraction and Time Dilation, Doppler Effect.
Einstein's energy and mass relation, energy and momentum of elementary particles.
Minkowski diagrams - graphical representation of past/present/future.
Commitment: 30 Lectures + 10 problems classes
Assessment: 2 hour examination
Recommended Text: H D Young and R A Freedman, University Physics, Pearson.
Leads from: A level Physics and Mathematics