## Pre-requisite modules

- None

## Co-requisite modules

- None

## Prohibited combinations

Occurrence | Teaching cycle |
---|---|

A | Autumn Term 2018-19 |

Classical mechanics is one of the cornerstones of physics. It provides methods for calculating the position, velocity, acceleration and other properties of the motion of point particles and extended bodies as function of time, if the forces acting are known. Classical mechanics is an important subject in its own right but it also forms the basis of several other branches of physical science; indeed many of the ideas incorporated in quantum theory have their origin in classical mechanics. This module commences with the study of translational motion in systems containing one or fewparticles. It then deals with rotational motion. Some of the central concepts of physics – such as momentum, force, energy, work, angular momentum and key conservation laws will be introduced. This module then expands on this classical material to provide an introduction to the ideas and concepts of Einstein’s special theory of relativity.

**At the end of this module successful students will be able to:**

- Apply dimensional homogeneity and dimensional analysis to simple physical systems.
- Explain and discuss the central concepts of classical mechanics, including force, energy, work, momentum, moments of inertia, torque and angular momentum
- Define inertial and non-inertial frames of reference
- Derive the key results presented in lectures
- Apply these results to seen and unseen physical situations by using them to set up a mathematical model and to find quantitative solutions
- Discuss qualitatively the limitations of classical mechanics
- Discuss the concepts and ideas that led to the theory of special relativity
- State Einstein’s two postulates of Special Relativity
- State the Lorentz transformation and apply it to simple problems
- Solve simple problems concerning the way that time is dilated and length contracted when clocks and objects are seen in uniform motion relative to an observer
- Describe and apply the relativistic Doppler effect
- Solve elementary problems involving objects moving at relativistic velocities

**Syllabus**

__Newtonian mechanics__

- Dimensions: Dimensional homogeneity and dimensional analysis
- One-dimensional kinematics: displacement, instantaneous/average velocity and acceleration, motion under constant acceleration and free-fall.
- Two-dimensional kinematics: position-, velocity- and acceleration-vectors, resolving into components, projectile motion, relative velocity in one and two dimensions.
- Circular motion: angular frequency, centripetal acceleration and uniform circular motion.
- Forces and Newton’s Laws: fundamental forces and interactions, Newton’s laws of motion and their applications, free-body diagrams, reaction forces, static and kinetic friction, dynamics of circular motion.
- Work and energy: definition of work, sign of work, the work-energy theorem, work with a constant force, work with a variable force, power, conservative forces, work and potential energy, force and potential energy.
- Momentum and collisions: Momentum and impulse, conservation of momentum, elastic and inelastic collisions, centre of mass, rocket propulsion.
- Rotational kinematics: Angular velocity and acceleration, comparison with linear motion, energy and rotation, moments of inertia, calculation of moments of inertia for simple systems,perpendicular and parallel axis theorems and their derivation.
- Rotational dynamics: Angular momentum, torque, relationship between torque & angular momentum & angular velocity & angular acceleration, conservation of angular momentum and its consequences, dynamics of simple systems with rotational and translational motion, Coriolis and centrifugal forces.

__Special relativity__

- Ideas and thoughts that lead to the special theory of relativity
- Inertial frames of reference
- Einsteins postulates of special relativity
- Spacetime
- Events; simultaneous events
- Time dilation; proper time
- Length contraction; proper length
- Lorentz transformation; examples and consequences
- Relativistic addition of velocities
- Relativistic Doppler shift for electromagnetic radiation
- Relativistic definitions of linear momentum and energy
- New units e.g. mass in terms of MeV/c2, linear momentum in terms of MeV/c
- Relativistic total energy and rest energy (E=mc2)
- Conservation laws for relativistic (total) energy and momentum

Task | Length | % of module mark |
---|---|---|

Essay/courseworkPhysics Practice Questions |
N/A | 14 |

University - closed examinationNewtonian & Relativistic Mechanics |
3 hours | 86 |

None

Task | Length | % of module mark |
---|---|---|

University - closed examinationNewtonian & Relativistic Mechanics |
3 hours | 86 |

**Physics Practice Questions (PPQs) -** You will receive the marked scripts either in problem classes orvia your pigeon holes. Feedback solutions will be provided on the VLE or by other equivalent means from your lecturer. As feedback solutions are provided, normally detailed comments will not be written on your returned work, although markers will indicate where you have lost marks or made mistakes. You should use your returned scripts in conjunction with the feedback solutions.

**Exams -** You will receive the marks for the individual exams from eVision. Detailed model answers will be provided on the intranet. You should discuss your performance with your supervisor.

**Advice on academic progress - **Individual meetings with supervisor will take place where you can discuss your academic progress in detail.

H D Young and R A Freedman:* University Physics with Modern Physics* ****

*The Feynman Lectures on Physics: Volume 1 *(Addison Wesley) **

K S Krane: *Modern Physics* ***

A.P. French: *Special Relativity* **