Table of Contents

Reference Frames

Course Overview

Individual observers describe physics using physical quantities defined with respect to their own reference frame, such as the relative velocity of an object (compared to that of the observer). Yet the physics itself is independent of the reference frame used to describe it. This key idea already had a substantial impact on Newtonian physics, but its most famous consequence is that it leads to Einstein's theory of special relativity. This course considers both of these aspects.

After a brief review of inertial frames in Newtonian physics, physics on a rotating Earth is described in terms of apparent centrifugal and Coriolis forces due to the use of rotating reference frames. The heart of the course is to then extend the use of multiple frames of reference from the Newtonian framework to Einstein's special theory of relativity. After first contrasting Galilean and Lorentz transformations, the underlying geometric ideas are emphasized and used to resolve the standard paradoxes. Finally, the beautiful unification of electricity and magnetism provided by special relativity is presented.

Course Goals

Sample Syllabi

Course Contents

Unit: Rotating Reference Frames

Reference Frames (40 minutes)

2-D Rotations (110 minutes)

3-D Rotations (160 minutes)

Motion Relative to Earth (40 minutes)

Unit: Special Relativity

Basics of Special Relativity (45 minutes)

Lorentz Transformations (95 minutes)

Spacetime Geometry (150 minutes)

Unit: Relativistic Mechanics

Relativistic Mechanics (50 minutes)

Relativistic Dynamics (150 minutes)

Unit: Relativistic Electromagnetism

Relativistic E&M (85 minutes)

Unit: Transition to General Relativity

Course Summary (10 minutes)

General Relativity (30 minutes)

Miscellaneous Topics (10 minutes)

Activities Included