A5-1. Special Relativity: Reference Frames and Galilean RelativityHL ONLY
1. Reference Frames
In physics, motion is entirely relative. To measure velocity, displacement, or time, we must first establish a point of view. A reference frame (or frame of reference) is a set of coordinates used to record the position and time of events.
Inertial vs. Non-Inertial Frames:
- Inertial Reference Frame: A frame of reference that is either entirely completely at rest or moving at a constant velocity. In an inertial frame, Newton's First Law holds true (an object at rest stays at rest unless acted upon by a force). There is no "fictitious" acceleration.
- Non-Inertial Reference Frame: A frame of reference that is accelerating or rotating. In these frames, objects appear to accelerate without a physical force acting on them (e.g., being pushed back into your seat when a car accelerates).
Special relativity deals exclusively with inertial reference frames.
2. Galilean Relativity & Transformations
Before Einstein, classical mechanics relied on Galilean relativity. Galileo proposed that the fundamental laws of mechanics are identical in all inertial reference frames. If you are in a train moving at a perfectly constant velocity, tossing a ball straight up looks exactly the same as if you were standing on the ground.
Galilean Transformation Equations:
Suppose Frame $S'$ is moving at a constant velocity $v$ relative to a stationary Frame $S$ along the x-axis. For an event occurring at position $x$ and time $t$, Galilean transformations allow us to translate coordinates between the frames:
- $x, x'$: Position of the event in Frame S and Frame S'.
- $u, u'$: Velocity of an object in Frame S and Frame S'.
- $v$: Relative velocity between the two frames.
- $t, t'$: Time. Crucially, in Galilean relativity, time is absolute. It flows at the exact same rate for all observers everywhere ($t' = t$).
Example 1: Galilean Velocity Addition
Problem: A train (Frame S') is moving right at $v = 20\text{ m/s}$ relative to the ground (Frame S). A passenger on the train throws a ball forward at $u' = 5\text{ m/s}$ relative to the train. What is the velocity of the ball ($u$) relative to an observer standing on the ground?
Solution:
- Using the Galilean velocity transformation: $u' = u - v$
- Rearranging for $u$: $u = u' + v$
- $u = 5\text{ m/s} + 20\text{ m/s} = \mathbf{25\text{ m/s}}$
- Insight: This simple addition perfectly describes classical mechanics, but it critically fails when speeds approach the speed of light.