Evidence for relativity and mass–energy consequences
Key ideas
- Special relativity makes testable predictions. The classic piece of evidence at this level is the muon decay problem.
- Muons are unstable particles created high in the atmosphere (around km up) by cosmic rays, travelling toward Earth at close to (typically around ).
- A muon's average lifetime, measured at rest (its proper time), is only about .
- Classically, in even light travels only m — nowhere near far enough for most muons to reach the ground before decaying.
- Observation: large numbers of these muons ARE detected at sea level.
- Relativity resolves this two equivalent ways:
- From Earth's frame: the muon's clock is moving, so time dilation means Earth observers measure the muon's lifetime as longer than (by a factor of ) — long enough for the muon to cover the km.
- From the muon's frame: the muon's own lifetime is still (its proper time), but the km distance to the ground is length-contracted (by the same factor of ) to a much shorter distance — one the muon can cross in its own short lifetime.
- Both explanations use the same and give the same physical outcome: more muons survive to reach the ground than classical physics predicts.
- This agreement between two very different-looking explanations (one using time dilation, one using length contraction) is strong evidence that special relativity, not classical mechanics, correctly describes fast-moving particles.
Mass–energy consequences (qualitative)
- Special relativity also connects mass and energy. As an object's speed increases toward , more and more of the energy put into accelerating it appears as an increase in its relativistic mass/energy, not as speed.
- This is why no object with mass can reach or exceed : as , , so an infinite amount of energy would be required.
- It means mass and energy are equivalent — mass is a form of stored energy, related by (covered fully in the nuclear physics section of this standard).
- These consequences are why particle accelerators can push particles very close to , but never all the way to it.
Tips
- State both explanations, and say they agree. A common Merit/Excellence question is "explain the muon observation from Earth's frame AND the muon's frame" — full marks need both frames explained, plus the point that they predict the same outcome.
- Do not say "the muon's own clock speeds up" or "the muon shrinks" — nothing changes in the muon's own frame. It is other observers who measure it differently. Keep straight whose measurement is being described.
Test yourself
Practice by grade
One question each at Achieved, Merit and Excellence. Have a go, then compare with the model answer.
Achieved
A muon has a proper lifetime of and travels at , giving .
Calculate the muon's lifetime as measured by an observer on Earth.
Merit
A muon travels at () toward the ground, m away as measured from Earth.
Calculate the distance to the ground as measured in the muon's own frame, and hence show it is plausible for the muon to survive the trip given its proper lifetime of .
Excellence
Explain, using both the Earth frame and the muon's frame, why more muons reach the ground than classical physics predicts, and explain why the two explanations must give the same result.