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F. Revolutions in Modern Physics: Quantum Mechanics and Special Relativity · Special Relativity

Special Relativity: Unit Review

F1.1 F1.2 F2.1 F2.3 F2.4 F3 A1.6 A1.8 A1.10 A1.12 A1.13 A2.1About 40 minutes
Learning goals
  • I can explain the postulates of special relativity and the evidence for them.
  • I can solve problems with time dilation, length contraction, velocity addition, momentum and energy.
  • I can assess technologies that depend on relativity and explain how relativity changed scientific thinking.

Words to know

proper time
Time between two events measured by a clock present at both.
proper length
Length measured in the frame where the object is at rest.
Lorentz factor
γ = 1/√(1 − v²/c²) ≥ 1.
rest energy
E₀ = mc².

Let's review!

In this unit you followed one of the great revolutions in physics. You started with frames of reference and the Galilean picture of absolute time, saw the crisis caused by the speed of light and the Michelson–Morley null result, and met Einstein's two postulates. From them you derived the relativity of simultaneity, time dilation and length contraction, resolved the twin paradox with spacetime diagrams, and learned how velocities add near c. You redefined momentum and energy (p = γmv, E = γmc²), used E = mc² for nuclear energy and antimatter, analysed the evidence (muons, atomic clocks, accelerators) and assessed technologies such as GPS, accelerators, PET and nuclear power.

This review has a few questions from every lesson. Try each one, then press Show answer to check. The sibling unit Quantum Mechanics completes strand F.

How to use this review

Work through one or two sections at a time, with a scientific calculator. For every problem, first name the two events and decide which frame measures the proper time or proper length. Keep at least four significant figures in γ, and round only the final answer. Use units of c for speeds in velocity-addition problems and MeV for particle energies. For each question you miss, write down why (wrong proper time? forgot the square root? sign error?) and go back to that lesson. Finish with the 10-question quiz.

Frames and etherlessons 1, 2Two postulateslesson 3Simultaneitylesson 4Time dilationlessons 5, 6 (evidence)Length contractionlesson 7Twins, spacetimelesson 8Velocity additionlesson 9p = γmv, E = γmc²lessons 10, 11Nuclear, GPS, societylessons 12, 13
How the ideas in this unit connect (read across, then down). The two postulates, with the relativity of simultaneity, lead to time dilation, length contraction and spacetime, and from there to new rules for velocity, momentum and energy, and the technologies that use them.
Lorentz factorγ = 1/√(1 − v²/c²)Time dilationΔt = γΔt₀ (Δt₀: clock present at both events)Length contractionL = L₀/γ (L₀: measured at rest)Intervals² = (cΔt)² − (Δx)²Velocity additionu = (u′ + v)/(1 + u′v/c²)Momentump = γmvEnergyE = γmc², Ek = (γ − 1)mc², E² = (pc)² + (mc²)²Units1 u = 931.5 MeV/c², 1 eV = 1.602 × 10⁻¹⁹ J
The key equations of the unit. Use c = 3.00 × 10⁸ m/s.

Frames of Reference and Galilean Relativity

1

A train moves at 30 m/s east. A passenger walks west at 2.0 m/s relative to the train. Find the passenger's velocity relative to the ground (Galilean).

2

Is a car turning a corner at constant speed an inertial frame? Explain.

3

Why did Maxwell's prediction of c create a problem for Galilean relativity?

The Ether and the Michelson–Morley Experiment

1

What did Michelson and Morley expect to see when they rotated their interferometer, and what did they see?

2

A boat moving at 3.0 m/s relative to water crosses a river with a 1.0 m/s current, 60 m across and back. How long does it take?

3

Why is the null result considered strong evidence, not a failed experiment?

Einstein's Two Postulates and the Power of Thought Experiments

1

State both postulates.

2

A spaceship moving at 0.70c fires a laser backward. What speed does Earth measure for the light?

3

Describe one thought experiment Einstein used and what it suggested.

The Relativity of Simultaneity

1

Lightning strikes both ends of a train simultaneously in the ground frame. The train moves toward the front strike. Which strike happens first for a passenger?

2

A centre lamp flashes in a car 20 m long (ground measurement) moving at 0.60c. When does light reach each door in the ground frame?

3

Can observers disagree about the order of a cause and its effect? Explain.

Time Dilation: Moving Clocks Run Slow

1

Calculate γ for v = 0.95c.

2

A ship moves at 0.95c. The crew measures 2.0 years for a task. How long does Earth measure?

3

Earth measures 30 years for a round trip at 0.99c. How much does the traveller age?

4

By how much does a clock moving at 300 m/s fall behind in 1.0 day?

Evidence for Time Dilation: Muons, Atomic Clocks and Accelerators

1

Muons travel 4.5 km at 0.99c. Using a half-life of 1.52 µs, find the surviving fraction without and with time dilation.

2

In the Hafele–Keating experiment, which direction of flight made the clocks lose time, and why?

3

A lab measures 410 ± 20 muons per hour; theory predicts 420. Do they agree?

Length Contraction

1

A 50 m spaceship passes Earth at 0.80c. What length does Earth measure?

2

A star is 6.0 ly away (Earth frame). How far is it for a crew travelling at 0.60c, and how long is the trip for them?

3

Who measures the proper length of a racetrack: a spectator in the stands or a driver on the track?

The Twin Paradox and Spacetime Diagrams

1

Two events: cΔt = 13 ly, Δx = 5.0 ly. Find the proper time between them.

2

A twin travels at 0.80c to a star 4.0 ly away and back. Find the ages added to each twin.

3

Why is the twin situation not symmetric?

Adding Velocities Near the Speed of Light

1

A ship at 0.70c launches a probe forward at 0.70c relative to the ship. Find the probe's speed relative to Earth.

2

A ship at 0.90c fires a probe backward at 0.50c relative to it. Find the probe's velocity relative to Earth.

3

Show that if u′ = c, then u = c.

Relativistic Momentum and the Cosmic Speed Limit

1

Find the momentum of a proton (1.67 × 10⁻²⁷ kg) at 0.90c.

2

At what speed is p = 3mv?

3

Why can't any amount of force push an object to c?

Mass–Energy Equivalence: E = mc², Total Energy and Kinetic Energy

1

Find the rest energy of 1.0 g in joules.

2

An electron has kinetic energy 1.533 MeV. Find γ and v.

3

A proton has total energy 1876 MeV. Find pc.

4

Why is ½mv² wrong for a particle at 0.9c?

Mass–Energy at Work: Binding Energy, Nuclear Power and Antimatter

1

A mass defect of 0.0500 u corresponds to how much energy?

2

Why does fission of uranium release energy?

3

What is produced when an electron and positron annihilate at rest?

Relativity in Technology and Society

1

Give the two relativistic effects on GPS clocks and their approximate sizes.

2

Name two other technologies that depend on relativity.

3

State one benefit and one risk of nuclear power.

Just for fun

Review-day riddle: what do a muon, a GPS satellite and a twin coming home from space all have in common?

They all have time on their side, just not the same amount of it.

Check your understanding

Quiz

1.

Which is Einstein's second postulate?

2.

What did the Michelson–Morley experiment find?

3.

A clock moves at 0.80c. One hour passes on it. How long is that in the stationary frame?

4.

A 100 m spacecraft moves at 0.60c. What length does Earth measure?

5.

Which measurement is a proper time?

6.

Two ships approach each other, each at 0.50c relative to Earth. What is their relative speed?

7.

An electron (0.511 MeV) has total energy 1.022 MeV. What is its speed?

8.

Why do cosmic-ray muons reach sea level in large numbers?

9.

What is the net daily effect of relativity on a GPS satellite clock?

10.

Between two events, which worldline has the greatest proper time?

For parents and teachers

How to use this review at home: Your teen should work through the sections, then do the quiz. Use mistakes to decide what to revisit:

  • Sign errors or confusion about who measures what speed: lesson 1 (Frames of Reference) and lesson 9 (Adding Velocities).
  • Can't explain the ether or the null result: lesson 2.
  • Unsure of the postulates or uses Galilean addition for light: lesson 3.
  • Confused about which event happens first: lesson 4 (Simultaneity).
  • Swaps Δt and Δt₀, or multiplies when they should divide: lesson 5 (Time Dilation) and lesson 7 (Length Contraction). The key question is always 'which clock is present at both events?' or 'in which frame is the object at rest?'
  • Half-life or uncertainty mistakes in evidence questions: lesson 6.
  • Spacetime interval or twin errors: lesson 8.
  • Momentum or energy formula errors (½mv² at high speed, missing γ): lessons 10 and 11.
  • Mass-defect errors (rounding before subtracting): lesson 12.
  • Weak assessments of technology (one-sided, no evidence): lesson 13.

Most errors in this unit come from the calculator (forgetting the square root in γ, or squaring 3.00 × 10⁸ incorrectly). Ask your teen to compute γ for 0.60c (it should be exactly 1.25) as a quick check.