Reading Time: < 1 minute
Table of Contents
ToggleRelativity: Time Dilation, Mass-Energy Equivalence, and Modern Applications
Fundamentals of Special Relativity
Einstein’s 1905 theory revolutionized our understanding of space-time by introducing two postulates:
- The laws of physics are identical in all inertial frames
- The speed of light (c ≈ 3×10⁸ m/s) is constant in all frames
Core Relativistic Effects
Time Dilation
Moving clocks run slower by factor γ (Lorentz factor):
Example: At 0.8c (γ=1.67), 1 Earth hour = 1.67 ship hours
Length Contraction
Objects contract along motion direction:
Mass-Energy Equivalence
Components:
- Rest energy: E₀=mc²
- Kinetic energy: K=(γ-1)mc²
Practical Applications
Global Positioning System
- Satellite clocks run 38μs/day faster due to velocity (SR)
- 45μs/day slower from gravitational time dilation (GR)
- Net correction: -7μs/day
Particle Physics
- LHC protons reach 0.999999991c (γ=7,000)
- Mass increases to 6,500× rest mass
Astrophysics
- Muons (τ=2.2μs) reach Earth’s surface due to γ≈9 at 0.994c
- Black hole event horizons demonstrate extreme spacetime curvature
Worked Example
Time Dilation at 0.8c:
Common Errors
- Using Newtonian kinetic energy (½mv²) at relativistic speeds
- Confusing proper time (Δt) and dilated time (Δt’)
- Misapplying length contraction perpendicular to motion
Practice Problems
- Calculate γ and time dilation for:
- 0.6c (γ=1.25)
- 0.99c (γ≈7.09)
- Compute the energy equivalent of 1μg mass (E≈90kJ)
- Explain how GPS requires both special and general relativity
Skinat Tuition | Excellence in SAT, GCSE, and A-Level Tutoring.