Relativistic Kinetic Energy
Also known as: Relativistic KE · SR Kinetic Energy
Kinetic energy is the extra energy a body gains by moving — it diverges as v approaches c, not 1/2 mv^2.
K = (γ−1)mc²; curve diverges near c, sweeping marker.
Equivalent forms
Reduces to (1/2)mv^2 at low speeds yet diverges at the speed of light — both Newtonian and Einsteinian limits in one expression.
Unit systems
Where it holds
Dimensional analysis
Derived from Einstein's special relativity by subtracting rest energy from total relativistic energy gamma m c^2.
Why does it take more than 938 MeV to accelerate a proton to 0.99c?
Classical KE = (1/2)mv^2 underestimates true energy at high speeds. Use K = (gamma - 1)mc^2 with gamma ≈ 7.09 at v = 0.99c → K ≈ 6.09 * 938 MeV ≈ 5.71 GeV.
- LHC beam energy calibration
- Medical proton therapy protons)
- Cosmic-ray air shower modeling
- Free-electron laser design
- K is NOT (1/2) gamma m v^2 — that expression is wrong
- K and rest energy mc^2 are separate; total energy is their sum
- There is no upper limit on K, only on v
Limiting cases
What if…
(1/2) m v^2 gives — off by a factor of 3.2x; underestimates by 67%.
Doubling K increases gamma roughly linearly when gamma ≫ 1, but v changes negligibly — we trade energy for relativistic mass.
— the particle carries 999 times its rest energy as kinetic energy.
Electron at 0.9c
- m:
- 9.1093837015e-31
- v:
- 269813212
- ,
Proton in LHC
- m:
- 1.67262192369e-27
- v:
- 299792455
- (from LHC design energy 7 TeV)