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Relativistic energy and momentum explain how motion changes when objects move at speeds close to the speed of light. This cheat sheet helps students connect classical mechanics to special relativity using the formulas most often needed in physics courses. It is useful for solving problems involving fast particles, particle accelerators, photons, and mass-energy conversion.

The reference emphasizes when to use each equation and how the quantities fit together.

Key Facts

  • The Lorentz factor is γ=11v2c2\gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}}, where vv is speed and cc is the speed of light.
  • Relativistic momentum is p=γmvp = \gamma mv, which approaches classical momentum p=mvp = mv when vcv \ll c.
  • Total relativistic energy is E=γmc2E = \gamma mc^2, including both rest energy and kinetic energy.
  • Rest energy is E0=mc2E_0 = mc^2, which is the energy an object has even when v=0v = 0.
  • Relativistic kinetic energy is K=(γ1)mc2K = (\gamma - 1)mc^2, not K=12mv2K = \frac{1}{2}mv^2 at high speeds.
  • The energy-momentum relation is E2=(pc)2+(mc2)2E^2 = (pc)^2 + (mc^2)^2, which works for massive particles and simplifies for photons.
  • For a photon with m=0m = 0, the energy-momentum relation becomes E=pcE = pc.
  • No object with nonzero rest mass can reach cc because γ\gamma increases without bound as vv approaches cc.

Vocabulary

Lorentz factor
The factor γ=11v2c2\gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} that measures how strongly relativistic effects appear at speed vv.
Rest energy
The energy E0=mc2E_0 = mc^2 stored in an object's mass when it is not moving relative to the observer.
Total energy
The full relativistic energy E=γmc2E = \gamma mc^2, equal to rest energy plus kinetic energy.
Relativistic momentum
The momentum p=γmvp = \gamma mv of an object moving at speed vv, including the effect of the Lorentz factor.
Invariant mass
The rest mass mm of an object, which is the same in all inertial reference frames.
Photon
A massless particle of light that travels at speed cc and has energy E=pcE = pc.

Common Mistakes to Avoid

  • Using K=12mv2K = \frac{1}{2}mv^2 for speeds near cc is wrong because classical kinetic energy only works well when vcv \ll c.
  • Forgetting that E=γmc2E = \gamma mc^2 is total energy is wrong because it includes rest energy, not just kinetic energy.
  • Treating mm as increasing with speed can be misleading because modern relativity usually keeps rest mass mm constant and puts speed effects in γ\gamma.
  • Setting v=cv = c for a massive particle is wrong because γ=11v2c2\gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} becomes undefined as vv reaches cc.
  • Using E=pcE = pc for every particle is wrong because E=pcE = pc applies directly to massless particles, while massive particles use E2=(pc)2+(mc2)2E^2 = (pc)^2 + (mc^2)^2.

Practice Questions

  1. 1 Find γ\gamma for a particle moving at v=0.80cv = 0.80c.
  2. 2 An electron has rest energy E0=0.511MeVE_0 = 0.511\,\text{MeV} and moves with γ=3.00\gamma = 3.00. Find its total energy EE and kinetic energy KK.
  3. 3 A particle has momentum p=4.0MeV/cp = 4.0\,\text{MeV}/c and rest energy mc2=3.0MeVmc^2 = 3.0\,\text{MeV}. Use E2=(pc)2+(mc2)2E^2 = (pc)^2 + (mc^2)^2 to find EE.
  4. 4 Explain why a spaceship with nonzero rest mass cannot be accelerated to exactly cc, even if energy is continually added.