Relativistic Momentum Calculator
Momentum, kinetic energy and the energy-momentum relation at relativistic speeds
Momentum and Kinetic Energy at Relativistic Speeds
Momentum is still mass times velocity, but with the Lorentz factor attached:
- — momentum, kg·m/s (or MeV/c in particle physics)
- — invariant rest mass, kg
- — speed in the observer's frame, m/s; m/s
Kinetic energy is not with a bolted on. It is the total energy minus the rest energy:
both in joules, or in MeV if you use in MeV.
When it applies: any inertial frame, any speed. Both formulas reduce to the Newtonian ones as — expand and falls out.
The assumption people forget: diverges as , which is the real content of the speed limit. A photon has but still carries momentum , because is an indeterminate form, not a zero.
The Energy-Momentum Relation
Eliminating between and gives the single most useful identity in relativistic mechanics:
Every term is an energy, so work in eV throughout: J, MeV, MeV. Momentum then comes out in MeV/c, which is a perfectly good unit — divide by only if the question wants SI.
The relation is frame-independent: and both change between frames, but is always . Two consequences worth memorising:
Those two let you recover speed and Lorentz factor from an energy measurement without ever touching a square root of .
The assumption people forget: here is the total energy, not the kinetic energy. Substituting for is the single most common error on this topic.
Common Mistakes to Avoid
- Using above about — at the classical value is twelve times too small.
- Putting into — that slot takes total energy, .
- Writing but forgetting to square — at the denominator is , not .
- Mixing MeV with kg·m/s mid-line — pick natural units or SI and convert only at the end.
- Treating as the mass in every formula — it works for by coincidence and fails for , where is simply wrong.
- Assuming momentum caps out — energy and momentum both grow without bound; only is bounded by .
Examples
Frequently Asked Questions
p = γmv, where γ = 1/√(1 − v²/c²) and m is the invariant rest mass. In SI the answer is in kg·m/s; particle physicists usually quote it in MeV/c, obtained from pc = γmc²β.
K = (γ − 1)mc², the total energy γmc² minus the rest energy mc². It is not ½mv² with a gamma attached, and it is not ½γmv² either. As v becomes small, γ ≈ 1 + ½β² and the formula reduces correctly to ½mv².
Roughly above 0.1c, where γ = 1.005 and the error is half a percent. By 0.5c the classical value is 13 percent low, and at 0.9c it is off by a factor of 2.3. In accelerator or cosmic-ray problems, always use the relativistic form.
Use β = v/c = pc/E, with both in the same energy units. Equivalently γ = E/mc², then β = √(1 − 1/γ²). Both routes avoid recomputing the Lorentz factor from the speed.
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