
Optional unit · institution-dependent · Interactive lesson
Relativistic momentum and dynamics
Momentum earns its name by being conserved for every inertial observer, and Newton's mv stops doing that once velocities compose relativistically. Here you repair it with the particle's own clock, differentiate the result to find the γ³ that replaces F = ma, and watch a constant force push a speed towards c without ever getting there.
UPIII-08.08 · Lesson 8 of 9 in this unit. Position is not a completion score.Optional unit · institution-dependent. This modern-physics material is an introductory survey, not a complete course in relativity, quantum, atomic, nuclear or particle physics. Your university determines the required depth and assessment. Optional work is not a required completion gate.
Build the model
Keep the mass invariant and put the γ where the clock is.
The key idea
Relativistic momentum is the invariant mass times the rate of change of the frame's position coordinate with respect to the particle's own proper time, p = m dx/dτ = γmv, the one definition whose conservation holds in every inertial frame.
Example. An electron (m = 9.109 × 10⁻³¹ kg) at 0.800c has γ = 1.667, so p = γmv = 3.64 × 10⁻²² kg m s⁻¹, two thirds more than the Newtonian mv = 2.18 × 10⁻²² kg m s⁻¹.
The complete physical model and assumptions
Momentum is defined by a job, not a formula: it is the quantity whose total a collision leaves unchanged, in every inertial frame. Newton's mv did that job while velocities added by plain subtraction. Once they compose by the relativistic rule, a collision that balances Σmv in one frame fails to balance it in another: in a symmetric glancing collision watched from one ball's own frame, the other ball's transverse velocity arrives divided by γ and the Newtonian ledger no longer closes. The repair keeps the mass and the displacement and changes only the clock. Differentiate the lab position by the particle's own proper time, p = m dx/dτ = γmv, since dt/dτ = γ, and the conservation law is restored for every observer at once. The price is paid in dynamics. F = dp/dt survives, but γ depends on v, so a push along the motion has to raise γ as well as v and the result is F = γ³ma; a push across the motion leaves γ alone and gives F = γma. Under a constant force the momentum grows as Ft without limit while the speed climbs towards c and never arrives. The m in all of this is the invariant mass, the same number in every frame; no speed-dependent mass is needed, and none could serve both directions at once. The model covers one particle of fixed mass under a force measured in one inertial frame. Systems whose mass can change, and what the force does to energy, wait for the next topic.
1A conservation law has to survive a change of frame
Momentum is worth having only because its total is conserved, and a law of physics must hold for every inertial observer. Test Newton's mv on a collision built to be symmetric. Two identical balls, A and B, each of mass m. In frame S, A moves straight up the y-axis at speed u, glances off B and comes straight back down at u. B's own frame S′ moves along x at speed v relative to S, and in S′ the story is the mirror image: B moves straight down at u and rebounds straight up. Seen from S, B's velocity follows from the velocity transformation of the previous topics: uₓ = v and uy = −u/γ, with γ = 1/√(1 − v²/c²). Take v = 0.800c, so γ = 1.667 and B's transverse speed in S is only 0.600u. Newton's y-momentum in S before the collision is mu − 0.600μ = +0.400mu; afterwards both y-velocities have reversed, so it is −0.400mu. The total has changed by 0.800mu with no external force anywhere. Nothing about the collision is exotic; the mismatch comes entirely from how velocities transform. Either momentum conservation is not a law, or mv is not momentum.
2Differentiate the position by the particle's own clock
p = m dx/dt has three ingredients. The mass belongs to the particle. The displacement dx is what the motion does in the frame doing the measuring. The dt is the one dubious ingredient: a reading on the observer's clock, which another observer disputes. Replace it with the particle's proper time τ, which every frame agrees on, and p = m dx/dτ. Since dt/dτ = γ evaluated at the particle's own speed, this is p = γmv. Return to the collision. A's factor is γA = 1/√(1 − u²/c²). B's speed squared in S is v² + u²/γ² = v² + u²(1 − v²/c²), so 1 − vB²/c² = 1 − v²/c² − u²/c² + u²v²/c⁴ = (1 − v²/c²)(1 − u²/c²), which gives γB = γγA exactly. B's y-momentum is therefore γB m(u/γ) = γA μ, A's own value, up against down: the total is zero before and zero after, in S, in S′ and in every other inertial frame. The γ is not a factor bolted on to make the sums close. It is the conversion between the two clocks, and no other timekeeper would have transformed the same way. Nothing here uses energy; the next topic shows that γmc² does for energy what γmv has just done for momentum.
3Differentiate p, and F = ma splits in two
Keep F = dp/dt as the definition of force and differentiate p = γmv with m constant: F = m(γ dv/dt + v dγ/dt). The second term is the new physics. From γ = (1 − v²/c²)(−1/2), the chain rule gives dγ/dt = γ³(v/c²)(dv/dt), so for a push along the motion F = mγa(1 + γ²v²/c²) = γ³ma, using γ²β² = γ² − 1. For a push at right angles to the velocity the speed is unchanged to first order, dγ/dt = 0, and F = γma. The same force is γ² times more effective sideways than forwards. At 0.600c, γ = 1.250: a forward push produces a = F/(1.953m), a sideways one F/(1.250m). At 0.950c the two are F/(32.8m) and F/(3.20m). No single speed-dependent mass can be written into F = ma to reproduce both, which is why this course keeps m invariant and lets γ live inside p. The sideways law is the one that runs bending magnets: with F = qvB always perpendicular to v, qvB = γmv²/r gives r = γmv/(qB) = p/(qB), and the orbital frequency qB/(γm) falls with speed. A fixed-frequency cyclotron loses step with its protons once γ has grown by a few per cent.
4A constant force gives runaway momentum and a saturating speed
Integrate F = dp/dt for a constant force on a particle starting from rest: p = Ft, exact at every speed, with no γ anywhere in it. Relativity enters when you ask what speed that momentum represents. From γmv = Ft, γβ = Ft/(mc), and solving for β gives β = (Ft/mc)/√(1 + (Ft/mc)²). The natural time is t₁ = mc/F, when Newton would announce v = c. An electron in a uniform field of 1.00 MV m⁻¹ feels F = eE = 1.602 × 10⁻¹³ N, and its mc is 2.731 × 10⁻²² kg m s⁻¹, so t₁ = 1.70 ns. At t₁ the real speed is β = 1/√2 = 0.707; at 2t₁ it is 2/√5 = 0.894; at 10t₁, 17.0 ns into the flight, it is 10/√101 = 0.995. The momentum keeps to its straight line, 10mc after 17 ns and 100mc after 170 ns, while the speed flattens against c. The forward acceleration at 10t₁ is F/(γ³m) with γ = √101 = 10.05, so γ³ = 1015 and the electron is gaining speed at a thousandth of its starting rate. c is not a wall the electron hits. It is the asymptote of a curve whose slope the γ³ keeps stealing, and the momentum, which the force actually delivers, never notices.
5Check the limits, and know what the model leaves out
Expand for small speeds: p = γmv = mv(1 + ½β² + ⅜β⁴ + …). The fractional correction is ½β² at leading order, 0.1% at β = 0.045, 1% at β = 0.14 and 10% at β = 0.42, so mv is recovered exactly where it was ever tested. Every result above must pass the same check: γ³ma → ma as β → 0, and p = Ft gives v = Ft/m for t ≪ mc/F. Dimensions pass too, because γ is a pure number and γmv, γ³ma carry the units of mv and ma. Now the boundaries. The mass m is invariant: a proton at 0.950c is the same 1.673 × 10⁻²⁷ kg it was at rest, and a mass that grows with speed is simply the γ of p filed under the wrong symbol. The three-force F = dp/dt is measured in one frame and, unlike position and momentum, does not transform by a simple rule, so a force law must be applied in the frame where it is stated. And everything here is for a single particle whose mass does not change. A collision that absorbs kinetic energy, or a decay, changes the rest masses of the bodies taking part, and momentum can only be balanced there once energy has been brought into the ledger, which is the business of the next topic.
Key equations
Read the units, assumptions and limits before substituting.
Lorentz factor as a clock ratio
γ = dt/dτ = 1/√(1 − v²/c²)
Every γ in this lesson is the ratio of the frame's clock to the particle's own: 1.250 at 0.600c, 3.203 at 0.950c, and 1 as v → 0.
v the particle's speed in the frame, m s⁻¹; c = 2.998 × 10⁸ m s⁻¹; τ the particle's proper time, sRelativistic momentum
p = m dx/dτ = γmv
Timing the frame's displacement by the particle's clock is what makes a total conserved in one frame conserved in all of them.
m the invariant mass, kg, identical in every frame; p in kg m s⁻¹; v the velocity in that frame, m s⁻¹Force along the motion
F∥ = dp/dt = γ³ma
Speeding up means raising γ as well as v, so the inertia against a forward push is γ³m, not m and not γm.
F in N, a = dv/dt in m s⁻² along v; uses dγ/dt = γ³(v/c²)(dv/dt)Force across the motion
F⊥ = γma
For a charge in a magnetic field this gives r = γmv/(qB) = p/(qB): the orbit radius tracks p, and the cyclotron frequency falls as qB/(γm).
a the sideways (centripetal) acceleration in m s⁻², with |v| and hence γ momentarily unchangedConstant force from rest
p = Ftv = c(Ft/mc)/√(1 + (Ft/mc)²)
Momentum climbs linearly for ever; the speed it represents is 0.707c at t₁, 0.894c at 2t₁, and never reaches c.
F constant in N, t the frame time in s; t₁ = mc/F is the time at which Newton would have reached cLow-speed correspondence
p = mv(1 + ½β² + ⅜β⁴ + …)
The correction γ − 1 starts as ½β² and reaches 0.1% at β = 0.045, 1% at β = 0.14, and 10% only at β = 0.42, so Newton is recovered where he was tested.
β = v/c, dimensionless; the series is the binomial expansion of γ for β² < 1Interactive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Slide β up from 0 and watch B's arrow tilt: its transverse part shrinks by 1/γ, so Newton's two bars fall out of step while the γmv pair stay level. At β = 0.80 the Newtonian ledger is out by 0.40 of A's mv, at β = 0.95 by 0.69, and raising u changes the scale but never the balance.
Live results
- LORENTZ FACTOR γ(v)
- 1.250
- NEWTON |py| OF B
- 0.160 mc
- γmv |py| OF A
- 0.204 mc
- γmv |py| OF B
- 0.204 mc
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Speed of B's frame β = v/c: 0.60; Transverse speed u/c of each ball: 0.20
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
Students who have just met p = γmv tend to differentiate it as if γ were a constant and write F = γma for a push along the motion, or, equivalently, to picture a relativistic mass γm on which Newton's second law then acts. The missing step is dγ/dt = γ³(v/c²)(dv/dt): speeding up changes γ as well as v, and that extra term turns the γ into γ³. At 0.600c the mistake underestimates the force a given forward acceleration needs by a factor γ² = 1.56; at 0.950c by a factor 10.3. The same habit gets the sideways case right by accident, because there γ really does stay fixed, which is why the idea of a single speed-dependent mass survives as long as it does. Keep m invariant, keep γ inside p, and differentiate honestly.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
A cosmic-ray muon (m = 1.883 × 10⁻²⁸ kg) travels at 0.940c. Find its momentum, compare it with the Newtonian mv, and find the speed a Newtonian physicist would infer from p/m.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 4 steps revealed.
- β = 0.940 gives β² = 0.8836 and 1 − β² = 0.1164, so γ = 1/√0.1164 = 2.931.
- The speed is v = 0.940 × 2.998 × 10⁸ = 2.818 × 10⁸ m s⁻¹, so the Newtonian product is mv = 1.883 × 10⁻²⁸ × 2.818 × 10⁸ = 5.307 × 10⁻²⁰ kg m s⁻¹.
- Relativistic momentum: p = γmv = 2.931 × 5.307 × 10⁻²⁰ = 1.555 × 10⁻¹⁹ kg m s⁻¹. The whole excess is the factor γ, since m and v are unchanged.
- mv/p = 1/γ = 0.341, so the Newtonian value is 66% too low. Reading p/m as a speed gives γv = 2.931 × 0.940c = 2.755c = 8.26 × 10⁸ m s⁻¹, faster than light: momentum per unit mass stops being a speed as soon as γ differs from 1.
Answer. p = 1.56 × 10⁻¹⁹ kg m s⁻¹, which is 2.93 times the Newtonian 5.31 × 10⁻²⁰ kg m s⁻¹; p/m = 2.76c = 8.26 × 10⁸ m s⁻¹, so p/m cannot be read as a speed.
MediumExample 2
A proton (m = 1.673 × 10⁻²⁷ kg) moving at 0.600c is pushed by a constant force of 8.00 × 10⁻¹³ N along its velocity. Find (a) its acceleration at that instant, compared with F/m and with F/(γm), and (b) the time the force takes to bring it to 0.900c, compared with Newton's prediction.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- γ₁ = 1/√(1 − 0.360) = 1.250, so γ₁³ = 1.953. The Newtonian benchmark is F/m = 8.00 × 10⁻¹³ ÷ 1.673 × 10⁻²⁷ = 4.782 × 10¹⁴ m s⁻².
- (a) Along the motion the force must raise γ too, so F = γ³ma and a = 4.782 × 10¹⁴ ÷ 1.953 = 2.448 × 10¹⁴ m s⁻². The relativistic-mass guess F/(γm) = 3.825 × 10¹⁴ m s⁻² is too high by γ² = 1.56.
- (b) F = dp/dt with F constant gives Δp = FΔt exactly. In units of mc = 1.673 × 10⁻²⁷ × 2.998 × 10⁸ = 5.016 × 10⁻¹⁹ kg m s⁻¹: γ₁β₁ = 1.250 × 0.600 = 0.750, and at 0.900c γ₂ = 1/√(1 − 0.810) = 2.294, so γ₂β₂ = 2.065. Δp = 5.016 × 10⁻¹⁹ × (2.065 − 0.750) = 6.594 × 10⁻¹⁹ kg m s⁻¹.
- Δt = Δp/F = 6.594 × 10⁻¹⁹ ÷ 8.00 × 10⁻¹³ = 8.24 × 10⁻⁷ s = 0.824 μs.
- Newton: Δv = 0.300c = 8.994 × 10⁷ m s⁻¹ and Δt = mΔv/F = 1.673 × 10⁻²⁷ × 8.994 × 10⁷ ÷ 8.00 × 10⁻¹³ = 1.88 × 10⁻⁷ s = 0.188 μs. The real flight takes 4.38 times longer, and on arrival at 0.900c the same force yields only F/(γ₂³m) = 4.782 × 10¹⁴ ÷ 12.07 = 3.96 × 10¹³ m s⁻².
Answer. (a) a = 2.45 × 10¹⁴ m s⁻², against F/m = 4.78 × 10¹⁴ m s⁻² and F/(γm) = 3.83 × 10¹⁴ m s⁻². (b) Δt = 0.824 μs, 4.4 times Newton's 0.188 μs.
HardExample 3
An electron (m = 9.109 × 10⁻³¹ kg, e = 1.602 × 10⁻¹⁹ C) is released from rest in a uniform electric field of 1.50 MV m⁻¹. Find (a) the time to reach 0.950c, (b) the distance covered in that time by integrating v(t), and (c) the speed and distance Newton would assign to the same time.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- F = eE = 1.602 × 10⁻¹⁹ × 1.50 × 10⁶ = 2.403 × 10⁻¹³ N, constant, so p = Ft exactly. With mc = 9.109 × 10⁻³¹ × 2.998 × 10⁸ = 2.731 × 10⁻²² kg m s⁻¹, the Newtonian light-speed time is t₁ = mc/F = 1.136 ns.
- (a) At 0.950c, γ = 1/√(1 − 0.9025) = 3.203 and γβ = 3.042. Setting γβ = t/t₁ gives t = 3.042 × 1.136 ns = 3.46 ns.
- (b) v(t) = c s/√(1 + s²) with s = t/t₁. Then x = ∫₀ᵗ v dt = c t₁ ∫₀ˢ s ds/√(1 + s²) = c t₁ [√(1 + s²) − 1]. At the end √(1 + s²) = γ, so x = c t₁(γ − 1).
- c t₁ = 2.998 × 10⁸ × 1.1364 × 10⁻⁹ = 0.3407 m, so x = 0.3407 × (3.2026 − 1) = 0.3407 × 2.2026 = 0.750 m.
- (c) Newton: v = (F/m)t = 2.638 × 10¹⁷ × 3.458 × 10⁻⁹ = 9.12 × 10⁸ m s⁻¹ = 3.04c, and x = ½(F/m)t² = 0.5 × 2.638 × 10¹⁷ × (3.458 × 10⁻⁹)² = 1.58 m, 2.1 times the true distance.
- Checks: for s ≪ 1, √(1 + s²) − 1 → ½s², so x → ½ c t₁ s² = ½(F/m)t², which is Newton; and c t₁ = mc²/F has units J N⁻¹ = m, a length.
Answer. (a) 3.46 ns; (b) 0.750 m; (c) Newton would claim 3.04c and 1.58 m, twice the real distance at a speed the electron never reaches.
Quick check
Select an answer and explain it before checking.
Review & continue
Relativistic momentum is the invariant mass times the rate of change of the frame's position coordinate with respect to the particle's own proper time, p = m dx/dτ = γmv, the one definition whose conservation holds in every inertial frame.
- Explain the relationship without looking at the equation.
- Check a sign, a unit and a model assumption in your working.
- Return to the lab or worked example if a step is still unclear.
Optional supporting lessons
These chapter resources can help with earlier ideas; they are not additional required Physics III completion tasks.