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Relativistic Momentum & Dynamics

In special relativity, momentum is $\vec p=\gamma m\vec v$. The relativistic second law $\vec F=d\vec p/dt$ preserves causality — as $v\to c$, the momentum grows without bound, requiring infinite force and energy to reach $c$. This is why the speed of light is an absolute limit for massive objects.

Key Concepts

Relativistic Momentum
p=γmv\vec p=\gamma m\vec v. In the low-speed limit, γ1\gamma\to1 and pmv\vec p\to m\vec v. As vcv\to c, p|\vec p|\to\infty.
Relativistic Force
F=dp/dt\vec F=d\vec p/dt. This is Lorentz-covariant. Longitudinal force (FF_{||}) relates to γ3ma\gamma^3 m a_{||}; transverse force (FF_\perp) to γma\gamma m a_\perp — the effective mass is direction-dependent.
Speed Limit
For a massive particle, reaching v=cv=c requires infinite momentum (and energy). A constant force produces continuously decreasing acceleration as vcv\to c; the particle asymptotically approaches but never reaches cc.
Four-Momentum
pμ=(E/c,p)p^\mu=(E/c,\vec p). The invariant pμpμ=(mc)2p_\mu p^\mu=(mc)^2 gives the energy-momentum relation E2=(pc)2+(mc2)2E^2=(pc)^2+(mc^2)^2.

Key Equations

Relativistic momentum
p=γmv\vec{p} = \gamma m\vec{v}
Reduces to mv for v ≪ c; diverges as v → c.
Energy-momentum relation
E2=(pc)2+(mc2)2E^2 = (pc)^2 + (mc^2)^2
Invariant relation; for massless particles (photons), E = pc.
Kinetic energy
K=(γ1)mc2K = (\gamma - 1)mc^2
Relativistic KE; reduces to ½mv² for v ≪ c (to first order in β²).
Worked Example

Proton Momentum and Kinetic Energy

Problem

A proton (mpc2=938.3m_p c^2=938.3 MeV) moves at v=0.80cv=0.80c. Find its (a) relativistic momentum (in MeV/c) and (b) kinetic energy (in MeV).

Solution

γ=1/10.64=5/3=1.667\gamma=1/\sqrt{1-0.64}=5/3=1.667.

p=γmpv=53×938.3×0.80 MeV/c=53×750.6=1251 MeV/cp = \gamma m_p v = \frac{5}{3}\times938.3\times0.80\text{ MeV}/c = \frac{5}{3}\times750.6 = 1251\text{ MeV}/c
K=(γ1)mpc2=(1.6671)×938.3=0.667×938.3=625.8 MeVK = (\gamma-1)m_pc^2 = (1.667-1)\times938.3 = 0.667\times938.3 = 625.8\text{ MeV}
Answer p=1251p=1251 MeV/c, K=625.8K=625.8 MeV.
Practice

Exercises

7 problems
1 of 7

A proton (mpc2=938.3m_pc^2=938.3 MeV) moves at β=0.60\beta=0.60 (γ=1.25\gamma=1.25). Find its momentum pp (in MeV/c).

MeV/c
2 of 7

Same proton (β=0.60\beta=0.60, γ=1.25\gamma=1.25). Find its kinetic energy KK (in MeV).

MeV
3 of 7

An electron (mec2=0.511m_ec^2=0.511 MeV) moves at β=0.90\beta=0.90 (γ=2.294\gamma=2.294). Find its total energy E=γmec2E=\gamma m_ec^2 (in MeV).

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4 of 7

An electron has total energy E=1.00E=1.00 MeV. Find its momentum pp (in MeV/c). Use E2=(pc)2+(mec2)2E^2=(pc)^2+(m_ec^2)^2, mec2=0.511m_ec^2=0.511 MeV.

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5 of 7

A photon has energy E=2.0E=2.0 MeV. Find its momentum pp (in MeV/c). (Photons have m=0m=0, so E=pcE=pc.)

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6 of 7

Find the speed β=v/c\beta=v/c of a proton with kinetic energy K=938.3K=938.3 MeV (equal to its rest energy). γ=K/(mpc2)+1=2\gamma=K/(m_pc^2)+1=2. β=11/γ2\beta=\sqrt{1-1/\gamma^2}.

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7 of 7

Two particles of mass m=1.0m=1.0 GeV/c² collide head-on each at γ=10\gamma=10 (total Ecm=2γmc2E_{\rm cm}=2\gamma mc^2). Find the available center-of-mass energy (in GeV).

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Key Takeaways

  • Relativistic momentum p=γmv\vec p=\gamma m\vec v diverges as vcv\to c, making cc an unreachable speed limit for massive particles.
  • Kinetic energy K=(γ1)mc2K=(\gamma-1)mc^2 reduces to 12mv2\frac{1}{2}mv^2 at low speeds; at v=cv=c, KK\to\infty.
  • Energy-momentum invariant: E2(pc)2=(mc2)2E^2-(pc)^2=(mc^2)^2 — same in all frames.
  • Photons have m=0m=0 and E=pcE=pc; they always travel at cc and carry both energy and momentum.