Spacetime diagram with light cones illustrating relativistic physics

Relativistic momentum

PHYS 401 · Relativistic Dynamics

Relativistic momentum preserves conservation laws in all inertial frames. This lesson introduces $ ec{p}=gamma m ec{v}$ and compares it with classical momentum.

Key equations

ec{p}=m ec{v} ec{p}=gamma m ec{v}gamma= rac{1}{sqrt{1-v^2/c^2}} ec{p}approx m ec{v}lim*{v o c}gamma=infty ec{F}= rac{d ec{p}}{dt} ec{p}*{total}=sum_i gamma_i m_i ec{v}*i ec{p}*{initial}= ec{p}*{final}m*{rel}=gamma m

Learning objectives

  • Define relativistic momentum.
  • Show that classical momentum is the low-speed limit.
  • Explain why momentum grows without bound near $c$.
  • Use $ ec{F}=d ec{p}/dt$ as the relativistic form of Newton's second law.
  • Explain why modern treatments avoid relativistic mass.

Why momentum must change

Classical momentum is

ec{p}=m ec{v}

This works at low speeds, but it is not compatible with Lorentz transformations and conservation laws at speeds near cc. Special relativity requires a momentum definition that is conserved in isolated systems for all inertial observers.

The relativistic momentum of a particle with rest mass mm and velocity ec{v} is

ec{p}=gamma m ec{v}

where

gamma= rac{1}{sqrt{1-v^2/c^2}}

Low-speed limit

When vllcvll c, gammaapprox1gammaapprox1, so relativistic momentum becomes

ec{p}approx m ec{v}

Thus classical momentum is the low-speed approximation to relativistic momentum.

Growth near light speed

As vv approaches cc, the Lorentz factor gammagamma grows without bound. Therefore momentum grows without bound even though speed approaches a maximum:

limvocgamma=inftylim*{v o c}gamma=infty

This is one reason a massive particle cannot be accelerated to light speed. More and more momentum and energy are required for smaller and smaller increases in speed.

Force and momentum

Newton's second law is best written in relativity as

ec{F}= rac{d ec{p}}{dt}

not simply ec{F}=m ec{a}. Because ec{p}=gamma m ec{v}, force and acceleration are not always parallel in the same simple way as in classical mechanics, especially when forces have components parallel and perpendicular to motion.

Conservation of momentum

Relativistic momentum is designed so that total momentum is conserved in isolated collisions:

ec{p}*{total}=sum_i gamma_i m_i ec{v}*i

For an isolated system,

ec{p}*{initial}= ec{p}*{final}

This conservation holds across inertial frames when energy is also treated relativistically.

Particle accelerators

In particle accelerators, particles can reach speeds extremely close to cc. Adding energy mostly increases gammagamma and momentum, not speed. This is why accelerator physicists often describe beams by energy or momentum rather than speed.

An electron at very high energy may move at 0.999999c0.999999c, and doubling its energy changes speed only slightly.

Relativistic mass caution

Older treatments sometimes define relativistic mass as mrel=gammamm*{rel}=gamma m. Modern physics usually avoids this language and keeps rest mass mm invariant, placing the factor gammagamma in momentum and energy. This avoids confusion and supports four-vector notation.

The big idea

Relativistic momentum is ec{p}=gamma m ec{v}. It reduces to classical momentum at low speeds but grows dramatically near light speed. This definition preserves momentum conservation in special relativity and leads naturally to relativistic energy and four-momentum.

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