
Relativistic momentum
PHYS 401 · Relativistic Dynamics
Relativistic momentum preserves conservation laws in all inertial frames. This lesson introduces $ec{p}=gamma mec{v}$ and compares it with classical momentum.
Key equations
ec{p}=mec{v}ec{p}=gamma mec{v}gamma=rac{1}{sqrt{1-v^2/c^2}}ec{p}approx mec{v}lim*{v o c}gamma=inftyec{F}=rac{dec{p}}{dt}ec{p}*{total}=sum_i gamma_i m_iec{v}*iec{p}*{initial}=ec{p}*{final}m*{rel}=gamma mLearning objectives
- Define relativistic momentum.
- Show that classical momentum is the low-speed limit.
- Explain why momentum grows without bound near $c$.
- Use $ec{F}=dec{p}/dt$ 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}=mec{v}
This works at low speeds, but it is not compatible with Lorentz transformations and conservation laws at speeds near . 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 and velocity ec{v} is
ec{p}=gamma mec{v}
where
gamma=rac{1}{sqrt{1-v^2/c^2}}
Low-speed limit
When , , so relativistic momentum becomes
ec{p}approx mec{v}
Thus classical momentum is the low-speed approximation to relativistic momentum.
Growth near light speed
As approaches , the Lorentz factor grows without bound. Therefore momentum grows without bound even though speed approaches a maximum:
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{dec{p}}{dt}
not simply ec{F}=mec{a}. Because ec{p}=gamma mec{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_iec{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 . Adding energy mostly increases 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 , and doubling its energy changes speed only slightly.
Relativistic mass caution
Older treatments sometimes define relativistic mass as . Modern physics usually avoids this language and keeps rest mass invariant, placing the factor in momentum and energy. This avoids confusion and supports four-vector notation.
The big idea
Relativistic momentum is ec{p}=gamma mec{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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