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NSWPhysicsSyllabus dot point

Inquiry Question 3: What evidence supports the relativistic model of the universe?

Compare classical and relativistic momentum, derive p = gamma m v, and analyse the role of relativistic momentum in particle accelerators

A focused answer to the HSC Physics Module 7 dot point on relativistic momentum. Why p = mv fails near c, the relativistic form p = gamma m v, the relativistic energy-momentum relation E^2 = (pc)^2 + (mc^2)^2, and how this drives the design of particle accelerators.

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What this dot point is asking

NESA wants you to know that classical p=mvp = m v fails near cc, that the correct relativistic momentum is p=Ξ³mvp = \gamma m v, that energy and momentum are linked by E2=(pc)2+(mc2)2E^2 = (pc)^2 + (mc^2)^2, and to explain how this shapes the design of particle accelerators.

The answer

Why classical momentum fails

Newtonian mechanics gives momentum as p=mvp = m v. Two clues that this must break at high speed:

  1. Light has no rest mass, yet it carries momentum (radiation pressure, comet tails, solar sails). The classical expression mvm v gives zero for m=0m = 0.
  2. Charged particles in cyclotrons fall out of phase with the accelerating voltage at high energies, contrary to the simple r=mv/(qB)r = m v / (q B) relation.

The resolution is that momentum must be modified at high speed so that conservation of momentum holds in all inertial frames consistent with Einstein's postulates.

Relativistic momentum

The correct expression for momentum of a particle of rest mass mm moving at velocity v⃗\vec{v} is:

pβƒ—=Ξ³mvβƒ—,Ξ³=11βˆ’v2/c2\boxed{\vec{p} = \gamma m \vec{v}, \quad \gamma = \frac{1}{\sqrt{1 - v^2 / c^2}}}

At low speeds Ξ³β†’1\gamma \to 1 and we recover pβƒ—=mvβƒ—\vec{p} = m \vec{v}. As vβ†’cv \to c, Ξ³β†’βˆž\gamma \to \infty and momentum grows without bound even though vv is capped at cc.

This relation can be derived from a number of arguments: requiring momentum conservation in elastic collisions analysed from two different inertial frames, deriving the four-momentum from the four-velocity in spacetime, or demanding that Newton's second law F⃗=dp⃗/dt\vec{F} = d\vec{p}/dt produce a well-defined response with finite forces.

Total energy and the energy-momentum relation

The total relativistic energy is E=Ξ³mc2E = \gamma m c^2. Combining with p=Ξ³mvp = \gamma m v, eliminating Ξ³\gamma and vv:

E2=(pc)2+(mc2)2\boxed{E^2 = (p c)^2 + (m c^2)^2}

This is the fundamental energy-momentum invariant of special relativity. Two important limits:

  • Rest: p=0p = 0, E=mc2E = m c^2 (the rest energy).
  • Massless particle (photon): m=0m = 0, E=pcE = p c. Combined with E=hfE = h f and Ξ»f=c\lambda f = c, this gives the photon momentum p=hf/c=h/Ξ»p = h f / c = h / \lambda.

The speed limit

The kinetic energy is KE=(Ξ³βˆ’1)mc2KE = (\gamma - 1) m c^2. As vβ†’cv \to c, KEβ†’βˆžKE \to \infty, which means no finite amount of work can accelerate a massive particle to the speed of light. Massless particles travel at cc and cannot be accelerated or decelerated (they exist only at cc in vacuum).

Particle accelerators

The whole job of an accelerator is to push charged particles to extremely high energies for collision experiments. Relativistic momentum dominates the design.

Circular machines (cyclotron, synchrotron). A particle of momentum pp in a perpendicular magnetic field BB has radius:

r=pqB=Ξ³mvqBr = \frac{p}{q B} = \frac{\gamma m v}{q B}

In a cyclotron, BB is fixed and the radius grows with pp. The angular frequency Ο‰=qB/(Ξ³m)\omega = q B / (\gamma m) decreases as Ξ³\gamma grows, so the AC accelerating voltage falls out of phase with the particle. This limits classical cyclotrons to non-relativistic energies (about 1010 MeV per nucleon for protons).

Synchrotrons fix the radius and ramp both BB and the AC frequency in step with the rising Ξ³\gamma. The Large Hadron Collider keeps rr near 4.34.3 km and ramps BB from about 0.50.5 T to 8.38.3 T while protons are accelerated from 450450 GeV to 77 TeV. At 77 TeV, Ξ³β‰ˆ7460\gamma \approx 7460, v/cβ‰ˆ1βˆ’9Γ—10βˆ’9v / c \approx 1 - 9 \times 10^{-9} - just a hair below light speed, but with enormous momentum.

Linear accelerators (linacs). A linac uses successive RF cavities to add small kicks to the particle's energy along a straight line. Relativistic momentum determines the spacing of the drift tubes: as Ξ³\gamma grows, vv saturates near cc but pp keeps increasing, so cavity spacings only need to grow modestly along the line.

Why this matters in collisions

The reachable physics is set not by the lab-frame energy but by the centre-of-mass energy s\sqrt{s} available to make new particles. For a fixed-target collision of a particle with rest energy mc2m c^2 on a target of the same kind:

sβ‰ˆ2mc2β‹…Elab\sqrt{s} \approx \sqrt{2 m c^2 \cdot E_{\text{lab}}} (for Elab≫mc2E_{\text{lab}} \gg m c^2),

which scales as Elab\sqrt{E_{\text{lab}}}. For collider experiments (two beams meeting head-on), s=2Ebeam\sqrt{s} = 2 E_{\text{beam}}, scaling linearly with beam energy. This is why almost all modern high-energy machines are colliders rather than fixed-target.

Worked example: a proton at the LHC

At E=7E = 7 TeV, E0=mpc2=0.938E_0 = m_p c^2 = 0.938 GeV.

Ξ³=E/E0=7000/0.938=7463\gamma = E / E_0 = 7000 / 0.938 = 7463.

v/c=1βˆ’1/Ξ³2β‰ˆ1βˆ’1/(2Ξ³2)=1βˆ’9.0Γ—10βˆ’9v / c = \sqrt{1 - 1/\gamma^2} \approx 1 - 1/(2 \gamma^2) = 1 - 9.0 \times 10^{-9}.

pc=E2βˆ’(mc2)2β‰ˆE=7p c = \sqrt{E^2 - (m c^2)^2} \approx E = 7 TeV (the rest energy is negligible compared to total energy).

Each proton carries the kinetic energy of a mosquito in flight, but concentrated into a single subatomic particle.

Common traps

Writing p=mv/1βˆ’v2/c2p = m v / \sqrt{1 - v^2/c^2} then thinking mm changes. Modern convention: mm is the invariant rest mass; relativistic effects sit in Ξ³\gamma. "Relativistic mass" is an older language used in early textbooks.

Using p=mvp = m v for fast electrons. At 0.95c0.95 c the classical value is off by a factor of Ξ³β‰ˆ3.2\gamma \approx 3.2. At 0.99c0.99 c it is off by a factor of 77.

Forgetting the photon momentum. Photons have p=E/c=hf/c=h/Ξ»p = E / c = h f / c = h / \lambda despite being massless. Important for radiation pressure and Compton scattering.

Saying particles "approach but cannot reach cc" as a kinematic limit. It is a dynamical limit: a massive particle cannot be accelerated to cc because that would require infinite energy.

Treating r=mv/(qB)r = mv/(qB) as exact for relativistic particles. The correct form is r=p/(qB)=Ξ³mv/(qB)r = p/(qB) = \gamma m v / (q B). This is why cyclotrons need to be replaced by synchrotrons at high energies.

In one sentence

The classical momentum p=mvp = m v must be replaced by p=Ξ³mvp = \gamma m v near the speed of light, with energy and momentum linked by E2=(pc)2+(mc2)2E^2 = (pc)^2 + (mc^2)^2, and the unbounded growth of Ξ³\gamma near cc dictates the use of synchrotrons and linacs with ramped fields rather than fixed-field cyclotrons in modern particle accelerators.

Past exam questions, worked

Real questions from past NESA papers on this dot point, with our answer explainer.

2023 HSC4 marksAn electron is accelerated to 0.95c in a linear accelerator. Calculate the electron's relativistic momentum and compare it to the classical momentum at the same speed. Electron rest mass is 9.11 x 10^-31 kg.
Show worked answer β†’

Speed: v=0.95c=2.85Γ—108v = 0.95 c = 2.85 \times 10^8 m/s.

Lorentz factor:

Ξ³=1/1βˆ’0.9025=1/0.0975=1/0.3122=3.203\gamma = 1 / \sqrt{1 - 0.9025} = 1 / \sqrt{0.0975} = 1 / 0.3122 = 3.203.

Relativistic momentum:

p=Ξ³mv=3.203Γ—9.11Γ—10βˆ’31Γ—2.85Γ—108=8.31Γ—10βˆ’22p = \gamma m v = 3.203 \times 9.11 \times 10^{-31} \times 2.85 \times 10^8 = 8.31 \times 10^{-22} kg m/s.

Classical momentum at the same speed:

pc=mv=9.11Γ—10βˆ’31Γ—2.85Γ—108=2.60Γ—10βˆ’22p_c = m v = 9.11 \times 10^{-31} \times 2.85 \times 10^8 = 2.60 \times 10^{-22} kg m/s.

Ratio: p/pc=Ξ³=3.20p / p_c = \gamma = 3.20.

At 0.95c0.95c the relativistic momentum is more than three times the classical value, so classical mechanics underestimates the momentum substantially. Markers reward correct γ\gamma, both momenta, and an explicit comparison showing that the discrepancy grows rapidly as v→cv \to c.

2019 HSC3 marksExplain why particle accelerators must use larger and larger magnetic fields (or larger radii) to keep increasing the energy of particles, even though the particles' speeds approach but never reach c.
Show worked answer β†’

A charged particle of momentum pp moving perpendicular to a magnetic field BB follows a circular path of radius:

r=p/(qB)r = p / (q B)

with p=Ξ³mvp = \gamma m v in the relativistic case. As the particle is accelerated, its speed quickly saturates close to cc, but Ξ³\gamma continues to grow without bound (it tends to infinity as vβ†’cv \to c). The momentum, and the kinetic energy KE=(Ξ³βˆ’1)mc2KE = (\gamma - 1) m c^2, continue to grow with Ξ³\gamma even though vv barely changes.

To keep a particle of growing Ξ³\gamma on the same circular path, either BB must be increased (synchrotrons ramp BB in lockstep with Ξ³\gamma during acceleration) or rr must be made very large (LHC has rβ‰ˆ4r \approx 4 km). Otherwise the particle's radius would exceed the beam pipe.

The non-relativistic formula r=mv/(qB)r = m v / (q B) would predict the radius levels off as v→cv \to c, but in reality the radius keeps growing as γmv\gamma m v grows. This is direct evidence in operating accelerators that relativistic momentum is the right expression.

Markers reward the r=p/(qB)r = p/(qB) relationship, the role of growing Ξ³\gamma, and connection to the design choices in real machines.

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