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 fails near , that the correct relativistic momentum is , that energy and momentum are linked by , and to explain how this shapes the design of particle accelerators.
The answer
Why classical momentum fails
Newtonian mechanics gives momentum as . Two clues that this must break at high speed:
- Light has no rest mass, yet it carries momentum (radiation pressure, comet tails, solar sails). The classical expression gives zero for .
- Charged particles in cyclotrons fall out of phase with the accelerating voltage at high energies, contrary to the simple 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 moving at velocity is:
At low speeds and we recover . As , and momentum grows without bound even though is capped at .
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 produce a well-defined response with finite forces.
Total energy and the energy-momentum relation
The total relativistic energy is . Combining with , eliminating and :
This is the fundamental energy-momentum invariant of special relativity. Two important limits:
- Rest: , (the rest energy).
- Massless particle (photon): , . Combined with and , this gives the photon momentum .
The speed limit
The kinetic energy is . As , , which means no finite amount of work can accelerate a massive particle to the speed of light. Massless particles travel at and cannot be accelerated or decelerated (they exist only at 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 in a perpendicular magnetic field has radius:
In a cyclotron, is fixed and the radius grows with . The angular frequency decreases as grows, so the AC accelerating voltage falls out of phase with the particle. This limits classical cyclotrons to non-relativistic energies (about MeV per nucleon for protons).
Synchrotrons fix the radius and ramp both and the AC frequency in step with the rising . The Large Hadron Collider keeps near km and ramps from about T to T while protons are accelerated from GeV to TeV. At TeV, , - 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 grows, saturates near but 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 available to make new particles. For a fixed-target collision of a particle with rest energy on a target of the same kind:
(for ),
which scales as . For collider experiments (two beams meeting head-on), , 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 TeV, GeV.
.
.
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.
Examples in context
Example 1. Australian Synchrotron 3 GeV electron beam. Electrons in the storage ring have total energy and rest energy , so and . Relativistic momentum . From , , so . The Newtonian estimate underestimates by a factor - the synchrotron simply could not exist without relativity.
Example 2. Cosmic-ray proton hitting a Lucas Heights detector. An ultra-high-energy cosmic-ray proton arrives with total energy . Proton rest energy is , so . The proton's speed is (extraordinarily close to ). Its momentum is . From the proton's frame, the Earth's diameter is contracted to .
Try this
Q1. Write the equation for relativistic momentum and the energy-momentum relation, defining each symbol. [2 marks]
- Cue. where ; .
Q2. A proton of rest mass has . Calculate (a) its speed and (b) its momentum. [4 marks]
- Cue. (a) ; . (b) .
Q3. An electron is accelerated through a potential difference of . (a) Calculate its total energy and . (b) Find its speed as a fraction of . (c) Explain why fixed-field cyclotrons fail at this energy but synchrotrons succeed. [2+2+2 marks]
- Cue. (a) , , . (b) . (c) Cyclotron frequency depends on ; as grows, the electron falls out of resonance. Synchrotrons ramp both and .
Exam-style practice questions
Practice questions written in the style of NESA exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.
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 →
Speed: m/s.
Lorentz factor:
.
Relativistic momentum:
kg m/s.
Classical momentum at the same speed:
kg m/s.
Ratio: .
At the relativistic momentum is more than three times the classical value, so classical mechanics underestimates the momentum substantially. Markers reward correct , both momenta, and an explicit comparison showing that the discrepancy grows rapidly as .
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 →
A charged particle of momentum moving perpendicular to a magnetic field follows a circular path of radius:
with in the relativistic case. As the particle is accelerated, its speed quickly saturates close to , but continues to grow without bound (it tends to infinity as ). The momentum, and the kinetic energy , continue to grow with even though barely changes.
To keep a particle of growing on the same circular path, either must be increased (synchrotrons ramp in lockstep with during acceleration) or must be made very large (LHC has km). Otherwise the particle's radius would exceed the beam pipe.
The non-relativistic formula would predict the radius levels off as , but in reality the radius keeps growing as grows. This is direct evidence in operating accelerators that relativistic momentum is the right expression.
Markers reward the relationship, the role of growing , and connection to the design choices in real machines.
Related dot points
- Analyse the Michelson-Morley experiment, state Einstein's two postulates of special relativity, and apply the consequences of time dilation, length contraction and relativity of simultaneity
A focused answer to the HSC Physics Module 7 dot point on light and special relativity. The Michelson-Morley null result, Einstein's two postulates, and quantitative application of time dilation t = gamma t_0, length contraction L = L_0 / gamma and relativity of simultaneity.
- Derive and apply the mass-energy equivalence E = mc^2, including the calculation of mass defect and binding energy in nuclear reactions
A focused answer to the HSC Physics Module 7 dot point on mass-energy equivalence. The total relativistic energy E = gamma m c^2, the rest energy E_0 = mc^2, mass defect Delta m in nuclear binding, and worked examples for fission, fusion and the deuteron binding energy.
- Investigate experimental and observational evidence for special relativity, including atmospheric and accelerator muon decay, GPS clock corrections, and the routine use of relativistic mechanics in particle physics
A focused answer to the HSC Physics Module 7 dot point on evidence for special relativity. Atmospheric muon flux at sea level, accelerator muon lifetimes, the daily GPS clock corrections (combined SR and GR), and the routine use of relativistic kinematics in particle physics.