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Energy, mass and antimatterEdexcel A-Level Physics: Revision notes

Section 1

Conservation laws in particle interactions

In every interaction between particles, charge, energy (including the rest energy of the particles) and momentum are conserved. Momentum is a vector, so the momenta must cancel in direction as well as size.

Tracks in bubble chambers and cloud chambers are used to test this. Only charged particles leave tracks, and a photon or neutron leaves none. In a magnetic field the magnetic force is perpendicular to the velocity, so tracks curve: oppositely charged particles curve in opposite senses, and a faster, higher-momentum particle has a track of larger radius (r = p/BQ). A particle that loses energy to the chamber spirals inwards.

A pair of tracks that start at one point and curve in opposite senses shows that a neutral particle has produced two oppositely charged particles.

Key termsconservation of chargeconservation of momentumtrack
Exam tip

Always check momentum as a vector. A single photon cannot turn into an electron and a positron in empty space because the total momentum could not balance.

Section 2

Mass–energy equivalence and units

Mass and energy are equivalent: ΔE = c²Δm. A particle of mass m has a rest energy E = mc².

Particle energies are measured in electronvolts: 1 eV = 1.60 × 10⁻¹⁹ J, so 1 MeV = 1.60 × 10⁻¹³ J and 1 GeV = 1.60 × 10⁻¹⁰ J.

Masses are quoted in MeV/c² or GeV/c², which is just rest energy divided by c². The electron has mass 0.511 MeV/c² and the proton about 938 MeV/c².

Worked example: proton mass in kg = (938 × 10⁶ × 1.60 × 10⁻¹⁹) ÷ (3.00 × 10⁸)² = 1.50 × 10⁻¹⁰ ÷ 9.00 × 10¹⁶ = 1.67 × 10⁻²⁷ kg.

Key termsrest energyelectronvoltMeV/c²
Common mistake

Converting to joules but forgetting the 10⁶ or 10⁹. Write MeV and GeV out in full before you divide by c².

Section 3

Annihilation and pair production

Every particle has an antiparticle with the same rest mass and opposite charge (and opposite baryon and lepton number). The photon is its own antiparticle.

Annihilation: a particle and its antiparticle meet and their mass is converted entirely to energy, usually as two photons, e.g. e⁻ + e⁺ → 2γ. For an electron and positron at rest the total energy is 2 × 0.511 = 1.022 MeV, so each photon has 0.511 MeV. Two photons are needed because the total momentum is zero, so they leave in opposite directions with equal energies. PET scanners detect these photon pairs.

Pair production: a photon of energy at least 2mc² (1.022 MeV for an electron–positron pair) creates a particle and its antiparticle, e.g. γ → e⁻ + e⁺. It happens close to a nucleus, which takes up momentum. Any extra photon energy becomes the kinetic energy of the pair.

Key termsantiparticleannihilationpair production
Common mistake

The minimum energy for pair production is 2mc², not mc². Both the particle and the antiparticle must be created.

Section 4

Why high energies probe nucleons

Particles behave as waves with de Broglie wavelength λ = h/p. To resolve detail the wavelength must be comparable to or smaller than the object, so probing a nucleon (about 10⁻¹⁵ m) needs a very large momentum.

For a high-energy electron, E ≫ rest energy, so p ≈ E/c and λ ≈ hc/E.

Worked example: for 1.0 GeV electrons, E = 1.60 × 10⁻¹⁰ J and λ = (6.63 × 10⁻³⁴ × 3.00 × 10⁸) ÷ 1.60 × 10⁻¹⁰ = 1.2 × 10⁻¹⁵ m.

Electrons of 10 GeV or more, with λ well below 10⁻¹⁵ m, scatter from point-like quarks inside protons. High energies are also needed to create massive new particles, since the collision energy must supply their rest energy.

Key termsde Broglie wavelengthresolution

Section 5

Relativistic increase in particle lifetime

An unstable particle has a mean lifetime that is shortest when measured in its own rest frame. For an observer who sees the particle moving, the lifetime is longer. This is the relativistic increase in lifetime (time dilation). You do not need the relativistic equations.

The effect is only significant when the speed is a large fraction of the speed of light. At everyday speeds it is negligible.

Worked example: a muon (rest lifetime 2.2 μs) at 0.99c travels about 0.99 × 3.00 × 10⁸ × 2.2 × 10⁻⁶ = 650 m before decaying if the effect is ignored. Muons formed many kilometres up reach the ground, so their lifetime in the Earth frame must be much longer. Fast particles in accelerators also survive for longer, which is what makes beam experiments possible.

Key termstime dilationmean lifetime

Must know

  • Charge, energy and momentum are conserved in all interactions
  • ΔE = c²Δm; 1 eV = 1.60 × 10⁻¹⁹ J; masses in MeV/c² or GeV/c²
  • Annihilation: all the mass becomes photons; pair production needs at least 2mc²
  • High energy means short wavelength, which is needed to resolve nucleon structure
  • Lifetimes of fast particles are longer in the laboratory, significantly only close to c

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Exam questions on Energy, mass and antimatter

  1. In a positron emission tomography (PET) scanner, a positron emitted by a radioactive tracer in a patient annihilates with an electron in the surrounding tissue. Both particles can be taken to be at rest when they annihilate. The rest mass of an electron is 0.511 MeV/c².
    Calculate the energy, in MeV, of each photon produced.2 marks
  2. A gamma ray photon of energy 3.0 MeV, which leaves no track in a bubble chamber, converts into an electron and a positron close to an atomic nucleus. The chamber is in a uniform magnetic field and the two particles leave tracks that start at the same point. The rest mass of an electron is 0.511 MeV/c².
    Calculate the total kinetic energy of the electron and the positron, in MeV, immediately after the pair is created. Assume the nucleus takes negligible energy.2 marks
  3. Physicists fire a beam of electrons at liquid hydrogen to investigate the structure of the proton, which has a radius of about 1 × 10⁻¹⁵ m. At low beam energies the electrons scatter as if the proton were a single point. At very high beam energies some electrons are scattered through large angles, showing that the proton has internal structure.
    Explain why electrons of very high energy are needed to investigate the internal structure of the proton.3 marks
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Written by the Exaim team, led by Shaun Daswani (Head of Upper Secondary, Improve ME Institute; MSc Financial Mathematics, Imperial College London; BSc, UCL) and Jason Daswani (operational lead, Improve ME Institute; LSE).