OCR Specification focus:
‘Describe particle–antiparticle creation and annihilation processes qualitatively.’
This section explores how energetic interactions produce particle–antiparticle pairs and how their mutual destruction releases energy, providing foundational insight into relativistic processes in particle physics.
Creation and Annihilation in Particle Physics
Particle–antiparticle creation and annihilation lie at the heart of high-energy physics and provide crucial evidence for the structure of matter and the conservation laws that govern fundamental interactions. These processes occur in environments where energies are sufficiently large for mass–energy conversion to take place, reinforcing the principle that energy and mass are interchangeable, as expressed through relativistic physics. OCR expects students to understand these processes qualitatively, with emphasis on what occurs, under what circumstances, and why conservation rules are essential.
Fundamental Ideas Underlying Creation
When energy is concentrated in a small region of space, it can be converted into matter in the form of a particle and its corresponding antiparticle. This process is known as pair creation, often occurring when a high-energy photon interacts with a nucleus or an electric field that provides momentum balance.

Pair production occurs when a sufficiently energetic γ-ray interacts with the Coulomb field of a nucleus, creating an electron and a positron. The nucleus recoils slightly to conserve momentum. Labels clearly indicate the incident photon, the nucleus, and the e⁻/e⁺ tracks. Source.
Pair Creation: The process in which a high-energy photon produces a particle and its antiparticle, typically an electron and positron.
Creation requires the photon’s energy to be at least equal to the combined rest energy of the two particles, with any excess appearing as kinetic energy. Conservation laws determine whether the process can proceed and how it must occur. Key conservation principles include:
• Conservation of charge — the total electrical charge before and after creation must match.
• Conservation of momentum — a nearby nucleus is usually involved to satisfy momentum conditions.
• Conservation of energy — the incoming photon must supply sufficient energy.
• Conservation of lepton number — a lepton is always accompanied by its corresponding antilepton.
Creation processes illustrate how fundamental interactions transform electromagnetic energy into massive particles. They also demonstrate the symmetry between particles and antiparticles that underpins modern particle physics.
Photon Requirements for Pair Creation
Because photons have no rest mass, all of the mass of the produced particles must come from the incoming energy. This leads to a minimum-energy condition governed by the rest energies of the created pair.
EQUATION
—-----------------------------------------------------------------
Rest Energy (E₀) = mc²
E₀ = Minimum energy needed to create a particle from energy alone (joules)
m = Rest mass of the particle (kilograms)
c = Speed of light in vacuum (metres per second)
—-----------------------------------------------------------------
A normal sentence must follow the equation to maintain the required separation between instructional blocks. In experimental and natural settings, creation is observable through particle tracks and interaction signatures that emerge as the produced pair separates under electromagnetic influences.
The Process of Annihilation
Annihilation is the reverse of creation. When a particle encounters its corresponding antiparticle, they undergo mutual destruction, converting their mass into energy. This transformation occurs rapidly and is one of the most efficient mass-to-energy conversion mechanisms known.

The diagram shows an electron and positron meeting and annihilating to form two γ photons. The photons move in opposite directions so that momentum is conserved. The simple layout keeps focus on the two-photon final state. Source.
Annihilation: The process in which a particle and its antiparticle destroy each other, producing photons or other energy-carrying particles.
During annihilation, the energy of the outgoing photons equals the combined rest energy and kinetic energy of the original particles. GCSE and general-level treatments often emphasise electron–positron annihilation, but OCR A-Level requires a deeper conceptual appreciation that the process applies to all particle–antiparticle pairs. The key qualitative point is that the products must carry away any conserved quantities, such as momentum.
Conservation Laws in Annihilation
Annihilation obeys strict conservation rules, ensuring continuity of physical quantities across the interaction. These include:
• Charge conservation — the net charge before annihilation is zero, so the products must also be chargeless.
• Momentum conservation — typically two or more photons are emitted so that the vector sum of photon momenta cancels out.
• Energy conservation — total energy before and after annihilation remains equal.
• Lepton number conservation — lepton number is conserved in the transformation from matter–antimatter pair to photons.
These principles ensure that annihilation produces photons of specific energies and directions, enabling experimental verification through detectors and spectral measurements.
Significance of Creation and Annihilation
Although OCR requires only a qualitative understanding, it is important to recognise the centrality of these processes in physics. Creation explains the emergence of particles from high-energy fields, while annihilation provides insight into symmetry, conservation laws, and mass–energy equivalence. Both phenomena are indispensable in modern research contexts, including collider experiments, astrophysical observations, and theoretical models of the early Universe.
FAQ
Pair creation always produces the lightest available particle–antiparticle pair that satisfies the energy conditions. Electrons and positrons have the smallest rest mass of any charged leptons, so they require the least photon energy to form.
Heavier pairs such as muon–antimuon or proton–antiproton can occur, but only if the incoming photon has energy equal to or exceeding the combined rest energies of the heavier particles.
Environmental conditions, such as strong electromagnetic fields, also influence which pairs can be produced.
A photon in free space cannot create a particle–antiparticle pair because momentum cannot be conserved without an additional body.
In pair creation, the photon’s momentum must be balanced by recoil. A nearby nucleus or strong electric field provides this recoil, allowing both energy and momentum conservation to be satisfied.
This is why pair creation is observed near atoms or in regions of intense electromagnetic fields, such as near heavy nuclei.
Electron and positron tracks curve in opposite directions when moving through a magnetic field due to their equal and opposite charges.
In detectors such as cloud or bubble chambers:
• the electron curves one way; the positron curves the other
• the radius of curvature reveals each particle’s momentum
• the point where both tracks originate identifies the creation event
This curvature pattern provides a clear experimental signature of pair creation.
A single photon cannot simultaneously satisfy energy and momentum conservation when produced from a particle–antiparticle pair initially at rest.
Two photons emitted in opposite directions allow:
• total momentum to remain zero
• total energy to match the mass–energy and kinetic energy of the annihilating pair
• symmetric distribution of energy
Although rarer, three or more photons can be produced if the initial particles have additional kinetic energy.
Yes, if the electron and positron possess enough kinetic energy, their total energy may exceed the rest mass of other particle–antiparticle pairs.
Possible products include:
• muon–antimuon pairs
• hadrons, provided energy thresholds are met
However, at low energies, annihilation predominantly produces gamma photons because photons have no rest mass and require the least energy to form, making them the most probable outcome.
Practice Questions
Question 1 (2 marks)
State what is meant by pair creation and explain why a nearby nucleus is usually required for this process to occur.
Mark scheme:
• Pair creation is the formation of a particle and its corresponding antiparticle from energy, typically from a high-energy photon. (1 mark)
• A nearby nucleus is required to conserve momentum during the interaction. (1 mark)
Question 2 (5 marks)
A high-energy gamma photon interacts in a detector and produces an electron–positron pair.
Explain, with reference to conservation laws, how both pair creation and annihilation demonstrate the interchangeability of mass and energy. In your answer, comment on:
• the energy requirements for pair creation
• the role of charge, momentum, and lepton number conservation
• why two photons are typically produced during annihilation
Mark scheme:
• Pair creation requires the incoming photon to have energy at least equal to the combined rest energies of the electron and positron. (1 mark)
• Any excess photon energy appears as kinetic energy of the electron–positron pair. (1 mark)
• Charge is conserved because the photon has zero charge, producing particles whose charges sum to zero. (1 mark)
• Lepton number is conserved because one lepton (electron) and one antilepton (positron) are produced. (1 mark)
• During annihilation, two photons are emitted in opposite directions to conserve momentum, and the total photon energy equals the total mass–energy and kinetic energy of the original pair. (1 mark)
