AQA · GCSE · 8463
AQA GCSE Physics (8463) — Specification (2026)
Topic-by-topic keywords, key terms and definitions for precise exam language—separate from our revision checklists (topic coverage) and formula sheets (equations).
Examiner-style keywords and definitions organised by syllabus topic. Terms are tagged Essential (start here), Core (typical exam standard), and Advanced for harder distinctions — tick each row when you can recall it. Your progress is saved in this browser for this list.
AQA GCSE Physics (8463)
AQA GCSE Physics (8463) — Specification (2026)
Topics match the AQA GCSE Physics specification headings (energy; electricity; particle model of matter; atomic structure; forces; waves; magnetism & electromagnetism; space).
Mark schemes: AQA mark schemes reward precise scientific terms, correct units, and clear cause→effect links (e.g., “increases, therefore…”). Use full terms (not vague ‘it’) and include required quantities/units when defining.
Active recall: 0 / 52 terms ticked
| Recalled | Topic | Level | Keyword | Definition |
|---|---|---|---|---|
| Energy | Essential | Energy | The capacity to do work or cause change; measured in joules (J). | |
| Energy | Essential | Work done | Energy transferred when a force causes a displacement: work done = force × distance moved in the direction of the force. | |
| Energy | Core | Efficiency | Useful output energy (or power) ÷ total input energy (or power), often expressed as a percentage. | |
| Energy | Core | Power | The rate of energy transfer (or work done) per second; measured in watts (W). | |
| Energy | Core | Specific heat capacity | Energy required to raise the temperature of 1 kg of a substance by 1°C (or 1 K). | |
| Energy | Advanced | Thermal conductivity | A measure of how quickly thermal energy is transferred through a material by conduction. | |
| Energy | Advanced | Energy conservation | In a closed system, total energy remains constant; energy is transferred/stored, not created or destroyed. | |
| Electricity | Essential | Charge | A property of matter that can be positive or negative; measured in coulombs (C). | |
| Electricity | Essential | Current | Rate of flow of electric charge: current = charge ÷ time; measured in amperes (A). | |
| Electricity | Core | Potential difference (voltage) | Energy transferred per unit charge between two points: potential difference = energy ÷ charge; measured in volts (V). | |
| Electricity | Core | Resistance | A measure of how much a component opposes current: resistance = potential difference ÷ current; measured in ohms (Ω). | |
| Electricity | Core | Series circuit | A circuit with one loop; current is the same through all components; potential differences add to the supply. | |
| Electricity | Core | Parallel circuit | A circuit with branches; potential difference is the same across each branch; currents in branches add to the total. | |
| Electricity | Advanced | Ohmic conductor | A component where current is directly proportional to potential difference (constant resistance) at constant temperature. | |
| Electricity | Advanced | LDR (light-dependent resistor) | A resistor whose resistance decreases as light intensity increases. | |
| Particle model of matter | Essential | Density | Mass per unit volume: density = mass ÷ volume; measured in kg/m³. | |
| Particle model of matter | Core | Internal energy | Total energy stored in a system’s particles (kinetic + potential energies). | |
| Particle model of matter | Core | Specific latent heat | Energy required to change the state of 1 kg of a substance without changing temperature. | |
| Particle model of matter | Core | Gas pressure | Force per unit area from particle collisions with container walls; measured in pascals (Pa). | |
| Particle model of matter | Advanced | Brownian motion | Random motion of small particles in a fluid due to collisions with fluid particles. | |
| Particle model of matter | Advanced | Absolute zero | 0 K, the lowest possible temperature; particles have minimum possible kinetic energy. | |
| Atomic structure & radiation | Essential | Isotope | Atoms of the same element with the same number of protons but different numbers of neutrons. | |
| Atomic structure & radiation | Core | Alpha (α) radiation | Helium nucleus emitted from an unstable nucleus; strongly ionising and stopped by paper/skin. | |
| Atomic structure & radiation | Core | Beta (β) radiation | A fast electron (or positron) emitted from the nucleus; moderately ionising; stopped by a few mm of aluminium. | |
| Atomic structure & radiation | Core | Gamma (γ) radiation | Electromagnetic radiation from the nucleus; weakly ionising; reduced by thick lead or concrete. | |
| Atomic structure & radiation | Core | Half-life | Time taken for the number of undecayed nuclei (or activity) to halve. | |
| Atomic structure & radiation | Advanced | Activity | The rate of nuclear decays per second; measured in becquerels (Bq). | |
| Forces & motion | Essential | Resultant force | The overall force on an object found by combining all the forces acting on it. | |
| Forces & motion | Core | Newton’s second law | Resultant force = mass × acceleration (F = ma). | |
| Forces & motion | Core | Momentum | Mass × velocity; measured in kg·m/s. | |
| Forces & motion | Core | Conservation of momentum | In a closed system, total momentum before an interaction equals total momentum after. | |
| Forces & motion | Advanced | Stopping distance | Thinking distance + braking distance; affected by speed, reaction time, brakes/tyres, and road conditions. | |
| Waves | Essential | Wave speed | Speed of wave movement: wave speed = frequency × wavelength. | |
| Waves | Essential | Frequency | Number of waves passing a point each second; measured in hertz (Hz). | |
| Waves | Core | Reflection | Waves bounce off a surface; angle of incidence equals angle of reflection. | |
| Waves | Core | Refraction | Change in direction when a wave enters a different medium due to a change in speed. | |
| Waves | Core | Diffraction | Spreading of waves when they pass through a gap or around an obstacle, most noticeable when gap size ~ wavelength. | |
| Waves | Advanced | Electromagnetic spectrum | All types of EM waves ordered by wavelength/frequency (radio → gamma). | |
| Magnetism & electromagnetism | Essential | Magnetic field | A region where a magnetic material or moving charge experiences a force. | |
| Magnetism & electromagnetism | Essential | Permanent magnet | A magnet that produces its own persistent magnetic field. | |
| Magnetism & electromagnetism | Core | Induced magnetism | When a material becomes magnetised in the presence of a magnetic field. | |
| Magnetism & electromagnetism | Core | Electromagnet | A magnet produced by an electric current in a coil (often around an iron core). | |
| Magnetism & electromagnetism | Core | Solenoid | A coil of wire that produces a magnetic field when current flows through it. | |
| Magnetism & electromagnetism | Core | Motor effect | A force on a current-carrying conductor in a magnetic field. | |
| Magnetism & electromagnetism | Advanced | Electromagnetic induction | Producing a potential difference by changing the magnetic flux linking a conductor/coil. | |
| Magnetism & electromagnetism | Advanced | Transformer | A device that changes the potential difference using induction; works with alternating current. | |
| Space physics | Essential | Solar system | The Sun and the objects orbiting it (planets, moons, asteroids, comets). | |
| Space physics | Core | Orbit | The curved path of an object around another due to gravitational attraction. | |
| Space physics | Core | Redshift | Light from a distant galaxy is shifted to longer wavelengths, indicating it is moving away. | |
| Space physics | Core | Big Bang theory | Model that the Universe began from a hot, dense state and has been expanding since. | |
| Space physics | Advanced | Cosmic microwave background (CMB) | Radiation left over from the early Universe; evidence for the Big Bang. | |
| Space physics | Advanced | Dark matter | Unseen matter inferred from gravitational effects (e.g., galaxy rotation curves). |
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