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Physics — Keywords & Key Terms — Definitions Glossary (2026)

Cambridge IGCSE Physics (0625)

Topic-by-topic keywords, key terms and definitions for precise exam language—separate from our revision checklists (topic coverage) and formula sheets (equations).

Keywords & Key Terms — definitions

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.

Cambridge International IGCSE Physics (0625)

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Cambridge International IGCSE Physics (0625)

Cambridge IGCSE Physics (0625)

Topics follow the Cambridge IGCSE Physics 0625 syllabus for 2026 (Core and Extended). Extended candidates cover all objectives; Core omits some Extended-only content — check your entry for Core vs Extended papers.

Mark schemes: Marks reward precise scientific vocabulary, clear algebra in calculations, and logically linked physical reasoning. Practical papers (5/6) often assess measurement technique, handling of anomalies, uncertainty, and correct interpretation of gradients and intercepts on graphs.

Active recall: 0 / 80 terms ticked

RecalledTopicLevelKeywordDefinition
1. Motion, forces and energyEssentialDistanceHow far an object has travelled along a path (scalar).
1. Motion, forces and energyEssentialDisplacementStraight-line distance and direction from start to finish (vector).
1. Motion, forces and energyCoreSpeedDistance travelled per unit time; scalar.
1. Motion, forces and energyCoreVelocityRate of change of displacement; vector quantity.
1. Motion, forces and energyCoreAccelerationRate of change of velocity; a = (v − u)/t.
1. Motion, forces and energyCoreNewton’s first lawA body stays at rest or uniform velocity unless a resultant force acts.
1. Motion, forces and energyCoreNewton’s second lawF = ma for constant mass; resultant force = mass × acceleration.
1. Motion, forces and energyCoreNewton’s third lawForces between two objects are equal in size, opposite in direction, same type.
1. Motion, forces and energyCoreFrictionForce opposing relative motion between surfaces.
1. Motion, forces and energyCoreDrag (air resistance)Opposes motion through a fluid; increases with speed.
1. Motion, forces and energyCoreTerminal velocityConstant speed when drag equals weight for falling objects.
1. Motion, forces and energyAdvancedLinear momentump = mv; conserved in a closed system in the absence of external resultant force.
1. Motion, forces and energyCoreWork doneW = Fs cos θ — energy transferred when a force moves an object.
1. Motion, forces and energyCoreKinetic energyEnergy due to motion: Ek = ½mv².
1. Motion, forces and energyCoreGravitational potential energyEnergy stored due to position in a field (near Earth: Ep = mgh).
1. Motion, forces and energyCoreElastic potential energyStored when a spring or material is stretched or compressed.
1. Motion, forces and energyAdvancedPrinciple of conservation of energyTotal energy in a closed system is constant; energy is transferred between stores.
1. Motion, forces and energyCorePowerRate of energy transfer or rate of doing work: P = E/t or P = W/t.
1. Motion, forces and energyCoreEfficiencyUseful energy output ÷ total energy input × 100%.
2. Thermal physicsEssentialTemperatureMeasure related to average kinetic energy of particles in a substance.
2. Thermal physicsCoreKinetic particle modelSolids, liquids, gases differ in particle arrangement, movement and spacing.
2. Thermal physicsCoreInternal energyTotal kinetic and potential energy of particles in a substance.
2. Thermal physicsCoreSpecific heat capacityEnergy to raise 1 kg of a substance by 1 °C.
2. Thermal physicsCoreSpecific latent heatEnergy per kilogram for a change of state at constant temperature.
2. Thermal physicsCoreMelting / freezingSolid ↔ liquid at melting point.
2. Thermal physicsCoreBoiling / condensingLiquid ↔ gas at boiling point.
2. Thermal physicsCoreEvaporationLiquid → gas below boiling point at the surface.
2. Thermal physicsCoreConductionEnergy transfer through a material by particle vibration or free electron movement.
2. Thermal physicsCoreConvectionEnergy transfer by movement of fluids (convection currents).
2. Thermal physicsCoreRadiationEnergy transfer by infrared and other EM waves; no medium required.
2. Thermal physicsAdvancedThermal equilibriumNo net energy transfer between objects at the same temperature.
2. Thermal physicsCoreThermal expansionMost substances expand when heated (exceptions noted in syllabus).
3. Properties of waves (including light and sound)EssentialWaveTransfer of energy without permanent transfer of matter.
3. Properties of waves (including light and sound)CoreTransverse waveOscillation perpendicular to energy transfer direction.
3. Properties of waves (including light and sound)CoreLongitudinal waveOscillation parallel to energy transfer (e.g. sound).
3. Properties of waves (including light and sound)CoreAmplitudeMaximum displacement from equilibrium.
3. Properties of waves (including light and sound)CoreFrequencyNumber of complete oscillations per second (Hz).
3. Properties of waves (including light and sound)CoreWavelengthDistance between two adjacent in-phase points on a wave.
3. Properties of waves (including light and sound)CorePeriodTime for one complete oscillation; T = 1/f.
3. Properties of waves (including light and sound)CoreWave equationv = fλ.
3. Properties of waves (including light and sound)CoreReflectionWave bounces off a boundary; angle of incidence = angle of reflection.
3. Properties of waves (including light and sound)CoreRefractionChange in speed/direction when crossing a boundary between media.
3. Properties of waves (including light and sound)CoreDiffractionSpreading when waves pass through a gap or past an edge.
3. Properties of waves (including light and sound)AdvancedTotal internal reflectionOccurs when angle of incidence > critical angle; used in optical fibres.
3. Properties of waves (including light and sound)CoreEchoReflection of sound; use for distance = speed × time ÷ 2.
3. Properties of waves (including light and sound)CoreElectromagnetic spectrumFamily of transverse waves — radio, microwave, IR, visible, UV, X-ray, gamma.
4. Electricity and magnetismEssentialElectric currentRate of flow of charge; I = Q/t; measured in amperes.
4. Electricity and magnetismEssentialPotential differenceEnergy transferred per unit charge between two points; V = W/Q.
4. Electricity and magnetismCoreResistanceR = V/I; opposition to current; unit ohm (Ω).
4. Electricity and magnetismCoreOhm’s lawFor a metallic conductor at constant temperature, I ∝ V.
4. Electricity and magnetismCoreSeries circuitSingle path — same current everywhere.
4. Electricity and magnetismCoreParallel circuitBranches — same p.d. across each parallel branch.
4. Electricity and magnetismCoreElectrical powerP = IV = I²R = V²/R.
4. Electricity and magnetismCoreElectrical energyE = Pt = IVt.
4. Electricity and magnetismCoreMagnetic fieldRegion where magnetic materials experience a force.
4. Electricity and magnetismCoreElectromagnetSolenoid with iron core; field controlled by current.
4. Electricity and magnetismAdvancedElectromagnetic inductionInduced e.m.f. when magnetic flux through a circuit changes (Faraday’s law idea at IGCSE level).
4. Electricity and magnetismCoreTransformerChanges alternating voltage using electromagnetic induction between coils.
4. Electricity and magnetismCoreMotor effectForce on current-carrying conductor in magnetic field.
4. Electricity and magnetismCoreGenerator effectInduced e.m.f. when conductor cuts magnetic field lines.
5. Nuclear physics & spaceEssentialAtomNucleus (protons + neutrons) surrounded by electrons.
5. Nuclear physics & spaceCoreProton number (atomic number)Number of protons in nucleus; defines the element.
5. Nuclear physics & spaceCoreNucleon number (mass number)Total protons + neutrons in nucleus.
5. Nuclear physics & spaceCoreIsotopeSame proton number, different nucleon number.
5. Nuclear physics & spaceCoreAlpha radiationHelium nucleus; highly ionising; stopped by paper.
5. Nuclear physics & spaceCoreBeta radiationFast electron from nucleus; moderate penetration.
5. Nuclear physics & spaceCoreGamma radiationEM wave from nucleus; highly penetrating.
5. Nuclear physics & spaceCoreHalf-lifeAverage time for half the radioactive nuclei to decay.
5. Nuclear physics & spaceCoreActivityDecays per second (becquerel, Bq).
5. Nuclear physics & spaceAdvancedBackground radiationNatural ionising radiation always present; subtract from readings in experiments.
5. Nuclear physics & spaceCoreFusionLight nuclei join; releases energy (stars).
5. Nuclear physics & spaceCoreFissionHeavy nucleus splits; used in power and weapons.
5. Nuclear physics & spaceCoreSolar systemStar, planets, moons, asteroids, comets — basic descriptive astronomy.
6. Pressure, moments & densityEssentialDensityMass per unit volume: ρ = m/V.
6. Pressure, moments & densityCorePressureForce per unit area: p = F/A.
6. Pressure, moments & densityCoreLiquid pressureIncreases with depth; depends on density and gravitational field.
6. Pressure, moments & densityCoreAtmospheric pressureDue to weight of air; decreases with altitude.
6. Pressure, moments & densityCoreMoment of a forceTurning effect = force × perpendicular distance to pivot.
6. Pressure, moments & densityCorePrinciple of momentsFor equilibrium, sum of clockwise moments = sum of anticlockwise moments.
6. Pressure, moments & densityAdvancedCentre of massPoint where weight appears to act; stability depends on base area and position.

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Physics (0625) — Keywords & Key Terms FAQ

What is on this Cambridge International IGCSE Physics keywords and key terms list?
It is a topic-organised glossary of important physics terms with short, exam-style definitions aligned to Cambridge IGCSE Physics (0625) (0625). It is designed for “define”, “state”, “outline” and “explain” questions where precise vocabulary earns marks.
How should I use this Physics glossary alongside past papers?
Tick terms when you can recall them without reading the answer, then check your wording against mark schemes. Pair vocabulary practice with past papers for IGCSE Physics (0625) so you apply terms in context.
Is this the same as a revision checklist or a formula sheet?
No. Revision checklists help you track which syllabus topics you have covered and your confidence—separate pages on Tutopiya. Formula sheets summarise equations and quantitative relationships. This page is only a definitions and key-terms glossary for Physics. Quantitative relationships belong on formula sheets; this list emphasises language and concepts.
Can I download this Physics keywords and key terms list for free?
Yes. After a quick free sign-up you can download a UTF-8 CSV (opens in Excel or Google Sheets) or open a print-friendly page and save as PDF. Browsing the list on the page is free.
Is this Physics list aligned to the 0625 specification?
Topic groupings and wording follow Cambridge IGCSE Physics (0625) for Cambridge International IGCSE. Always confirm final learning objectives and any regional options in your official specification and recent examiner reports for your exam session.
Why focus on definitions instead of full notes?
Mark schemes reward correct technical terms and clear links between ideas. A compact glossary lets you drill the exact language examiners expect for Physics at IGCSE, separate from longer notes or topic trackers.