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

IB Diploma Programme Physics (HL/SL)

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.

IB Diploma Programme Physics (HL/SL)

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IB Diploma Programme Physics (HL/SL)

IB Diploma Programme Physics (HL/SL)

Topics follow the IB DP Physics syllabus (first assessment 2025). The IB data booklet provides equations — keywords focus on conceptual understanding, definitions and the ability to apply principles.

Mark schemes: IB Physics demands precise language: 'rate of change of velocity' not 'getting faster'. State the law or principle first, then apply it. Equations must have units on every line.

Active recall: 0 / 46 terms ticked

RecalledTopicLevelKeywordDefinition
MechanicsEssentialScalarPhysical quantity with magnitude only (e.g. distance, speed, mass, time, energy).
MechanicsEssentialVectorPhysical quantity with both magnitude and direction (e.g. displacement, velocity, acceleration, force).
MechanicsCoreDisplacementChange in position from a reference point; vector quantity (m).
MechanicsCoreVelocityRate of change of displacement with time; vector (m/s).
MechanicsCoreAccelerationRate of change of velocity with time; vector (m/s²).
MechanicsCoreNewton's first lawAn object remains at rest or constant velocity unless acted on by a resultant force.
MechanicsCoreNewton's second lawThe resultant force on an object equals its rate of change of momentum: F = ma (for constant mass).
MechanicsCoreNewton's third lawWhen object A exerts a force on object B, object B exerts an equal and opposite force on object A. Forces are the same type, act on different objects.
MechanicsCoreLinear momentump = mv; conserved in a closed system (no external resultant force).
MechanicsCoreImpulseChange in momentum; equal to force × time: J = FΔt.
MechanicsCoreKinetic energyEnergy due to motion: Ek = ½mv².
MechanicsCoreGravitational potential energyEnergy stored in a gravitational field: Ep = mgh (near Earth's surface).
MechanicsCoreWork-energy theoremNet work done on an object equals its change in kinetic energy.
MechanicsAdvancedCentre of massPoint where the entire mass of a system can be considered to act for the purpose of analysing translational motion.
WavesEssentialWaveTransfer of energy through a medium (or vacuum for EM waves) without net transfer of matter.
WavesCoreTransverse waveWave in which oscillation is perpendicular to the direction of energy transfer (e.g. light, water).
WavesCoreLongitudinal waveWave in which oscillation is parallel to the direction of energy transfer (e.g. sound, P-waves).
WavesCoreAmplitudeMaximum displacement of a particle from equilibrium position; related to wave energy.
WavesCoreFrequency (f)Number of complete oscillations per unit time; measured in Hz.
WavesCoreWavelength (λ)Distance between two adjacent points in phase (e.g. crest to crest).
WavesCoreWave speed (v)Speed at which the wave pattern propagates: v = fλ.
WavesCoreSuperpositionWhen two or more waves meet, the resultant displacement equals the sum of individual displacements.
WavesCoreDiffractionSpreading of waves as they pass through a gap or around an obstacle; most significant when gap ≈ wavelength.
WavesCoreInterferenceSuperposition of coherent waves producing regions of constructive (in phase) and destructive (out of phase) combination.
WavesCoreDoppler effectChange in observed frequency when source or observer moves relative to each other.
WavesAdvancedStanding waveStationary pattern formed by superposition of two identical waves travelling in opposite directions; has nodes (zero displacement) and antinodes (maximum displacement).
Electricity and MagnetismEssentialElectric charge (Q)Fundamental property of matter; measured in coulombs (C). Like charges repel, opposite charges attract.
Electricity and MagnetismCoreElectric current (I)Rate of flow of charge: I = Q/t; measured in amperes (A).
Electricity and MagnetismCorePotential difference (V)Work done per unit charge moved between two points: V = W/Q; measured in volts (V).
Electricity and MagnetismCoreResistance (R)Opposition to current flow: R = V/I; measured in ohms (Ω).
Electricity and MagnetismCoreOhm's lawCurrent is directly proportional to potential difference at constant temperature: V = IR.
Electricity and MagnetismCoreElectromotive force (EMF)Energy supplied per unit charge by a source of electrical energy; measured in volts (V).
Electricity and MagnetismCoreInternal resistanceResistance within a source of EMF; causes terminal voltage to be less than EMF under load.
Electricity and MagnetismCoreKirchhoff's current lawSum of currents entering a junction equals sum of currents leaving; conservation of charge.
Electricity and MagnetismCoreKirchhoff's voltage lawSum of EMFs around a closed loop equals sum of potential differences; conservation of energy.
Electricity and MagnetismAdvancedMagnetic flux (Φ)Measure of magnetic field passing through a surface: Φ = BA cos θ; measured in webers (Wb).
Electricity and MagnetismAdvancedFaraday's lawMagnitude of induced EMF equals rate of change of magnetic flux linkage.
Electricity and MagnetismAdvancedLenz's lawInduced current flows in a direction to oppose the change causing it; conservation of energy.
Thermal PhysicsEssentialTemperatureMeasure of the average kinetic energy of particles in a substance.
Thermal PhysicsCoreInternal energyTotal kinetic energy and potential energy of all particles in a substance.
Thermal PhysicsCoreSpecific heat capacity (c)Energy required to raise the temperature of 1 kg of a substance by 1 K: Q = mcΔT.
Thermal PhysicsCoreSpecific latent heat (L)Energy required to change the state of 1 kg of a substance without changing its temperature: Q = mL.
Thermal PhysicsCoreIdeal gasTheoretical gas where particles have no volume, no intermolecular forces, and collisions are perfectly elastic.
Thermal PhysicsCoreIdeal gas lawPV = nRT; P = pressure (Pa), V = volume (m³), n = moles, R = 8.31 J mol⁻¹ K⁻¹, T = temperature (K).
Thermal PhysicsAdvancedFirst law of thermodynamicsΔU = Q + W; change in internal energy equals heat added to system plus work done on system.
Thermal PhysicsAdvancedSecond law of thermodynamicsEntropy of an isolated system always increases; heat cannot spontaneously flow from cold to hot.

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Physics (HL/SL) — Keywords & Key Terms FAQ

What is on this AQA International A Level Physics keywords and key terms list?
It is a topic-organised glossary of important physics terms with short, exam-style definitions aligned to IB Diploma Programme Physics (HL/SL) (HL/SL). 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 International A Level Physics (HL/SL) 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 HL/SL specification?
Topic groupings and wording follow IB Diploma Programme Physics (HL/SL) for AQA International A Level. 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 International A Level, separate from longer notes or topic trackers.