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IGCSE Physics, Cambridge 0625, Malaysia

IGCSE Physics Key Definitions List

Every key definition in the IGCSE Physics 0625 syllabus, organised by topic, ready for revision and exam practice.

Written by IGCSEPhysics Content Team · Physics subject adviser: K. S. Tan, 15+ years teaching IGCSE Physics · Checked against the Cambridge IGCSE Physics (0625) 2026 to 2028 syllabus

This page lists every key definition in the Cambridge IGCSE Physics 0625 syllabus. Use it for revision and self-testing.

Topic 1: Motion, Forces and Energy

Speed: the distance travelled per unit time.

Velocity: the speed of an object in a given direction; displacement per unit time.

Acceleration: the change in velocity per unit time.

Mass: a measure of the quantity of matter in an object.

Weight: the gravitational force acting on an object; W = mg.

Density: the mass per unit volume of a substance.

Force: a push or pull that can change the motion, shape or direction of an object.

Resultant force: the single force that has the same effect as all the forces acting on an object combined.

Moment: the turning effect of a force; moment = force x perpendicular distance from the pivot.

Centre of gravity: the point at which the entire weight of an object may be considered to act.

Momentum: the product of mass and velocity of an object; p = mv.

Impulse: the change in momentum of an object; impulse = force x time.

Work: the energy transferred when a force moves an object through a distance in the direction of the force; W = Fd.

Power: the rate of doing work or the rate of energy transfer; P = W/t.

Kinetic energy: the energy an object has because of its motion; KE = 0.5mv^2.

Gravitational potential energy: the energy an object has because of its position in a gravitational field; GPE = mgh.

Efficiency: the ratio of useful energy output to total energy input, expressed as a percentage.

Pressure: the force acting per unit area; P = F/A.

Topic 2: Thermal Physics

Internal energy: the total kinetic energy and potential energy of the particles in a substance.

Temperature: a measure of the average kinetic energy of the particles in a substance.

Specific heat capacity: the energy required to raise the temperature of 1 kg of a substance by 1 degree C (or 1 K).

Specific latent heat of fusion: the energy required to change 1 kg of a substance from solid to liquid at constant temperature.

Specific latent heat of vaporisation: the energy required to change 1 kg of a substance from liquid to gas at constant temperature.

Thermal conduction: the transfer of thermal energy through a material by the vibration of particles, without the particles moving from their mean positions.

Convection: the transfer of thermal energy through a fluid by the movement of the fluid itself.

Thermal radiation: the transfer of energy by electromagnetic waves (infrared), which does not require a medium.

Topic 3: Waves

Wave: a disturbance that transfers energy from one place to another without transferring matter.

Wavelength: the minimum distance between two points on a wave that are in phase (e.g. crest to crest).

Frequency: the number of complete waves passing a point per unit time.

Amplitude: the maximum displacement of a point on the wave from its rest position.

Period: the time for one complete wave to pass a point.

Transverse wave: a wave in which the oscillations are perpendicular to the direction of energy transfer.

Longitudinal wave: a wave in which the oscillations are parallel to the direction of energy transfer.

Refraction: the change in direction of a wave as it passes from one medium to another, caused by a change in speed.

Diffraction: the spreading of a wave as it passes through a gap or around an obstacle.

Critical angle: the angle of incidence in the denser medium at which the angle of refraction is 90 degrees.

Total internal reflection: the complete reflection of light at the boundary between two media when the angle of incidence exceeds the critical angle.

Refractive index: the ratio of the speed of light in a vacuum to the speed of light in the medium; also sin(i)/sin(r).

Topic 4: Electricity and Magnetism

Electric current: the rate of flow of electric charge; I = Q/t.

Potential difference (voltage): the energy transferred per unit charge between two points; V = W/Q.

Resistance: the opposition to current flow; the ratio of potential difference to current; R = V/I.

Electromotive force (e.m.f.): the energy transferred per unit charge by a source of electrical energy.

Power (electrical): the rate at which electrical energy is transferred; P = IV.

Magnetic field: a region where a magnetic force acts on a magnetic material or a current-carrying conductor.

Electromagnetic induction: the generation of an e.m.f. (and hence a current in a closed circuit) when a conductor moves through a magnetic field or when the magnetic field through a conductor changes.

Transformer: a device that uses electromagnetic induction to change the voltage of an alternating current supply.

Topic 5: Nuclear Physics

Atom: the smallest particle of an element that retains the chemical properties of that element.

Nucleus: the dense central part of an atom, containing protons and neutrons.

Isotope: atoms of the same element that have the same number of protons but different numbers of neutrons.

Radioactive decay: the spontaneous and random emission of radiation from an unstable nucleus.

Half-life: the time taken for half of the radioactive nuclei in a sample to decay, or the time for the activity to halve.

Alpha particle: a particle consisting of 2 protons and 2 neutrons (a helium-4 nucleus), emitted during alpha decay.

Beta particle: a high-speed electron emitted from the nucleus when a neutron changes into a proton.

Gamma ray: a high-frequency electromagnetic wave emitted from the nucleus.

Nuclear fission: the splitting of a large nucleus into two smaller nuclei, with the release of energy and neutrons.

Nuclear fusion: the joining of two small nuclei to form a larger nucleus, with the release of energy.

Topic 6: Space Physics

Galaxy: a large collection of stars, gas and dust held together by gravity.

Red-shift: the increase in wavelength (and decrease in frequency) of light from galaxies moving away from us.

Hubble’s Law: the recessional velocity of a galaxy is proportional to its distance from us.

Big Bang theory: the theory that the universe began as a very hot, dense point approximately 13.8 billion years ago and has been expanding ever since.

Frequently Asked Questions

Do I need to learn every definition word-for-word?
You do not need to memorise the exact syllabus wording, but your definition must include the key physics terms and the correct relationship. Using the syllabus wording is the safest strategy.
How many definitions could be tested?
A typical Paper 4 has 2 to 4 definition questions. Any definition from the syllabus could appear.
What is the best way to learn definitions?
Flashcards with the term on one side and the definition on the other. Test yourself daily, focusing on definitions you get wrong.

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