CSEC Physics study materials
CSEC Physics study resources

CSEC Physics key terms

CSEC Physics · Get comfortable with the vocabulary.

Displacement

The straight-line distance and direction from a starting point to an ending point. It is a vector quantity, so moving in a closed loop gives zero displacement even though distance travelled is not zero.

Related: Velocity, Scalar and Vector
Velocity

The rate of change of displacement with time, including direction. Average velocity is total displacement divided by total time; instantaneous velocity is the value at one moment.

Related: Displacement, Acceleration
Acceleration

The rate at which velocity changes with time. Because velocity is a vector, acceleration occurs when speed changes, direction changes, or both change.

Related: Velocity, Free Fall
Scalar and Vector

A scalar has magnitude only, such as mass, time, or temperature. A vector has both magnitude and direction, such as force, velocity, or displacement, and is added using direction-sensitive rules.

Related: Displacement, Resultant Force
Free Fall

Motion under gravity alone, with air resistance ignored. Near the Earth's surface the acceleration is about 9.8 m/s² downward, so all objects fall at the same rate regardless of mass.

Related: Acceleration, Weight
Newton's First Law

An object stays at rest or moves with constant velocity unless a resultant external force acts on it. The law describes inertia, the tendency of matter to resist changes in motion.

Related: Newton's Second Law, Inertia
Newton's Second Law

The resultant force on an object equals its mass multiplied by its acceleration, written F = ma. A larger force produces greater acceleration, and a larger mass produces less.

Related: Resultant Force, Newton's First Law
Newton's Third Law

For every action force there is an equal and opposite reaction force. The pair acts on two different bodies, which is why the forces do not cancel each other.

Related: Resultant Force, Weight
Inertia

The resistance of an object to any change in its state of motion. It depends only on mass, so a more massive object needs a larger force to change its velocity.

Related: Newton's First Law, Mass
Resultant Force

The single force that has the same effect as all the forces acting on a body combined. If it is zero, the body is in equilibrium and its velocity does not change.

Related: Newton's Second Law, Moment
Moment

The turning effect of a force about a pivot, calculated as force multiplied by the perpendicular distance from the pivot. It is measured in newton metres.

Related: Principle of Moments, Centre of Gravity
Principle of Moments

For a body in equilibrium, the sum of clockwise moments about any point equals the sum of anticlockwise moments about that same point. This allows unknown forces or distances to be calculated.

Related: Moment, Centre of Gravity
Centre of Gravity

The point at which the whole weight of a body may be considered to act. For a uniform regular shape it lies at the geometric centre; for irregular shapes it can be found by hanging.

Related: Moment, Stability
Stability

The ability of an object to return to its original position after being tilted. It increases when the centre of gravity is low and the base area is wide.

Related: Centre of Gravity, Moment
Work and Power

Work is energy transferred when a force moves an object through a distance, measured in joules. Power is the rate of doing work, measured in watts, so power equals work divided by time.

Related: Kinetic Energy, Efficiency
Kinetic Energy

The energy a body possesses because of its motion, calculated as one half of mass times velocity squared. Doubling the speed gives four times the kinetic energy.

Related: Work and Power, Conservation of Energy
Conservation of Energy

Energy cannot be created or destroyed, only transferred or transformed from one form to another. In a closed system the total energy remains constant, though some may spread as heat.

Related: Kinetic Energy, Efficiency
Efficiency

The ratio of useful energy output to total energy input, usually expressed as a percentage. No real machine is 100 percent efficient because friction and other losses waste energy.

Related: Work and Power, Conservation of Energy
Pressure

The force acting normally per unit area on a surface, measured in pascals. The same force produces greater pressure when it acts over a smaller area.

Related: Upthrust, Density
Density

The mass of a substance per unit volume, measured in kilograms per cubic metre. It explains why objects of equal size can have very different masses and whether they float.

Related: Pressure, Upthrust
Upthrust

The upward force exerted by a fluid on an object immersed in it, caused by the greater pressure at the bottom than at the top. It equals the weight of fluid displaced.

Related: Density, Pressure
Internal Energy

The total kinetic and potential energy of the particles in a substance. Heating increases internal energy, raising temperature or causing a change of state.

Related: Specific Heat Capacity, Latent Heat
Specific Heat Capacity

The energy needed to raise the temperature of one kilogram of a substance by one degree Celsius. Water has a high value, so it heats and cools slowly.

Related: Internal Energy, Latent Heat
Latent Heat

The energy absorbed or released when a substance changes state without changing temperature. Latent heat of fusion applies to melting and freezing; latent heat of vaporisation applies to boiling and condensing.

Related: Internal Energy, Specific Heat Capacity
Conduction

The transfer of heat through a solid by particles passing on vibrations, or by free electrons in metals. Metals conduct well because their free electrons carry energy quickly.

Related: Convection, Radiation
Convection

Heat transfer in fluids by the movement of the fluid itself. Warmer, less dense fluid rises and cooler, denser fluid sinks, forming convection currents.

Related: Conduction, Density
Radiation

The transfer of heat by infrared electromagnetic waves, which needs no medium and can travel through a vacuum. Dark, matt surfaces absorb and emit it better than shiny ones.

Related: Conduction, Convection
Thermal Expansion

The increase in size of a substance as its temperature rises, because particles vibrate more and take up more space. It is allowed for in bridges, rails, and thermostats.

Related: Internal Energy, Bimetallic Strip
Bimetallic Strip

Two different metals joined together that bend when heated because they expand by different amounts. It is used in thermostats and fire alarms to make or break circuits.

Related: Thermal Expansion, Conduction
Wave

A disturbance that transfers energy from one place to another without transferring matter. Waves may be mechanical, needing a medium, or electromagnetic, which can travel through a vacuum.

Related: Wavelength, Frequency
Wavelength

The distance between two consecutive corresponding points on a wave, such as crest to crest. It is measured in metres and is represented by the symbol lambda.

Related: Frequency, Wave Speed
Frequency

The number of complete waves passing a point each second, measured in hertz. It is fixed by the source and does not change when a wave enters a new medium.

Related: Wavelength, Wave Speed
Wave Speed

The distance a wave travels each second, equal to frequency multiplied by wavelength. When a wave enters a denser medium its speed and wavelength change but frequency stays the same.

Related: Frequency, Wavelength
Refraction

The change in direction of a wave as it passes from one medium to another at an angle, caused by a change in speed. It bends towards the normal when slowing down.

Related: Refractive Index, Total Internal Reflection
Refractive Index

A measure of how much a medium slows light, found by dividing the speed of light in a vacuum by its speed in the medium. It also relates the angles of incidence and refraction.

Related: Refraction, Total Internal Reflection
Total Internal Reflection

When light travelling in a denser medium strikes a boundary beyond the critical angle, it is completely reflected back inside. This effect carries signals in optical fibres.

Related: Refractive Index, Refraction
Lens

A curved transparent object that refracts light to form an image. A converging lens brings parallel rays to a focus; a diverging lens spreads them apart.

Related: Focal Length, Refraction
Focal Length

The distance from the centre of a lens to its principal focus, where parallel rays converge. A shorter focal length gives a more powerful lens and a larger magnification.

Related: Lens, Magnification
Magnification

The ratio of the image height to the object height. A value greater than one means the image is larger; a negative value indicates an inverted image.

Related: Lens, Focal Length
Electric Current

The rate of flow of electric charge past a point, measured in amperes. One ampere is one coulomb of charge passing each second.

Related: Voltage, Resistance
Voltage

The energy transferred per unit charge as charge moves between two points, measured in volts. It is also called potential difference and is measured with a voltmeter in parallel.

Related: Electric Current, Resistance
Resistance

The opposition to the flow of electric current in a component, measured in ohms. It equals voltage divided by current and depends on material, length, and thickness.

Related: Ohm's Law, Electric Current
Ohm's Law

The current through a metallic conductor is directly proportional to the voltage across it, provided temperature stays constant. It is written as V = IR and fails for non-ohmic components.

Related: Resistance, Voltage
Series and Parallel

In a series circuit components share one path, so current is the same and voltages add. In a parallel circuit the voltage is the same across branches and currents add.

Related: Resistance, Electric Current
Electrical Power

The rate at which electrical energy is transferred by a component, measured in watts. It equals voltage multiplied by current, or current squared multiplied by resistance.

Related: Voltage, Resistance
Electromagnetic Induction

The production of a voltage in a conductor when it experiences a changing magnetic field. This principle underlies generators and transformers.

Related: Transformer, Magnetic Field
Magnetic Field

A region where a magnetic force acts on a moving charge or magnetic material. Its direction is shown by field lines running from north to south outside a magnet.

Related: Electromagnetic Induction, Transformer
Transformer

A device with two coils on a shared iron core that changes alternating voltage by electromagnetic induction. It works only with alternating current, not steady direct current.

Related: Electromagnetic Induction, Electrical Power
Atom

The smallest particle of an element that keeps its chemical properties. It has a nucleus of protons and neutrons surrounded by electrons in shells.

Related: Atomic Number, Isotope
Atomic Number

The number of protons in the nucleus of an atom, which identifies the element. In a neutral atom it also equals the number of orbiting electrons.

Related: Mass Number, Isotope
Mass Number

The total number of protons and neutrons in the nucleus of an atom. It is always a whole number and is used with atomic number to write nuclide symbols.

Related: Atomic Number, Isotope
Isotope

Atoms of the same element with the same number of protons but different numbers of neutrons. They have identical chemical properties but may differ in radioactivity and mass.

Related: Atomic Number, Mass Number
Radioactive Decay

The spontaneous breakdown of an unstable nucleus, emitting alpha, beta, or gamma radiation. It is random, so we can predict half-life but not the decay of a single nucleus.

Related: Half-Life, Ionising Radiation
Half-Life

The time taken for half the nuclei in a radioactive sample to decay. It is constant for a given isotope and is used in dating and medical treatment.

Related: Radioactive Decay, Ionising Radiation
Ionising Radiation

Radiation carrying enough energy to remove electrons from atoms, forming ions. Alpha, beta, and gamma radiation differ in penetrating power and in how easily they are stopped.

Related: Radioactive Decay, Half-Life
Nuclear Fission

The splitting of a heavy nucleus into two lighter nuclei, releasing energy and neutrons. It powers nuclear reactors and can sustain a chain reaction.

Related: Nuclear Fusion, Mass Number
Nuclear Fusion

The joining of two light nuclei to form a heavier one, releasing large amounts of energy. It occurs in stars and requires extremely high temperature and pressure.

Related: Nuclear Fission, Mass Number