Pancyprian Technical School Physics (4-hour) study materials
Pancyprian Technical School Physics (4-hour) study resources

Pancyprian Technical School Physics (4-hour) key terms

Pancyprian Technical School Physics (4-hour) · Get comfortable with the vocabulary.

Displacement

The straight-line vector from an object's initial position to its final position, including direction. It differs from distance travelled, which is a scalar and depends on the actual path taken.

Related: Velocity, Acceleration
Acceleration

The rate at which velocity changes with time, a vector quantity measured in metres per second squared. It arises whenever speed changes, direction changes, or both change simultaneously.

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

The resultant force on a body equals the product of its mass and acceleration, written F = ma. The acceleration points in the same direction as the resultant force acting on the body.

Related: Acceleration, Free-body Diagram
Free-body Diagram

A sketch showing one chosen object isolated from its surroundings, with all external forces drawn as arrows acting at their points of application. Used to identify the resultant force before applying Newton's laws.

Related: Newton's Second Law, Friction
Friction

A contact force opposing relative sliding or the tendency to slide between surfaces. Limiting static friction is proportional to the normal reaction, the constant of proportionality being the coefficient of friction.

Related: Free-body Diagram, Normal Reaction
Normal Reaction

The perpendicular contact force a surface exerts on a body resting against it. On a horizontal surface it equals the weight only when no other vertical forces act.

Related: Friction, Free-body Diagram
Principle of Conservation of Momentum

In a system with no net external force, the total vector momentum before an interaction equals the total vector momentum after it. This holds for collisions and explosions in any number of dimensions.

Related: Impulse, Elastic Collision
Impulse

The product of a force and the time interval over which it acts, equal to the change in momentum produced. Its SI unit is the newton second, equivalent to the kilogram metre per second.

Related: Principle of Conservation of Momentum, Elastic Collision
Elastic Collision

A collision in which both total momentum and total kinetic energy are conserved. In a perfectly inelastic collision momentum is still conserved but the bodies stick together and kinetic energy is lost.

Related: Principle of Conservation of Momentum, Impulse
Work Done by a Force

The product of the force component along the displacement and the displacement magnitude, measured in joules. Work is zero when force and displacement are perpendicular and negative when they oppose each other.

Related: Kinetic Energy, Power
Kinetic Energy

The energy a body possesses because of its motion, equal to one half of its mass times the square of its speed. It is a scalar and always non-negative.

Related: Work Done by a Force, Gravitational Potential Energy
Gravitational Potential Energy

Energy stored in a body because of its position in a gravitational field, near Earth equal to mass times gravitational field strength times height above a chosen reference level. Only changes in this quantity are physically meaningful.

Related: Kinetic Energy, Conservation of Mechanical Energy
Conservation of Mechanical Energy

When only conservative forces act on a system, the sum of kinetic and potential energy stays constant. Where friction or air resistance acts, mechanical energy decreases and heating occurs instead.

Related: Gravitational Potential Energy, Kinetic Energy
Power

The rate of transferring energy or doing work, measured in watts, where one watt is one joule per second. For a body moving at constant velocity it equals force times speed.

Related: Work Done by a Force, Efficiency
Efficiency

The ratio of useful energy output to total energy input for a device, usually expressed as a percentage. It is always less than one hundred per cent because some energy is dissipated, often as heat.

Related: Power, Conservation of Mechanical Energy
Centripetal Acceleration

The acceleration of a body moving along a circular path, directed towards the centre and equal to speed squared divided by radius. It changes the direction of velocity but not its magnitude.

Related: Centripetal Force, Angular Velocity
Centripetal Force

The resultant force directed towards the centre of a circular path that keeps a body moving in that path, equal to mass times centripetal acceleration. It is provided by tension, gravity, friction or another real force.

Related: Centripetal Acceleration, Angular Velocity
Angular Velocity

The rate of change of angular displacement, measured in radians per second. For uniform circular motion it equals two pi divided by the period of one revolution.

Related: Centripetal Acceleration, Simple Harmonic Motion
Simple Harmonic Motion

Oscillation in which acceleration is proportional to displacement from equilibrium and directed towards it. Its period is independent of amplitude, and displacement follows a sinusoidal variation with time.

Related: Resonance, Angular Velocity
Resonance

The large-amplitude oscillation that occurs when a system is driven at a frequency close to its natural frequency. Damping reduces the peak amplitude and broadens the response curve.

Related: Simple Harmonic Motion, Damping
Damping

The progressive loss of oscillation energy from a vibrating system, usually through friction or air resistance, so amplitudes decrease over time. Critical damping returns a system to equilibrium fastest without overshooting.

Related: Resonance, Simple Harmonic Motion
Kepler's Third Law

The square of a planet's orbital period is proportional to the cube of the semi-major axis of its orbit. The constant of proportionality depends on the mass of the central body.

Related: Gravitational Field Strength, Angular Velocity
Gravitational Field Strength

The gravitational force per unit mass experienced by a small test mass at a point, measured in newtons per kilogram. Near Earth's surface it is about 9.8 N/kg, directed towards Earth's centre.

Related: Gravitational Potential Energy, Kepler's Third Law
Pressure

The normal force per unit area exerted by a fluid or solid surface, measured in pascals. In a static fluid pressure increases with depth according to density, gravitational field strength and depth.

Related: Buoyancy, Density
Buoyancy

The upward force a fluid exerts on an immersed or floating body, equal to the weight of fluid displaced. A body floats when the buoyant force balances its weight.

Related: Pressure, Density
Density

The mass of a substance per unit volume, measured in kilograms per cubic metre. Relative density compares a substance's density with that of water and has no units.

Related: Pressure, Buoyancy
Absolute Temperature

Temperature measured on the Kelvin scale, starting at absolute zero, the lowest temperature theoretically possible. Kelvin values are obtained by adding 273 to Celsius readings.

Related: Ideal Gas Law, Specific Heat Capacity
Ideal Gas Law

The equation pV = nRT relating pressure, volume, amount of gas and absolute temperature, where R is the molar gas constant. It describes gases well at low pressure and moderate temperature.

Related: Absolute Temperature, Specific Heat Capacity
Specific Heat Capacity

The energy needed to raise the temperature of one kilogram of a substance by one kelvin, measured in joules per kilogram kelvin. Water's unusually high value explains its use as a coolant.

Related: Specific Latent Heat, Absolute Temperature
Specific Latent Heat

The energy required to change the state of one kilogram of a substance at constant temperature, without changing its temperature. It is released again when the substance changes back.

Related: Specific Heat Capacity, Absolute Temperature
Electric Field Strength

The electrostatic force per unit positive charge at a point, a vector measured in newtons per coulomb. Between parallel plates it equals voltage divided by plate separation.

Related: Electric Potential Difference, Coulomb's Law
Coulomb's Law

The electrostatic force between two point charges is proportional to the product of the charges and inversely proportional to the square of their separation. The force acts along the line joining them.

Related: Electric Field Strength, Electric Current
Electric Current

The rate of flow of electric charge past a point, measured in amperes, where one ampere is one coulomb per second. Conventional current direction is opposite to electron drift in metals.

Related: Ohm's Law, Electromotive Force
Ohm's Law

For a conductor at constant temperature, current is directly proportional to potential difference across it, so resistance equals voltage divided by current. Components such as filament lamps do not obey it.

Related: Electric Current, Electromotive Force
Electromotive Force

The energy supplied by a source per unit charge driven around a complete circuit, measured in volts. It differs from terminal potential difference because of energy lost across internal resistance.

Related: Electric Current, Ohm's Law
Magnetic Flux Density

The magnetic force per unit current per unit length on a conductor placed at right angles to a magnetic field, measured in tesla. It describes the strength and direction of the field.

Related: Electromagnetic Induction, Magnetic Flux
Magnetic Flux

The product of magnetic flux density and the area perpendicular to the field, measured in webers. When flux through a circuit changes, an electromotive force is induced.

Related: Electromagnetic Induction, Magnetic Flux Density
Electromagnetic Induction

The generation of an electromotive force in a conductor whenever the magnetic flux linked with it changes. The induced current opposes the change producing it, as stated by Lenz's law.

Related: Magnetic Flux, Magnetic Flux Density
Refractive Index

The ratio of the speed of light in vacuum to its speed in a medium, always at least one. It also equals the sine of the angle of incidence divided by the sine of the angle of refraction.

Related: Total Internal Reflection, Diffraction
Total Internal Reflection

The complete reflection of light at a boundary when it travels from a denser to a less dense medium and the angle of incidence exceeds the critical angle. It is the basis of optical fibres.

Related: Refractive Index, Diffraction
Diffraction

The spreading of waves as they pass through an aperture or around an obstacle, most pronounced when the wavelength is comparable with the obstacle size. It causes interference patterns behind narrow slits.

Related: Refractive Index, Resonance
Photoelectric Effect

The emission of electrons from a metal surface when light of sufficiently high frequency falls on it. It demonstrates that light delivers energy in discrete quanta called photons.

Related: Work Function, Half-life
Work Function

The minimum energy needed to remove an electron from the surface of a particular metal. It sets the threshold frequency below which no photoelectric emission occurs, whatever the light intensity.

Related: Photoelectric Effect, Half-life
Half-life

The time taken for half the nuclei in a sample of a radioactive isotope to decay. It is constant for a given isotope and independent of temperature, pressure or chemical state.

Related: Photoelectric Effect, Work Function
Uncertainty

The interval within which the true value of a measurement is expected to lie, reflecting limitations of the instrument and technique. It is often quoted as plus or minus half the smallest scale division.

Related: Percentage Error, Significant Figures
Percentage Error

The uncertainty of a measurement expressed as a percentage of the measured value. When quantities are multiplied or divided, their percentage errors add to give the overall percentage error.

Related: Uncertainty, Significant Figures
Significant Figures

The digits in a measured value that carry meaning about its precision, excluding leading zeros. A final answer should be quoted to the same precision as the least precise measurement used.

Related: Uncertainty, Percentage Error
Gradient of a Graph

The change in the vertical quantity divided by the corresponding change in the horizontal quantity, found from a straight line of best fit. It often represents a physical constant such as acceleration or resistance.

Related: Uncertainty, Percentage Error