Pearson Edexcel International GCSE in Physics Specification

Forces and Motion

Units

  • Kilogram (kg)

  • Metre (m)

  • Metre/second (m/s)

  • Metre/second squared (m/s²)

  • Newton (N)

  • Second (s)

  • Newton/kilogram (N/kg)

  • Newton metre (Nm)

  • Kilogram metre/second (kg m/s)

Movement and Position

  • Plotting and explaining distance-time graphs.

  • Relationship between average speed, distance moved, and time taken: averagespeed=distancemovedtimetakenaverage \, speed = \frac{distance \, moved}{time \, taken}

  • Practical investigation of motion of everyday objects.

  • Relationship between acceleration, change in velocity, and time taken: acceleration=changeinvelocitytimetakenacceleration = \frac{change \, in \, velocity}{time \, taken}, which can be written as a=vuta = \frac{v - u}{t}

  • Plotting and explaining velocity-time graphs.

  • Determining acceleration from the gradient of a velocity-time graph.

  • Determining the distance travelled from the area between a velocity-time graph and the time axis.

  • Relationship between final speed, initial speed, acceleration, and distance moved: (finalspeed)2=(initialspeed)2+(2×acceleration×distancemoved)(final \, speed)^2 = (initial \, speed)^2 + (2 \times acceleration \times distance \, moved), which can be written as v2=u2+(2×a×s)v^2 = u^2 + (2 \times a \times s)

Forces, Movement, Shape, and Momentum

  • Effects of forces between bodies: changes in speed, shape, or direction.

  • Different types of forces: gravitational, electrostatic, etc.

  • Difference between vector and scalar quantities.

  • Force is a vector quantity.

  • Calculating the resultant force of forces that act along a line.

  • Friction is a force that opposes motion.

  • Relationship between unbalanced force, mass, and acceleration: force=mass×accelerationforce = mass \times acceleration, which can be written as F=m×aF = m \times a

  • Relationship between weight, mass, and gravitational field strength: weight=mass×gravitationalfieldstrengthweight = mass \times gravitational \, field \, strength, which can be written as W=m×gW = m \times g

  • Stopping distance of a vehicle: sum of thinking distance and braking distance.

  • Factors affecting vehicle stopping distance: speed, mass, road condition, and reaction time.

  • Forces acting on falling objects and terminal velocity.

  • Practical investigation: how extension varies with applied force for helical springs, metal wires, and rubber bands.

  • Initial linear region of a force-extension graph is associated with Hooke’s law.

  • Elastic behavior: ability of a material to recover its original shape after the forces causing deformation have been removed.

  • Relationship between momentum, mass, and velocity: momentum=mass×velocitymomentum = mass \times velocity, which can be written as p=m×vp = m \times v

  • Using the idea of momentum to explain safety features.

  • Using the conservation of momentum to calculate mass, velocity, or momentum of objects.

  • Relationship between force, change in momentum, and time taken: force=changeinmomentumtimetakenforce = \frac{change \, in \, momentum}{time \, taken}, which can be written as F=(m×v)(m×u)tF = \frac{(m \times v) - (m \times u)}{t}

  • Understanding of Newton’s third law.

  • Relationship between the moment of a force and its perpendicular distance from the pivot: moment=force×perpendiculardistancefromthepivotmoment = force \times perpendicular \, distance \, from \, the \, pivot

  • The weight of a body acts through its center of gravity.

  • Using the principle of moments for a simple system of parallel forces acting in one plane.

  • Understanding how the upward forces on a light beam, supported at its ends, vary with the position of a heavy object placed on the beam.

Electricity

Units

  • Ampere (A)

  • Coulomb (C)

  • Joule (J)

  • Ohm (Ω)

  • Second (s)

  • Volt (V)

  • Watt (W)

Mains Electricity

  • How insulation, double insulation, earthing, fuses, and circuit breakers protect devices or users in domestic appliances.

  • Why a current in a resistor results in electrical transfer of energy and an increase in temperature and its use in domestic contexts.

  • Relationship between power, current, and voltage: power=current×voltagepower = current \times voltage, which can be written as P=I×VP = I \times V and apply the relationship to the selection of appropriate fuses.

  • Relationship between energy transferred, current, voltage, and time: energytransferred=current×voltage×timeenergy \, transferred = current \times voltage \times time, which can be written as E=I×V×tE = I \times V \times t

  • Difference between mains electricity being alternating current (a.c.) and direct current (d.c.) being supplied by a cell or battery.

Energy and Voltage in Circuits

  • Why a series or parallel circuit is more appropriate for particular applications, including domestic lighting.

  • How the current in a series circuit depends on the applied voltage and the number and nature of other components.

  • How current varies with voltage in wires, resistors, metal filament lamps, and diodes, and how to investigate this experimentally.

  • Qualitative effect of changing resistance on the current in a circuit.

  • Qualitative variation of resistance of light-dependent resistors (LDRs) with illumination and thermistors with temperature.

  • Lamps and LEDs can be used to indicate the presence of a current in a circuit.

  • Relationship between voltage, current, and resistance: voltage=current×resistancevoltage = current \times resistance, which can be written as V=I×RV = I \times R

  • Current is the rate of flow of charge.

  • Relationship between charge, current, and time: charge=current×timecharge = current \times time, which can be written as Q=I×tQ = I \times t

  • Electric current in solid metallic conductors is a flow of negatively charged electrons.

  • Why current is conserved at a junction in a circuit.

  • The voltage across two components connected in parallel is the same.

  • Calculating the currents, voltages, and resistances of two resistive components connected in a series circuit.

  • Voltage is the energy transferred per unit charge passed.

  • The volt is a joule per coulomb.

  • Relationship between energy transferred, charge, and voltage: energytransferred=charge×voltageenergy \, transferred = charge \times voltage, which can be written as E=Q×VE = Q \times V

Electric Charge

  • Common materials that are electrical conductors or insulators, including metals and plastics.

  • Practical investigation: how insulating materials can be charged by friction.

  • How positive and negative electrostatic charges are produced on materials by the loss and gain of electrons.

  • Forces of attraction between unlike charges and forces of repulsion between like charges.

  • Electrostatic phenomena in terms of the movement of electrons.

  • Potential dangers of electrostatic charges, e.g. when fuelling aircraft and tankers.

  • Some uses of electrostatic charges, e.g. in photocopiers and inkjet printers.

Waves

Units

  • Degree (°)

  • Hertz (Hz)

  • Metre (m)

  • Metre/second (m/s)

  • Second (s)

Properties of Waves

  • Difference between longitudinal and transverse waves.

  • Definitions of amplitude, wavefront, frequency, wavelength, and period of a wave.

  • Waves transfer energy and information without transferring matter.

  • Relationship between the speed, frequency, and wavelength of a wave: wavespeed=frequency×wavelengthwave \, speed = frequency \times wavelength, which can be written as v=f×λv = f \times λ

  • Relationship between frequency and time period: frequency=1timeperiodfrequency = \frac{1}{time \, period}, which can be written as f=1Tf = \frac{1}{T}

  • Using the above relationships in different contexts, including sound waves and electromagnetic waves.

  • Why there is a change in the observed frequency and wavelength of a wave when its source is moving relative to an observer, known as the Doppler effect.

  • All waves can be reflected and refracted.

The Electromagnetic Spectrum

  • Light is part of a continuous electromagnetic spectrum that includes radio, microwave, infrared, visible, ultraviolet, x-ray, and gamma ray radiations, and that all these waves travel at the same speed in free space.

  • Order of the electromagnetic spectrum in terms of decreasing wavelength and increasing frequency, including the colors of the visible spectrum.

  • Some of the uses of electromagnetic radiations, including:

    • Radio waves: broadcasting and communications

    • Microwaves: cooking and satellite transmissions

    • Infrared: heaters and night vision equipment

    • Visible light: optical fibers and photography

    • Ultraviolet: fluorescent lamps

    • X-rays: observing the internal structure of objects and materials, including for medical applications

    • Gamma rays: sterilizing food and medical equipment

  • Detrimental effects of excessive exposure of the human body to electromagnetic waves, including:

    • Microwaves: internal heating of body tissue

    • Infrared: skin burns

    • Ultraviolet: damage to surface cells and blindness

    • Gamma rays: cancer, mutation and describe simple protective measures against the risks

Light and Sound

  • Light waves are transverse waves that can be reflected and refracted.

  • The law of reflection (the angle of incidence equals the angle of reflection).

  • Drawing ray diagrams to illustrate reflection and refraction.

  • Practical investigation: the refraction of light, using rectangular blocks, semi-circular blocks, and triangular prisms.

  • Relationship between refractive index, angle of incidence, and angle of refraction: n=sinisinrn = \frac{sin \, i}{sin \, r}

  • Practical investigation: the refractive index of glass, using a glass block.

  • The role of total internal reflection in transmitting information along optical fibers and in prisms.

  • Meaning of critical angle.

  • Relationship between critical angle and refractive index: n=1sincn = \frac{1}{sin \, c}

  • Sound waves are longitudinal waves that can be reflected and refracted.

  • The frequency range for human hearing is 20–20 000 Hz.

  • Practical investigation: the speed of sound in air.

  • How an oscilloscope and microphone can be used to display a sound wave.

  • Practical investigation: the frequency of a sound wave using an oscilloscope.

  • How the pitch of a sound relates to the frequency of vibration of the source.

  • How the loudness of a sound relates to the amplitude of vibration of the source.

Energy Resources and Energy Transfers

Units

  • Kilogram (kg)

  • Joule (J)

  • Metre (m)

  • Metre/second (m/s)

  • Metre/second squared (m/s²)

  • Newton (N)

  • Second (s)

  • Watt (W)

Energy Transfers

  • Energy transfers involving energy stores:

    • Energy stores: chemical, kinetic, gravitational, elastic, thermal, magnetic, electrostatic, nuclear

    • Energy transfers: mechanically, electrically, by heating, by radiation (light and sound)

  • Using the principle of conservation of energy.

  • Relationship between efficiency, useful energy output, and total energy output: efficiency=usefulenergyoutputtotalenergyoutput×100%efficiency = \frac{useful \, energy \, output}{total \, energy \, output} \times 100\%

  • Describing a variety of everyday and scientific devices and situations, explaining the transfer of the input energy in terms of the above relationship, including their representation by Sankey diagrams.

  • How thermal energy transfer may take place by conduction, convection, and radiation.

  • The role of convection in everyday phenomena.

  • How emission and absorption of radiation are related to surface and temperature.

  • Practical investigation: thermal energy transfer by conduction, convection, and radiation.

  • Ways of reducing unwanted energy transfer, such as insulation.

Work and Power

  • Relationship between work done, force and distance moved in the direction of the force: workdone=force×distancemovedwork \, done = force \times distance \, moved, which can be written as W=F×dW = F \times d

  • Work done is equal to energy transferred.

  • Relationship between gravitational potential energy, mass, gravitational field strength, and height: gravitationalpotentialenergy=mass×gravitationalfieldstrength×heightgravitational \, potential \, energy = mass \times gravitational \, field \, strength \times height, which can be written as GPE=m×g×hGPE = m \times g \times h

  • Relationship: kineticenergy=12×mass×speed2kinetic \, energy = \frac{1}{2} \times mass \times speed^2, which can be written as KE=12×m×v2KE = \frac{1}{2} \times m \times v^2

  • How conservation of energy produces a link between gravitational potential energy, kinetic energy, and work.

  • Power as the rate of transfer of energy or the rate of doing work.

  • Relationship between power, work done (energy transferred) and time taken: power=workdonetimetakenpower = \frac{work \, done}{time \, taken}, which can be written as P=WtP = \frac{W}{t}

Energy Resources and Electricity Generation

  • Energy transfers involved in generating electricity using:

    • Wind

    • Water

    • Geothermal resources

    • Solar heating systems

    • Solar cells

    • Fossil fuels

    • Nuclear power

  • Advantages and disadvantages of methods of large-scale electricity production from various renewable and non-renewable resources.

Solids, Liquids and Gases

Units

  • Degree Celsius (°C)

  • Kelvin (K)

  • Joule (J)

  • Kilogram (kg)

  • Kilogram/metre cubed (kg/m³)

  • Metre (m)

  • Metre squared (m²)

  • Metre cubed (m³)

  • Metre/second (m/s)

  • Metre/second squared (m/s²)

  • Newton (N)

  • Pascal (Pa)

  • Joules/kilogram degree Celsius (J/kg °C)

Density and Pressure

  • Relationship between density, mass and volume: density=massvolumedensity = \frac{mass}{volume}, which can be written as ρ=mVρ = \frac{m}{V}

  • Practical investigation: density using direct measurements of mass and volume.

  • Relationship between pressure, force and area: pressure=forceareapressure = \frac{force}{area}, which can be written as p=FAp = \frac{F}{A}

  • How the pressure at a point in a gas or liquid at rest acts equally in all directions.

  • Relationship for pressure difference: pressuredifference=height×density×gravitationalfieldstrengthpressure \, difference = height \times density \times gravitational \, field \, strength, which can be written as p=h×ρ×gp = h \times ρ \times g

Change of State

  • Why heating a system will change the energy stored within the system and raise its temperature or produce changes of state.

  • Changes that occur when a solid melts to form a liquid, and when a liquid evaporates or boils to form a gas.

  • Arrangement and motion of particles in solids, liquids and gases.

  • Practical: obtain a temperature–time graph to show the constant temperature during a change of state

  • Specific heat capacity is the energy required to change the temperature of an object by one degree Celsius per kilogram of mass (J/kg °C).

  • Equation: changeinthermalenergy=mass×specificheatcapacity×changeintemperaturechange \, in \, thermal \, energy = mass \times specific \, heat \, capacity \times change \, in \, temperature, which can be written as ΔQ=m×c×ΔTΔQ = m \times c \times ΔT

  • Practical investigation: the specific heat capacity of materials including water and some solids

Ideal Gas Molecules

  • How molecules in a gas have random motion and that they exert a force, and hence a pressure, on the walls of a container.

  • Why there is an absolute zero of temperature, which is –273 °C.

  • Description of the Kelvin scale of temperature and be able to convert between the Kelvin and Celsius scales.

  • Why an increase in temperature results in an increase in the average speed of gas molecules.

  • Kelvin temperature of a gas is proportional to the average kinetic energy of its molecules.

  • For a fixed amount of gas, the qualitative relationship between:

    • pressure and volume at constant temperature

    • pressure and Kelvin temperature at constant volume

  • Relationship between the pressure and Kelvin temperature of a fixed mass of gas at constant volume: p<em>1T</em>1=p<em>2T</em>2\frac{p<em>1}{T</em>1} = \frac{p<em>2}{T</em>2}

  • Relationship between the pressure and volume of a fixed mass of gas at constant temperature:p<em>1V</em>1=p<em>2V</em>2p<em>1V</em>1 = p<em>2V</em>2

Magnetism and Electromagnetism

Units

  • Ampere (A)

  • Volt (V)

  • Watt (W)

Magnetism

  • Magnets repel and attract other magnets and attract magnetic substances.

  • Properties of magnetically hard and soft materials.

  • Understanding the term 'magnetic field line'.

  • Magnetism is induced in some materials when they are placed in a magnetic field.

  • Practical investigation: the magnetic field pattern for a permanent bar magnet and between two bar magnets.

  • How to use two permanent magnets to produce a uniform magnetic field pattern.

Electromagnetism

  • An electric current in a conductor produces a magnetic field around it.

  • Construction of electromagnets.

  • Drawing magnetic field patterns for a straight wire, a flat circular coil and a solenoid when each is carrying a current.

  • There is a force on a charged particle when it moves in a magnetic field as long as its motion is not parallel to the field.

  • Why a force is exerted on a current-carrying wire in a magnetic field and how this effect is applied in simple d.c. electric motors and loudspeakers.

  • Using the left-hand rule to predict the direction of the resulting force when a wire carries a current perpendicular to a magnetic field.

  • How the force on a current-carrying conductor in a magnetic field changes with the magnitude and direction of the field and current.

Electromagnetic Induction

  • A voltage is induced in a conductor or a coil when it moves through a magnetic field or when a magnetic field changes through it and describe the factors that affect the size of the induced voltage.

  • Generation of electricity by the rotation of a magnet within a coil of wire and of a coil of wire within a magnetic field, and describe the factors that affect the size of the induced voltage.

  • Description of the structure of a transformer and understand that a transformer changes the size of an alternating voltage by having different numbers of turns on the input and output sides.

  • Explanation of the use of step-up and step-down transformers in the large-scale generation and transmission of electrical energy.

  • Relationship between input (primary) and output (secondary) voltages and the turns ratio for a transformer: input(primary)voltageoutput(secondary)voltage=primaryturnssecondaryturns\frac{input \, (primary) \, voltage}{output \, (secondary) \, voltage} = \frac{primary \, turns}{secondary \, turns}

  • Relationship: input power = output power for 100% efficiency: V<em>p×I</em>p=V<em>s×I</em>sV<em>p \times I</em>p = V<em>s \times I</em>s

Radioactivity and Particles

Units

  • Becquerel (Bq)

  • Centimetre (cm)

  • Hour (h)

  • Minute (min)

  • Second (s)

Radioactivity

  • Description of the structure of an atom in terms of protons, neutrons and electrons and use symbols such as 614C^{14}_{6}C to describe particular nuclei.

  • Terms: atomic (proton) number, mass (nucleon) number and isotope.

  • Alpha (α) particles, beta (β−) particles, and gamma (γ) rays are ionizing radiations emitted from unstable nuclei in a random process.

  • Nature of alpha (α) particles, beta (β−) particles and gamma (γ) rays, and recall that they may be distinguished in terms of penetrating power and ability to ionise.

  • Practical investigation: the penetration powers of different types of radiation using either radioactive sources or simulations.

  • Effects on the atomic and mass numbers of a nucleus of the emission of each of the four main types of radiation (alpha, beta, gamma and neutron radiation).

  • How to balance nuclear equations in terms of mass and charge.

  • Photographic film or a Geiger−Müller detector can detect ionizing radiations.

  • Sources of background (ionizing) radiation from Earth and space.

  • The activity of a radioactive source decreases over a period of time and is measured in becquerels.

  • Definition of the term 'half-life' and understand that it is different for different radioactive isotopes.

  • Using the concept of the half-life to carry out simple calculations on activity, including graphical methods.

  • Uses of radioactivity in industry and medicine.

  • Difference between contamination and irradiation.

  • Dangers of ionizing radiations, including:

    • Radiation can cause mutations in living organisms

    • Radiation can damage cells and tissue

    • Problems arising from the disposal of radioactive waste and how the associated risks can be reduced

Fission and Fusion

  • Nuclear reactions, including fission, fusion and radioactive decay, can be a source of energy.

  • How a nucleus of U-235 can be split (the process of fission) by collision with a neutron and that this process releases energy as kinetic energy of the fission products.

  • The fission of U-235 produces two radioactive daughter nuclei and a small number of neutrons.

  • How a chain reaction can be set up if the neutrons produced by one fission strike other U-235 nuclei.

  • Role played by the control rods and moderator in the fission process.

  • The role of shielding around a nuclear reactor.

  • Difference between nuclear fusion and nuclear fission.

  • Nuclear fusion as the creation of larger nuclei resulting in a loss of mass from smaller nuclei, accompanied by a release of energy.

  • Fusion is the energy source for stars.

  • Why nuclear fusion does not happen at low temperatures and pressures, due to electrostatic repulsion of protons

Astrophysics

Units

  • Kilogram (kg)

  • Metre (m)

  • Metre/second (m/s)

  • Metre/second squared (m/s²)

  • Newton (N)

  • Second (s)

  • Newton/kilogram (N/kg)

Motion in the Universe

  • The universe is a large collection of billions of galaxies.

  • A galaxy is a large collection of billions of stars.

  • Our solar system is in the Milky Way galaxy.

  • Why gravitational field strength, g, varies and know that it is different on other planets and the Moon from that on the Earth.

  • Gravitational force:

    • Causes moons to orbit planets

    • Causes the planets to orbit the Sun

    • Causes artificial satellites to orbit the Earth

    • Causes comets to orbit the Sun

  • Differences in the orbits of comets, moons and planets.

  • Relationship between orbital speed, orbital radius and time period: orbitalspeed=2×π×orbitalradiustimeperiodorbital \, speed = \frac{2 \times π \times orbital \, radius}{time \, period}, which can be written as v=2×π×rTv = \frac{2 \times π \times r}{T}

Stellar Evolution

  • How stars can be classified according to their color.

  • A star’s color is related to its surface temperature.

  • Evolution of stars of similar mass to the Sun through the following stages:

    • Nebula

    • Star (main sequence)

    • Red giant

    • White dwarf

  • Evolution of stars with a mass larger than the Sun.

  • How the brightness of a star at a standard distance can be represented using absolute magnitude.

  • Drawing the main components of the Hertzsprung–Russell diagram (HR diagram)

Cosmology

  • Description of the past evolution of the universe and the main arguments in favor of the Big Bang theory.

  • Description of evidence that supports the Big Bang theory

    • Red-shift

    • Cosmic microwave background (CMB) radiation

  • Description that if a wave source is moving relative to an observer, there will be a change in the observed frequency and wavelength.

  • Equation relating to change in wavelength, reference wavelength, velocity of a galaxy and the speed of light: velocityofagalaxyspeedoflight=changeinwavelengthreferencewavelength\frac{velocity \, of \, a \, galaxy}{speed \, of \, light} = \frac{change \, in \, wavelength}{reference \, wavelength}, which can be written as vc=Δλλ0\frac{v}{c} = \frac{Δλ}{λ_0}

  • Description of the red-shift in light received from galaxies at different distances away from the Earth.

  • Explanation of why the red-shift of galaxies provides evidence for the expansion of the universe.