ScholaFly

Edexcel GCSE 1PH0 Physics specification: every spec point and its video lesson

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SpecStatementLessonYT search phrase
1.1Edexcel 1PH0Recall and use the SI unit for physical quantities, as listed in Appendix 3Units, prefixes and standard form in physicsScholaFly PH01-01
1.2Edexcel 1PH0Recall and use multiples and sub-multiples of units, including giga (G), mega (M), kilo (k), centi (c), milli (m), micro (μ) and nano (n)Units, prefixes and standard form in physicsScholaFly PH01-01
1.3Edexcel 1PH0Be able to convert between different units, including hours to secondsUnits, prefixes and standard form in physicsScholaFly PH01-01
1.4Edexcel 1PH0Use significant figures and standard form where appropriateUnits, prefixes and standard form in physicsScholaFly PH01-01
2.1Edexcel 1PH0Explain that a scalar quantity has magnitude (size) but no specific directionScalars and vectorsScholaFly PH01-02
Distance and displacementScholaFly PH01-03
VelocityScholaFly PH01-05
2.2Edexcel 1PH0Explain that a vector quantity has both magnitude (size) and a specific directionScalars and vectorsScholaFly PH01-02
Distance and displacementScholaFly PH01-03
VelocityScholaFly PH01-05
2.3Edexcel 1PH0Explain the difference between vector and scalar quantitiesScalars and vectorsScholaFly PH01-02
Distance and displacementScholaFly PH01-03
VelocityScholaFly PH01-05
2.4Edexcel 1PH0Recall vector and scalar quantities, including: a displacement/distance b velocity/speed c acceleration d force e weight/mass f momentum g energyScalars and vectorsScholaFly PH01-02
Distance and displacementScholaFly PH01-03
VelocityScholaFly PH01-05
2.5Edexcel 1PH0Recall that velocity is speed in a stated directionScalars and vectorsScholaFly PH01-02
Distance and displacementScholaFly PH01-03
VelocityScholaFly PH01-05
2.6Edexcel 1PH0Recall and use the equations: a (average) speed (metre per second, m/s) = distance (metre, m) ÷ time (s) b distance travelled (metre, m) = average speed (metre per second, m/s) × time (s)Speed, typical speeds and s = vtScholaFly PH01-04
2.7Edexcel 1PH0Analyse distance/time graphs including determination of speed from the gradientDistance-time graphsScholaFly PH02-01
2.8Edexcel 1PH0Recall and use the equation: acceleration (metre per second squared, m/s2) = change in velocity (metre per second, m/s) ÷ time taken (second, s)Acceleration and velocity-time graphsScholaFly PH02-03
2.9Edexcel 1PH0Use the equation: (final velocity)2 ((metre/second)2, (m/s)2) – (initial velocity)2 ((metre/second)2, (m/s)2) = 2 × acceleration (metre per second squared, m/s2) × distance (metre, m)The uniform acceleration equation: v^2 - u^2 = 2asScholaFly PH02-05
2.10Edexcel 1PH0Analyse velocity/time graphs to: a compare acceleration from gradients qualitatively b calculate the acceleration from the gradient (for uniform acceleration only) c determine the distance travelled using the area between the graph line and the time axis (for uniform acceleration only)Acceleration and velocity-time graphsScholaFly PH02-03
Distance from the area under a velocity-time graphScholaFly PH02-04
2.11Edexcel 1PH0Describe a range of laboratory methods for determining the speeds of objects such as the use of light gatesMeasuring speed in the laboratoryScholaFly PH01-06
2.12Edexcel 1PH0Recall some typical speeds encountered in everyday experience for wind and sound, and for walking, running, cycling and other transportation systemsSpeed, typical speeds and s = vtScholaFly PH01-04
2.13Edexcel 1PH0Recall that the acceleration, g, in free fall is 10 m/s2 and be able to estimate the magnitudes of everyday accelerationsSpeed, typical speeds and s = vtScholaFly PH01-04
2.14Edexcel 1PH0Recall Newton’s first law and use it in the following situations: a where the resultant force on a body is zero, i.e. the body is moving at a constant velocity or is at rest b where the resultant force is not zero, i.e. the speed and/or direction of the body change(s)Newton's First LawScholaFly PH04-01
2.15Edexcel 1PH0Recall and use Newton’s second law as: force (newton, N) = mass (kilogram, kg) × acceleration (metre per second squared, m/s2)Newton's Second Law: F = maScholaFly PH04-02
2.16Edexcel 1PH0Define weight, recall and use the equation: weight (newton, N) = mass (kilogram, kg) × gravitational field strength (newton per kilogram, N/kg)Weight, mass and gravitational field strengthScholaFly PH03-02
2.17Edexcel 1PH0Describe how weight is measuredWeight, mass and gravitational field strengthScholaFly PH03-02
2.18Edexcel 1PH0Describe the relationship between the weight of a body and the gravitational field strengthWeight, mass and gravitational field strengthScholaFly PH03-02
2.19Edexcel 1PH0Core Practical: Investigate the relationship between force, mass and acceleration by varying the masses added to trolleysPractical: acceleration, force and massScholaFly PH24-05
2.20Edexcel 1PH0Explain that an object moving in a circular orbit at constant speed has a changing velocity (qualitative only)Circular motion: constant speed, changing velocity (Higher)ScholaFly PH04-06
2.21Edexcel 1PH0Explain that for motion in a circle there must be a resultant force known as a centripetal force that acts towards the centre of the circleCircular motion: constant speed, changing velocity (Higher)ScholaFly PH04-06
2.22Edexcel 1PH0Explain that inertial mass is a measure of how difficult it is to change the velocity of an object (including from rest) and know that it is defined as the ratio of force over accelerationInertia and inertial mass (Higher)ScholaFly PH04-03
2.23Edexcel 1PH0Recall and apply Newton’s third law both to equilibrium situations and to collision interactions and relate it to the conservation of momentum in collisionsNewton's Third LawScholaFly PH04-04
Conservation of momentum (Higher)ScholaFly PH07-06
2.24Edexcel 1PH0Define momentum, recall and use the equation: momentum (kilogram metre per second, kg m/s) = mass (kilogram, kg) × velocity (metre per second, m/s)Momentum and p = mv (Higher)ScholaFly PH07-05
Conservation of momentum (Higher)ScholaFly PH07-06
2.25Edexcel 1PH0Describe examples of momentum in collisionsMomentum and p = mv (Higher)ScholaFly PH07-05
Conservation of momentum (Higher)ScholaFly PH07-06
2.26Edexcel 1PH0Use Newton’s second law as: force (newton, N) = change in momentum (kilogram metre per second, kg m/s) ÷ time (second, s)Force as the rate of change of momentum, and impact forcesScholaFly PH07-07
2.27Edexcel 1PH0Explain methods of measuring human reaction times and recall typical resultsReaction time and thinking distanceScholaFly PH07-01
2.28Edexcel 1PH0Recall that the stopping distance of a vehicle is made up of the sum of the thinking distance and the braking distanceStopping distanceScholaFly PH07-02
2.29Edexcel 1PH0Explain that the stopping distance of a vehicle is affected by a range of factors including: a the mass of the vehicle b the speed of the vehicle c the driver’s reaction time d the state of the vehicle’s brakes e the state of the road f the amount of friction between the tyre and the road surfaceStopping distanceScholaFly PH07-02
2.30Edexcel 1PH0Describe the factors affecting a driver’s reaction time including drugs and distractionsReaction time and thinking distanceScholaFly PH07-01
2.31Edexcel 1PH0Explain the dangers caused by large decelerations and estimate the forces involved in typical situations on a public roadBraking, energy and large decelerationsScholaFly PH07-03
Estimating the forces in a road-vehicle deceleration (Higher)ScholaFly PH07-04
2.32PEdexcel 1PH0Estimate how the distance required for a road vehicle to stop in an emergency varies over a range of typical speedsEstimating how stopping distance grows with speed (triple)ScholaFly PH07-08
2.33PEdexcel 1PH0Carry out calculations on work done to show the dependence of braking distance for a vehicle on initial velocity squared (work done to bring a vehicle to rest equals its initial kinetic energy)Estimating how stopping distance grows with speed (triple)ScholaFly PH07-08
3.1Edexcel 1PH0Recall and use the equation to calculate the change in gravitational PE when an object is raised above the ground: change in gravitational potential energy (joule, J) = mass (kilogram, kg) × gravitational field strength (newton per kilogram, N/kg) × change in vertical height (metre, m) GPE ∆Gravitational potential energyScholaFly PH05-06
3.2Edexcel 1PH0Recall and use the equation to calculate the amounts of energy associated with a moving object: kinetic energy (joule, J) = × mass (kilogram, kg) × (speed)2 ((metre/second)2, (m/s)2)Kinetic energyScholaFly PH05-05
3.3Edexcel 1PH0Draw and interpret diagrams to represent energy transfersEnergy transfer diagrams and the common scaleScholaFly PH05-02
3.4Edexcel 1PH0Explain what is meant by conservation of energyConservation of energy and dissipationScholaFly PH06-01
3.5Edexcel 1PH0Analyse the changes involved in the way energy is stored when a system changes, including: a an object projected upwards or up a slope b a moving object hitting an obstacle c an object being accelerated by a constant force d a vehicle slowing down e bringing water to a boil in an electric kettleEnergy stores and the three ways a system's energy changesScholaFly PH05-01
3.6Edexcel 1PH0Explain that where there are energy transfers in a closed system there is no net change to the total energy in that systemConservation of energy and dissipationScholaFly PH06-01
3.7Edexcel 1PH0Explain that mechanical processes become wasteful when they cause a rise in temperature so dissipating energy in heating the surroundingsConservation of energy and dissipationScholaFly PH06-01
3.8Edexcel 1PH0Explain, using examples, how in all system changes energy is dissipated so that it is stored in less useful waysConservation of energy and dissipationScholaFly PH06-01
3.9Edexcel 1PH0Explain ways of reducing unwanted energy transfer including through lubrication, thermal insulationReducing unwanted energy transfersScholaFly PH06-02
3.10Edexcel 1PH0Describe the effects of the thickness and thermal conductivity of the walls of a building on its rate of cooling qualitativelyReducing unwanted energy transfersScholaFly PH06-02
3.11Edexcel 1PH0Recall and use the equation: device the plied sup energy total device the transferre energy useful efficiency =EfficiencyScholaFly PH06-03
3.12Edexcel 1PH0Explain how efficiency can be increasedIncreasing efficiency (Higher)ScholaFly PH06-04
3.13Edexcel 1PH0Describe the main energy sources available for use on Earth (including fossil fuels, nuclear fuel, bio-fuel, wind, hydro- electricity, the tides and the Sun), and compare the ways in which both renewable and non-renewable sources are usedEnergy resources and how we use themScholaFly PH06-05
Reliability, environmental impact and the move away from fossil fuelsScholaFly PH06-06
3.14Edexcel 1PH0Explain patterns and trends in the use of energy resourcesEnergy resources and how we use themScholaFly PH06-05
Reliability, environmental impact and the move away from fossil fuelsScholaFly PH06-06
4.1Edexcel 1PH0Recall that waves transfer energy and information without transferring matterWhat a wave does: energy without matterScholaFly PH15-01
4.2Edexcel 1PH0Describe evidence that with water and sound waves it is the wave and not the water or air itself that travelsWhat a wave does: energy without matterScholaFly PH15-01
4.3Edexcel 1PH0Define and use the terms frequency and wavelength as applied to wavesAmplitude, wavelength, frequency and periodScholaFly PH15-03
4.4Edexcel 1PH0Use the terms amplitude, period, wave velocity and wavefront as applied to wavesAmplitude, wavelength, frequency and periodScholaFly PH15-03
4.5Edexcel 1PH0Describe the difference between longitudinal and transverse waves by referring to sound, electromagnetic, seismic and water wavesTransverse and longitudinal wavesScholaFly PH15-02
4.6Edexcel 1PH0Recall and use both the equations below for all waves: wave speed (metre/second, m/s) = frequency (hertz, Hz) × wavelength (metre, m) wave speed (metre/second, m/s) = distance (metre, m) ÷ time (second, s)The wave equationScholaFly PH15-04
4.7Edexcel 1PH0Describe how to measure the velocity of sound in air and ripples on water surfacesMeasuring the speed of a waveScholaFly PH15-05
4.8PEdexcel 1PH0Calculate depth or distance from time and wave velocityUltrasound, infrasound and echo sounding (triple, Higher)ScholaFly PH16-03
Seismic waves and the Earth's structure (triple, Higher)ScholaFly PH16-04
4.9PEdexcel 1PH0Describe the effects of a reflection b refraction c transmission d absorption of waves at material interfacesReflection, transmission and absorption at a boundary (triple)ScholaFly PH18-03
4.10Edexcel 1PH0Explain how waves will be refracted at a boundary in terms of the change of direction and speedRefraction at a boundaryScholaFly PH18-01
4.11Edexcel 1PH0Recall that different substances may absorb, transmit, refract or reflect waves in ways that vary with wavelengthHow different substances treat different wavelengths (Higher)ScholaFly PH18-02
4.12PEdexcel 1PH0Describe the processes which convert wave disturbances between sound waves and vibrations in solids, and a explain why such processes only work over a limited frequency range b use this to explain the way the human ear worksSound, the ear and the limits of human hearing (triple, Higher)ScholaFly PH16-02
4.13PEdexcel 1PH0Recall that sound with frequencies greater than 20 000 hertz, Hz, is known as ultrasoundUltrasound, infrasound and echo sounding (triple, Higher)ScholaFly PH16-03
Seismic waves and the Earth's structure (triple, Higher)ScholaFly PH16-04
4.14PEdexcel 1PH0Recall that sound with frequencies less than 20 hertz, Hz, is known as infrasoundUltrasound, infrasound and echo sounding (triple, Higher)ScholaFly PH16-03
Seismic waves and the Earth's structure (triple, Higher)ScholaFly PH16-04
4.15PEdexcel 1PH0Explain uses of ultrasound and infrasound, including a sonar b foetal scanning c exploration of the Earth’s coreUltrasound, infrasound and echo sounding (triple, Higher)ScholaFly PH16-03
Seismic waves and the Earth's structure (triple, Higher)ScholaFly PH16-04
4.16PEdexcel 1PH0Describe how changes, if any, in velocity, frequency and wavelength, in the transmission of sound waves from one medium to another are inter-relatedSound crossing from one medium to another (triple)ScholaFly PH16-01
4.17Edexcel 1PH0Core Practical: Investigate the suitability of equipment to measure the speed, frequency and wavelength of a wave in a solid and a fluidPractical: waves in a ripple tank and in a solidScholaFly PH24-08
5.1PEdexcel 1PH0Explain, with the aid of ray diagrams, reflection, refraction and total internal reflection (TIR), including the law of reflection and critical angleTotal internal reflection and the critical angle (triple)ScholaFly PH18-04
5.2PEdexcel 1PH0Explain the difference between specular and diffuse reflectionColour, filters, and specular versus diffuse reflection (triple)ScholaFly PH18-06
5.3PEdexcel 1PH0Explain how colour of light is related to a differential absorption at surfaces b transmission of light through filtersColour, filters, and specular versus diffuse reflection (triple)ScholaFly PH18-06
5.4PEdexcel 1PH0Relate the power of a lens to its focal length and shapeLenses and ray diagrams (triple)ScholaFly PH18-05
5.5PEdexcel 1PH0Use ray diagrams to show the similarities and differences in the refraction of light by converging and diverging lensesLenses and ray diagrams (triple)ScholaFly PH18-05
5.6PEdexcel 1PH0Explain the effects of different types of lens in producing real and virtual imagesLenses and ray diagrams (triple)ScholaFly PH18-05
5.7Edexcel 1PH0Recall that all electromagnetic waves are transverse, that they travel at the same speed in a vacuumThe electromagnetic spectrumScholaFly PH17-01
5.8Edexcel 1PH0Explain, with examples, that all electromagnetic waves transfer energy from source to observerThe electromagnetic spectrumScholaFly PH17-01
5.9Edexcel 1PH0Core Practical: Investigate refraction in rectangular glass blocks in terms of the interaction of electromagnetic waves with matterPractical: reflection and refraction of lightScholaFly PH24-09
5.10Edexcel 1PH0Recall the main groupings of the continuous electromagnetic spectrum including (in order) radio waves, microwaves, infrared, visible (including the colours of the visible spectrum), ultraviolet, x-rays and gamma raysThe electromagnetic spectrumScholaFly PH17-01
5.11Edexcel 1PH0Describe the electromagnetic spectrum as continuous from radio waves to gamma rays and that the radiations within it can be grouped in order of decreasing wavelength and increasing frequencyThe electromagnetic spectrumScholaFly PH17-01
5.12Edexcel 1PH0Recall that our eyes can only detect a limited range of frequencies of electromagnetic radiationThe electromagnetic spectrumScholaFly PH17-01
5.13Edexcel 1PH0Recall that different substances may absorb, transmit, refract or reflect electromagnetic waves in ways that vary with wavelengthHow different substances treat different wavelengths (Higher)ScholaFly PH18-02
5.14Edexcel 1PH0Explain the effects of differences in the velocities of electromagnetic waves in different substancesHow different substances treat different wavelengths (Higher)ScholaFly PH18-02
5.15PEdexcel 1PH0Explain that all bodies emit radiation, that the intensity and wavelength distribution of any emission depends on their temperatureInfrared emission and absorption, and black-body radiation (triple)ScholaFly PH17-05
5.16PEdexcel 1PH0Explain that for a body to be at a constant temperature it needs to radiate the same average power that it absorbsRadiation balance and the temperature of the Earth (triple, Higher)ScholaFly PH17-06
5.17PEdexcel 1PH0Explain what happens to a body if the average power it radiates is less or more than the average power that it absorbsRadiation balance and the temperature of the Earth (triple, Higher)ScholaFly PH17-06
5.18PEdexcel 1PH0Explain how the temperature of the Earth is affected by factors controlling the balance between incoming radiation and radiation emittedRadiation balance and the temperature of the Earth (triple, Higher)ScholaFly PH17-06
5.19PEdexcel 1PH0Core Practical: Investigate how the nature of a surface affects the amount of thermal energy radiated or absorbedPractical: infrared emission and absorptionScholaFly PH24-10
5.20Edexcel 1PH0Recall that the potential danger associated with an electromagnetic wave increases with increasing frequencyThe hazards of electromagnetic radiationScholaFly PH17-03
5.21Edexcel 1PH0Describe the harmful effects on people of excessive exposure to electromagnetic radiation, including: a microwaves: internal heating of body cells b infrared: skin burns c ultraviolet: damage to surface cells and eyes, leading to skin cancer and eye conditions d x-rays and gamma rays: mutation or damage to cells in the bodyThe hazards of electromagnetic radiationScholaFly PH17-03
5.22Edexcel 1PH0Describe some uses of electromagnetic radiation a radio waves: including broadcasting, communications and satellite transmissions b microwaves: including cooking, communications and satellite transmissions c infrared: including cooking, thermal imaging, short range communications, optical fibres, television remote controls and security systems d visible light: including vision, photography and illumination e ultraviolet: including security marking, fluorescent lamps, detecting forged bank notes and disinfecting water f x-rays: including observing the internal structure of objects, airport security scanners and medical x-rays g gamma rays: including sterilising food and medical equipment, and the detection of cancer and its treatmentUses of each part of the electromagnetic spectrumScholaFly PH17-02
5.23Edexcel 1PH0Recall that radio waves can be produced by, or can themselves induce, oscillations in electrical circuitsRadio waves and electrical oscillations (Higher)ScholaFly PH17-04
5.24Edexcel 1PH0Recall that changes in atoms and nuclei can a generate radiations over a wide frequency range b be caused by absorption of a range of radiationsRadiation from atoms and nucleiScholaFly PH19-05
6.1Edexcel 1PH0Describe an atom as a positively charged nucleus, consisting of protons and neutrons, surrounded by negatively charged electrons, with the nuclear radius much smaller than that of the atom and with almost all of the mass in the nucleusThe structure and size of an atomScholaFly PH19-01
6.2Edexcel 1PH0Recall the typical size (order of magnitude) of atoms and small moleculesThe structure and size of an atomScholaFly PH19-01
6.3Edexcel 1PH0Describe the structure of nuclei of isotopes using the terms atomic (proton) number and mass (nucleon) number and using symbols in the format using symbols in the formatAtomic number, mass number and isotopesScholaFly PH19-03
6.4Edexcel 1PH0Recall that the nucleus of each element has a characteristic positive charge, but that isotopes of an element differ in mass by having different numbers of neutronsAtomic number, mass number and isotopesScholaFly PH19-03
6.5Edexcel 1PH0Recall the relative masses and relative electric charges of protons, neutrons, electrons and positronsProtons, neutrons and electronsScholaFly PH19-02
6.6Edexcel 1PH0Recall that in an atom the number of protons equals the number of electrons and is therefore neutralProtons, neutrons and electronsScholaFly PH19-02
6.7Edexcel 1PH0Recall that in each atom its electrons orbit the nucleus at different set distances from the nucleusElectron energy levels and ionsScholaFly PH19-04
6.8Edexcel 1PH0Explain that electrons change orbit when there is absorption or emission of electromagnetic radiationElectron energy levels and ionsScholaFly PH19-04
6.9Edexcel 1PH0Explain how atoms may form positive ions by losing outer electronsElectron energy levels and ionsScholaFly PH19-04
6.10Edexcel 1PH0Recall that alpha, β– (beta minus), β+ (positron), gamma rays and neutron radiation are emitted from unstable nuclei in a random processAlpha, beta, gamma and neutron radiation comparedScholaFly PH20-02
6.11Edexcel 1PH0Recall that alpha, β– (beta minus), β+ (positron) and gamma rays are ionising radiationsAlpha, beta, gamma and neutron radiation comparedScholaFly PH20-02
6.12Edexcel 1PH0Explain what is meant by background radiationBackground radiationScholaFly PH21-01
6.13Edexcel 1PH0Describe the origins of background radiation from Earth and spaceBackground radiationScholaFly PH21-01
6.14Edexcel 1PH0Describe methods for measuring and detecting radioactivity limited to photographic film and a Geiger–Müller tubeDetecting radioactivityScholaFly PH20-03
6.15Edexcel 1PH0Recall that an alpha particle is equivalent to a helium nucleus, a beta particle is an electron emitted from the nucleus and a gamma ray is electromagnetic radiationAlpha, beta, gamma and neutron radiation comparedScholaFly PH20-02
6.16Edexcel 1PH0Compare alpha, beta and gamma radiations in terms of their abilities to penetrate and ioniseAlpha, beta, gamma and neutron radiation comparedScholaFly PH20-02
6.17Edexcel 1PH0Describe how and why the atomic model has changed over time including reference to the plum pudding model and Rutherford alpha particle scattering leading to the Bohr modelHow the model of the atom changedScholaFly PH19-06
6.18Edexcel 1PH0Describe the process of β– decay (a neutron becomes a proton plus an electron)Nuclear equations for alpha and beta decayScholaFly PH20-04
6.19Edexcel 1PH0Describe the process of β+ decay (a proton becomes a neutron plus a positron)Nuclear equations for alpha and beta decayScholaFly PH20-04
6.20Edexcel 1PH0Explain the effects on the atomic (proton) number and mass (nucleon) number of radioactive decays (α, β, γ and neutron emission)Nuclear equations for alpha and beta decayScholaFly PH20-04
6.21Edexcel 1PH0Recall that nuclei that have undergone radioactive decay often undergo nuclear rearrangement with a loss of energy as gamma radiationNuclear equations for alpha and beta decayScholaFly PH20-04
6.22Edexcel 1PH0Use given data to balance nuclear equations in terms of mass and chargeNuclear equations for alpha and beta decayScholaFly PH20-04
6.23Edexcel 1PH0Describe how the activity of a radioactive source decreases over a period of timeRadioactive decay is random: activity and count-rateScholaFly PH20-01
Half-lifeScholaFly PH20-05
Net decline after a number of half-livesScholaFly PH20-06
6.24Edexcel 1PH0Recall that the unit of activity of a radioactive isotope is the Becquerel, BqRadioactive decay is random: activity and count-rateScholaFly PH20-01
Half-lifeScholaFly PH20-05
Net decline after a number of half-livesScholaFly PH20-06
6.25Edexcel 1PH0Explain that the half-life of a radioactive isotope is the time taken for half the undecayed nuclei to decay or the activity of a source to decay by halfRadioactive decay is random: activity and count-rateScholaFly PH20-01
Half-lifeScholaFly PH20-05
Net decline after a number of half-livesScholaFly PH20-06
6.26Edexcel 1PH0Explain that it cannot be predicted when a particular nucleus will decay but half-life enables the activity of a very large number of nuclei to be predicted during the decay processRadioactive decay is random: activity and count-rateScholaFly PH20-01
Half-lifeScholaFly PH20-05
Net decline after a number of half-livesScholaFly PH20-06
6.27Edexcel 1PH0Use the concept of half-life to carry out simple calculations on the decay of a radioactive isotope, including graphical representationsRadioactive decay is random: activity and count-rateScholaFly PH20-01
Half-lifeScholaFly PH20-05
Net decline after a number of half-livesScholaFly PH20-06
6.28PEdexcel 1PH0Describe uses of radioactivity, including: a household fire (smoke) alarms b irradiating food c sterilisation of equipment d tracing and gauging thicknesses e diagnosis and treatment of cancerUses of radioactivity in medicine and industry (triple)ScholaFly PH21-05
6.29Edexcel 1PH0Describe the dangers of ionising radiation in terms of tissue damage and possible mutations and relate this to the precautions neededThe dangers of ionising radiation and the precautions takenScholaFly PH21-03
6.30PEdexcel 1PH0Explain how the dangers of ionising radiation depend on half- life and relate this to the precautions neededWhy the hazard of a source depends on its half-life (triple)ScholaFly PH21-04
6.31Edexcel 1PH0Explain the precautions taken to ensure the safety of people exposed to radiation, including limiting the dose for patients and the risks to medical personnelThe dangers of ionising radiation and the precautions takenScholaFly PH21-03
6.32Edexcel 1PH0Describe the differences between contamination and irradiation effects and compare the hazards associated with these twoContamination and irradiationScholaFly PH21-02
6.33PEdexcel 1PH0Compare and contrast the treatment of tumours using radiation applied internally or externallyUses of radioactivity in medicine and industry (triple)ScholaFly PH21-05
6.34PEdexcel 1PH0Explain some of the uses of radioactive substances in diagnosis of medical conditions, including PET scanners and tracersUses of radioactivity in medicine and industry (triple)ScholaFly PH21-05
6.35PEdexcel 1PH0Explain why isotopes used in PET scanners have to be produced nearbyUses of radioactivity in medicine and industry (triple)ScholaFly PH21-05
6.36PEdexcel 1PH0Evaluate the advantages and disadvantages of nuclear power for generating electricity, including the lack of carbon dioxide emissions, risks, public perception, waste disposal and safety issuesNuclear power: the arguments for and against (triple)ScholaFly PH21-08
6.37PEdexcel 1PH0Recall that nuclear reactions, including fission, fusion and radioactive decay, can be a source of energyNuclear fission and the chain reaction (triple)ScholaFly PH21-06
6.38PEdexcel 1PH0Explain how the fission of U-235 produces two daughter nuclei and the emission of two or more neutrons, accompanied by a release of energyNuclear fission and the chain reaction (triple)ScholaFly PH21-06
6.39PEdexcel 1PH0Explain the principle of a controlled nuclear chain reactionNuclear fission and the chain reaction (triple)ScholaFly PH21-06
6.40PEdexcel 1PH0Explain how the chain reaction is controlled in a nuclear reactor, including the action of moderators and control rodsNuclear fission and the chain reaction (triple)ScholaFly PH21-06
6.41PEdexcel 1PH0Describe how thermal (heat) energy from the chain reaction is used in the generation of electricity in a nuclear power stationNuclear fission and the chain reaction (triple)ScholaFly PH21-06
6.42PEdexcel 1PH0Recall that the products of nuclear fission are radioactiveNuclear fission and the chain reaction (triple)ScholaFly PH21-06
6.43PEdexcel 1PH0Describe nuclear fusion as the creation of larger nuclei resulting in a loss of mass from smaller nuclei, accompanied by a release of energy, and recognise fusion as the energy source for starsNuclear fusion (triple)ScholaFly PH21-07
6.44PEdexcel 1PH0Explain the difference between nuclear fusion and nuclear fissionNuclear fusion (triple)ScholaFly PH21-07
6.45PEdexcel 1PH0Explain why nuclear fusion does not happen at low temperatures and pressures, due to electrostatic repulsion of protonsNuclear fusion (triple)ScholaFly PH21-07
6.46PEdexcel 1PH0Relate the conditions for fusion to the difficulty of making a practical and economic form of power stationNuclear fusion (triple)ScholaFly PH21-07
7.1PEdexcel 1PH0Explain how and why both the weight of any body and the value of g differ between the surface of the Earth and the surface of other bodies in space, including the MoonWeight and gravitational field strength on other bodies (triple)ScholaFly PH22-03
7.2PEdexcel 1PH0Recall that our Solar System consists of the Sun (our star), eight planets and their natural satellites (such as our Moon); dwarf planets; asteroids and cometsThe Solar System and the Milky Way (triple)ScholaFly PH22-01
7.3PEdexcel 1PH0Recall the names and order, in terms of distance from the Sun, of the eight planetsThe Solar System and the Milky Way (triple)ScholaFly PH22-01
7.4PEdexcel 1PH0Describe how ideas about the structure of the Solar System have changed over timeHow ideas about the Solar System changed (triple)ScholaFly PH22-02
7.5PEdexcel 1PH0Describe the orbits of moons, planets, comets and artificial satellitesOrbits of moons, planets and satellites (triple)ScholaFly PH22-04
7.6PEdexcel 1PH0Explain for circular orbits how the force of gravity can lead to changing velocity of a planet but unchanged speedCircular orbits: gravity changes velocity, not speed (triple)ScholaFly PH22-05
7.7PEdexcel 1PH0Explain how, for a stable orbit, the radius must change if orbital speed changes (qualitative only)Circular orbits: gravity changes velocity, not speed (triple)ScholaFly PH22-05
7.8PEdexcel 1PH0Compare the Steady State and Big Bang theoriesThe Big Bang, the Steady State theory and the cosmic microwave background (triple)ScholaFly PH23-04
7.9PEdexcel 1PH0Describe evidence supporting the Big Bang theory, limited to red-shift and the cosmic microwave background (CMB) radiationThe Big Bang, the Steady State theory and the cosmic microwave background (triple)ScholaFly PH23-04
7.10PEdexcel 1PH0Recall that as there is more evidence supporting the Big Bang theory than the Steady State theory, it is the currently accepted model for the origin of the UniverseThe Big Bang, the Steady State theory and the cosmic microwave background (triple)ScholaFly PH23-04
7.11PEdexcel 1PH0Describe that if a wave source is moving relative to an observer there will be a change in the observed frequency and wavelengthRed-shift and the expanding Universe (triple)ScholaFly PH23-03
7.12PEdexcel 1PH0Describe the red-shift in light received from galaxies at different distances away from the EarthRed-shift and the expanding Universe (triple)ScholaFly PH23-03
7.13PEdexcel 1PH0Explain why the red-shift of galaxies provides evidence for the Universe expandingRed-shift and the expanding Universe (triple)ScholaFly PH23-03
7.14PEdexcel 1PH0Explain how both the Big Bang and Steady State theories of the origin of the Universe both account for red-shift of galaxiesRed-shift and the expanding Universe (triple)ScholaFly PH23-03
7.15PEdexcel 1PH0Explain how the discovery of the CMB radiation led to the Big Bang theory becoming the currently accepted modelRed-shift and the expanding Universe (triple)ScholaFly PH23-03
7.16PEdexcel 1PH0Describe the evolution of stars of similar mass to the Sun through the following stages: a nebula b star (main sequence) c red giant d white dwarfHow a star forms and why it is stable (triple)ScholaFly PH23-01
The life cycle of a star (triple)ScholaFly PH23-02
7.17PEdexcel 1PH0Explain how the balance between thermal expansion and gravity affects the life cycle of starsHow a star forms and why it is stable (triple)ScholaFly PH23-01
The life cycle of a star (triple)ScholaFly PH23-02
7.18PEdexcel 1PH0Describe the evolution of stars with a mass larger than the SunHow a star forms and why it is stable (triple)ScholaFly PH23-01
The life cycle of a star (triple)ScholaFly PH23-02
7.19PEdexcel 1PH0Describe how methods of observing the Universe have changed over time including why some telescopes are located outside the Earth’s atmosphereObserving the Universe (triple)ScholaFly PH23-05
8.1Edexcel 1PH0Describe the changes involved in the way energy is stored when systems changeEnergy stores and the three ways a system's energy changesScholaFly PH05-01
8.2Edexcel 1PH0Draw and interpret diagrams to represent energy transfersEnergy transfer diagrams and the common scaleScholaFly PH05-02
8.3Edexcel 1PH0Explain that where there are energy transfers in a closed system there is no net change to the total energy in that systemConservation of energy and dissipationScholaFly PH06-01
8.4Edexcel 1PH0Identify the different ways that the energy of a system can be changed a through work done by forces b in electrical equipment c in heatingEnergy stores and the three ways a system's energy changesScholaFly PH05-01
8.5Edexcel 1PH0Describe how to measure the work done by a force and understand that energy transferred (joule, J) is equal to work done (joule, J)Work done and energy transferScholaFly PH05-03
8.6Edexcel 1PH0Recall and use the equation: work done (joule, J) = force (newton, N) × distance moved in the direction of the force (metre, m)Work done and energy transferScholaFly PH05-03
8.7Edexcel 1PH0Describe and calculate the changes in energy involved when a system is changed by work done by forcesWork done and energy transferScholaFly PH05-03
8.8Edexcel 1PH0Recall and use the equation to calculate the change in gravitational PE when an object is raised above the ground: change in gravitational potential energy (joule, J) = mass (kilogram, kg) × gravitational field strength (newton per kilogram, N/kg) × change in vertical height (metre, m) GPE ∆Gravitational potential energyScholaFly PH05-06
8.9Edexcel 1PH0Recall and use the equation to calculate the amounts of energy associated with a moving object: kinetic energy (joule, J) = × mass (kilogram, kg) × (speed)2 ((metre/second)2, (m/s)2)Kinetic energyScholaFly PH05-05
8.10Edexcel 1PH0Explain, using examples, how in all system changes energy is dissipated so that it is stored in less useful waysConservation of energy and dissipationScholaFly PH06-01
8.11Edexcel 1PH0Explain that mechanical processes become wasteful when they cause a rise in temperature so dissipating energy in heating the surroundingsConservation of energy and dissipationScholaFly PH06-01
8.12Edexcel 1PH0Define power as the rate at which energy is transferred and use examples to explain this definitionPower as the rate of energy transferScholaFly PH05-04
8.13Edexcel 1PH0Recall and use the equation: power (watt, W) = work done (joule, J) ÷ time taken (second, s)Power as the rate of energy transferScholaFly PH05-04
8.14Edexcel 1PH0Recall that one watt is equal to one joule per second, J/sPower as the rate of energy transferScholaFly PH05-04
8.15Edexcel 1PH0Recall and use the equation: device the plied sup energy total device the transferre energy useful efficiency =EfficiencyScholaFly PH06-03
9.1Edexcel 1PH0Describe, with examples, how objects can interact a at a distance without contact, linking these to the gravitational, electrostatic and magnetic fields involved b by contact, including normal contact force and friction c producing pairs of forces which can be represented as vectorsContact and non-contact forcesScholaFly PH03-01
9.2Edexcel 1PH0Explain the difference between vector and scalar quantities using examplesScalars and vectorsScholaFly PH01-02
Distance and displacementScholaFly PH01-03
VelocityScholaFly PH01-05
9.3Edexcel 1PH0Use vector diagrams to illustrate resolution of forces, a net force, and equilibrium situations (scale drawings only)Resolving forces with a scale vector diagram (Higher)ScholaFly PH03-05
9.4Edexcel 1PH0Draw and use free body force diagramsResultant forcesScholaFly PH03-03
Free body diagrams (Higher)ScholaFly PH03-04
9.5Edexcel 1PH0Explain examples of the forces acting on an isolated solid object or a system where several forces lead to a resultant force on an object and the special case of balanced forces when the resultant force is zeroResultant forcesScholaFly PH03-03
Free body diagrams (Higher)ScholaFly PH03-04
9.6PEdexcel 1PH0Describe situations where forces can cause rotationMoments and the principle of moments (triple)ScholaFly PH03-08
Levers and gears (triple)ScholaFly PH03-09
9.7PEdexcel 1PH0Recall and use the equation: moment of a force (newton metre, N m) = force (newton, N) × distance normal to the direction of the force (metre, m)Moments and the principle of moments (triple)ScholaFly PH03-08
Levers and gears (triple)ScholaFly PH03-09
9.8PEdexcel 1PH0Recall and use the principle of moments in situations where rotational forces are in equilibrium: the sum of clockwise moments = the sum of anti-clockwise moments for rotational forces in equilibriumMoments and the principle of moments (triple)ScholaFly PH03-08
Levers and gears (triple)ScholaFly PH03-09
9.9PEdexcel 1PH0Explain how levers and gears transmit the rotational effects of forcesMoments and the principle of moments (triple)ScholaFly PH03-08
Levers and gears (triple)ScholaFly PH03-09
9.10Edexcel 1PH0Explain ways of reducing unwanted energy transfer through lubricationReducing unwanted energy transfersScholaFly PH06-02
10.1Edexcel 1PH0Describe the structure of the atom, limited to the position, mass and charge of protons, neutrons and electronsProtons, neutrons and electronsScholaFly PH19-02
10.2Edexcel 1PH0Draw and use electric circuit diagrams representing them with the conventions of positive and negative terminals, and the symbols that represent cells, including batteries, switches, voltmeters, ammeters, resistors, variable resistors, lamps, motors, diodes, thermistors, LDRs and LEDsCircuit diagrams and standard symbolsScholaFly PH10-01
10.3Edexcel 1PH0Describe the differences between series and parallel circuitsSeries circuitsScholaFly PH10-08
Parallel circuitsScholaFly PH10-09
10.4Edexcel 1PH0Recall that a voltmeter is connected in parallel with a component to measure the potential difference (voltage), in volt, across itVoltmeters and ammeters in a circuitScholaFly PH10-04
10.5Edexcel 1PH0Explain that potential difference (voltage) is the energy transferred per unit charge passed and hence that the volt is a joule per coulombPotential difference and E = QVScholaFly PH10-03
10.6Edexcel 1PH0Recall and use the equation: energy transferred (joule, J) = charge moved (coulomb, C) × potential difference (volt, V)Potential difference and E = QVScholaFly PH10-03
10.7Edexcel 1PH0Recall that an ammeter is connected in series with a component to measure the current, in amp, in the componentVoltmeters and ammeters in a circuitScholaFly PH10-04
10.8Edexcel 1PH0Explain that an electric current as the rate of flow of charge and the current in metals is a flow of electronsCharge, current and Q = ItScholaFly PH10-02
10.9Edexcel 1PH0Recall and use the equation: charge (coulomb, C) = current (ampere, A) × time (second, s)Charge, current and Q = ItScholaFly PH10-02
10.10Edexcel 1PH0Describe that when a closed circuit includes a source of potential difference there will be a current in the circuitCharge, current and Q = ItScholaFly PH10-02
10.11Edexcel 1PH0Recall that current is conserved at a junction in a circuitSeries circuitsScholaFly PH10-08
Parallel circuitsScholaFly PH10-09
10.12Edexcel 1PH0Explain how changing the resistance in a circuit changes the current and how this can be achieved using a variable resistorResistance and V = IRScholaFly PH10-05
10.13Edexcel 1PH0Recall and use the equation: potential difference (volt, V) = current (ampere, A) × resistance (ohm, Ω)Resistance and V = IRScholaFly PH10-05
10.14Edexcel 1PH0Explain why, if two resistors are in series, the net resistance is increased, whereas with two in parallel the net resistance is decreasedSeries circuitsScholaFly PH10-08
Parallel circuitsScholaFly PH10-09
10.15Edexcel 1PH0Calculate the currents, potential differences and resistances in series circuitsSeries circuitsScholaFly PH10-08
Parallel circuitsScholaFly PH10-09
10.16Edexcel 1PH0Explain the design and construction of series circuits for testing and measuringSeries circuitsScholaFly PH10-08
Parallel circuitsScholaFly PH10-09
10.17Edexcel 1PH0Core Practical: Construct electrical circuits to: a investigate the relationship between potential difference, current and resistance for a resistor and a filament lamp b test series and parallel circuits using resistors and filament lampsPractical: resistance of a wire and of componentsScholaFly PH24-06
Practical: I-V characteristicsScholaFly PH24-07
10.18Edexcel 1PH0Explain how current varies with potential difference for the following devices and how this relates to resistance a filament lamps b diodes c fixed resistorsI-V characteristics: ohmic conductor, filament lamp and diodeScholaFly PH10-06
Thermistors and light-dependent resistorsScholaFly PH10-07
10.19Edexcel 1PH0Describe how the resistance of a light-dependent resistor (LDR) varies with light intensityI-V characteristics: ohmic conductor, filament lamp and diodeScholaFly PH10-06
Thermistors and light-dependent resistorsScholaFly PH10-07
10.20Edexcel 1PH0Describe how the resistance of a thermistor varies with change of temperature (negative temperature coefficient thermistors only)I-V characteristics: ohmic conductor, filament lamp and diodeScholaFly PH10-06
Thermistors and light-dependent resistorsScholaFly PH10-07
10.21Edexcel 1PH0Explain how the design and use of circuits can be used to explore the variation of resistance in the following devices a filament lamps b diodes c thermistors d LDRsI-V characteristics: ohmic conductor, filament lamp and diodeScholaFly PH10-06
Thermistors and light-dependent resistorsScholaFly PH10-07
10.22Edexcel 1PH0Recall that, when there is an electric current in a resistor, there is an energy transfer which heats the resistorThe heating effect of a currentScholaFly PH11-04
10.23Edexcel 1PH0Explain that electrical energy is dissipated as thermal energy in the surroundings when an electrical current does work against electrical resistanceThe heating effect of a currentScholaFly PH11-04
10.24Edexcel 1PH0Explain the energy transfer (in 10.22 above) as the result of collisions between electrons and the ions in the latticeThe heating effect of a currentScholaFly PH11-04
10.25Edexcel 1PH0Explain ways of reducing unwanted energy transfer through low resistance wiresReducing unwanted transfer with low-resistance wires (Higher)ScholaFly PH11-05
10.26Edexcel 1PH0Describe the advantages and disadvantages of the heating effect of an electric currentThe heating effect of a currentScholaFly PH11-04
10.27Edexcel 1PH0Use the equation: energy transferred (joule, J) = current (ampere, A) × potential difference (volt, V) × time (second, s)Energy transferred by an appliance: E = Pt and E = IVtScholaFly PH11-02
10.28Edexcel 1PH0Describe power as the energy transferred per second and recall that it is measured in wattPower as the rate of energy transferScholaFly PH05-04
10.29Edexcel 1PH0Recall and use the equation: power (watt, W) = energy transferred (joule, J) ÷ time taken (second, s)Power as the rate of energy transferScholaFly PH05-04
10.30Edexcel 1PH0Explain how the power transfer in any circuit device is related to the potential difference across it and the current in itElectrical power: P = VI and P = I^2 RScholaFly PH11-01
10.31Edexcel 1PH0Recall and use the equations: electrical power (watt, W) = current (ampere, A) × potential difference (volt, V) electrical power (watt, W) = current squared (ampere2, A2) × resistance (ohm, Ω)Electrical power: P = VI and P = I^2 RScholaFly PH11-01
10.32Edexcel 1PH0Describe how, in different domestic devices, energy is transferred from batteries and the a.c. mains to the energy of motors and heating devicesDomestic appliances and power ratingsScholaFly PH11-03
10.33Edexcel 1PH0Explain the difference between direct and alternating voltageDirect and alternating potential difference and the mains supplyScholaFly PH11-06
10.34Edexcel 1PH0Describe direct current (d.c.) as movement of charge in one direction only and recall that cells and batteries supply direct current (d.c.)Direct and alternating potential difference and the mains supplyScholaFly PH11-06
10.35Edexcel 1PH0Describe that in alternating current (a.c.) the movement of charge changes directionDirect and alternating potential difference and the mains supplyScholaFly PH11-06
10.36Edexcel 1PH0Recall that in the UK the domestic supply is a.c., at a frequency of 50 Hz and a voltage of about 230 VDirect and alternating potential difference and the mains supplyScholaFly PH11-06
10.37Edexcel 1PH0Explain the difference in function between the live and the neutral mains input wiresMains wiring: live, neutral and earthScholaFly PH11-07
Electrical safety: fuses, circuit breakers and earthingScholaFly PH11-08
10.38Edexcel 1PH0Explain the function of an earth wire and of fuses or circuit breakers in ensuring safetyMains wiring: live, neutral and earthScholaFly PH11-07
Electrical safety: fuses, circuit breakers and earthingScholaFly PH11-08
10.39Edexcel 1PH0Explain why switches and fuses should be connected in the live wire of a domestic circuitMains wiring: live, neutral and earthScholaFly PH11-07
Electrical safety: fuses, circuit breakers and earthingScholaFly PH11-08
10.40Edexcel 1PH0Recall the potential differences between the live, neutral and earth mains wiresMains wiring: live, neutral and earthScholaFly PH11-07
Electrical safety: fuses, circuit breakers and earthingScholaFly PH11-08
10.41Edexcel 1PH0Explain the dangers of providing any connection between the live wire and earthMains wiring: live, neutral and earthScholaFly PH11-07
Electrical safety: fuses, circuit breakers and earthingScholaFly PH11-08
10.42Edexcel 1PH0Describe, with examples, the relationship between the power ratings for domestic electrical appliances and the changes in stored energy when they are in useDomestic appliances and power ratingsScholaFly PH11-03
11.1PEdexcel 1PH0Explain how an insulator can be charged by friction, through the transfer of electronsStatic charge: charging by friction, attraction and repulsionScholaFly PH12-01
11.2PEdexcel 1PH0Explain how the material gaining electrons becomes negatively charged and the material losing electrons is left with an equal positive chargeStatic charge: charging by friction, attraction and repulsionScholaFly PH12-01
11.3PEdexcel 1PH0Recall that like charges repel and unlike charges attractStatic charge: charging by friction, attraction and repulsionScholaFly PH12-01
11.4PEdexcel 1PH0Explain common electrostatic phenomena in terms of movement of electrons, including a shocks from everyday objects b lightning c attraction by induction such as a charged balloon attracted to a wall and a charged comb picking up small pieces of paperSparking, earthing, and the uses and dangers of staticScholaFly PH12-02
11.5PEdexcel 1PH0Explain how earthing removes excess charge by movement of electronsSparking, earthing, and the uses and dangers of staticScholaFly PH12-02
11.6PEdexcel 1PH0Explain some of the uses of electrostatic charges in everyday situations, including insecticide sprayersSparking, earthing, and the uses and dangers of staticScholaFly PH12-02
11.7PEdexcel 1PH0Describe some of the dangers of sparking in everyday situations, including fuelling cars, and explain the use of earthing to prevent dangerous build-up of chargeSparking, earthing, and the uses and dangers of staticScholaFly PH12-02
11.8PEdexcel 1PH0Define an electric field as the region where an electric charge experiences a forceElectric fields (triple)ScholaFly PH12-03
11.9PEdexcel 1PH0Describe the shape and direction of the electric field around a point charge and between parallel plates and relate the strength of the field to the concentration of linesElectric fields (triple)ScholaFly PH12-03
11.10PEdexcel 1PH0Explain how the concept of an electric field helps to explain the phenomena of static electricityElectric fields (triple)ScholaFly PH12-03
12.1Edexcel 1PH0Recall that unlike magnetic poles attract and like magnetic poles repelMagnetic poles, permanent and induced magnetsScholaFly PH13-01
12.2Edexcel 1PH0Describe the uses of permanent and temporary magnetic materials including cobalt, steel, iron and nickelMagnetic poles, permanent and induced magnetsScholaFly PH13-01
12.3Edexcel 1PH0Explain the difference between permanent and induced magnetsMagnetic poles, permanent and induced magnetsScholaFly PH13-01
12.4Edexcel 1PH0Describe the shape and direction of the magnetic field around bar magnets and for a uniform field, and relate the strength of the field to the concentration of linesMagnetic fields, plotting compasses and the Earth's fieldScholaFly PH13-02
12.5Edexcel 1PH0Describe the use of plotting compasses to show the shape and direction of the field of a magnet and the Earth’s magnetic fieldMagnetic fields, plotting compasses and the Earth's fieldScholaFly PH13-02
12.6Edexcel 1PH0Explain how the behaviour of a magnetic compass is related to evidence that the core of the Earth must be magneticMagnetic fields, plotting compasses and the Earth's fieldScholaFly PH13-02
12.7Edexcel 1PH0Describe how to show that a current can create a magnetic effect around a long straight conductor, describing the shape of the magnetic field produced and relating the direction of the magnetic field to the direction of the currentThe magnetic effect of a current, solenoids and electromagnetsScholaFly PH13-03
12.8Edexcel 1PH0Recall that the strength of the field depends on the size of the current and the distance from the long straight conductorThe magnetic effect of a current, solenoids and electromagnetsScholaFly PH13-03
12.9Edexcel 1PH0Explain how inside a solenoid (an example of an electromagnet) the fields from individual coils a add together to form a very strong almost uniform field along the centre of the solenoid b cancel to give a weaker field outside the solenoidThe magnetic effect of a current, solenoids and electromagnetsScholaFly PH13-03
12.10Edexcel 1PH0Recall that a current carrying conductor placed near a magnet experiences a force and that an equal and opposite force acts on the magnetThe motor effect and Fleming's left-hand rule (Higher)ScholaFly PH13-04
12.11Edexcel 1PH0Explain that magnetic forces are due to interactions between magnetic fieldsThe motor effect and Fleming's left-hand rule (Higher)ScholaFly PH13-04
12.12Edexcel 1PH0Recall and use Fleming’s left-hand rule to represent the relative directions of the force, the current and the magnetic field for cases where they are mutually perpendicularThe motor effect and Fleming's left-hand rule (Higher)ScholaFly PH13-04
12.13Edexcel 1PH0Use the equation: force on a conductor at right angles to a magnetic field carrying a current (newton, N) = magnetic flux density (tesla, T or newton per ampere metre, N/A m) × current (ampere, A) × length (metre, m)F = BIl (Higher)ScholaFly PH13-05
12.14PEdexcel 1PH0Explain how the force on a conductor in a magnetic field is used to cause rotation in electric motorsElectric motors (Higher)ScholaFly PH13-06
13.1PEdexcel 1PH0Explain how to produce an electric current by the relative movement of a magnet and a conductor a on a small scale in the laboratory b in the large-scale generation of electrical energyElectromagnetic induction and the generator effect (Higher)ScholaFly PH14-01
13.2Edexcel 1PH0Recall the factors that affect the size and direction of an induced potential difference, and describe how the magnetic field produced opposes the original changeElectromagnetic induction and the generator effect (Higher)ScholaFly PH14-01
13.3PEdexcel 1PH0Explain how electromagnetic induction is used in alternators to generate current which alternates in direction (a.c.) and in dynamos to generate direct current (d.c.)Alternators and dynamos (triple, Higher)ScholaFly PH14-04
13.4PEdexcel 1PH0Explain the action of the microphone in converting the pressure variations in sound waves into variations in current in electrical circuits, and the reverse effect as used in loudspeakers and headphonesMicrophones and loudspeakers (triple, Higher)ScholaFly PH14-05
13.5Edexcel 1PH0Explain how an alternating current in one circuit can induce a current in another circuit in a transformerTransformers and the turns-ratio equation (Higher)ScholaFly PH14-02
13.6Edexcel 1PH0Recall that a transformer can change the size of an alternating voltageTransformers and the turns-ratio equation (Higher)ScholaFly PH14-02
13.7PEdexcel 1PH0Use the turns ratio equation for transformers to calculate either the missing voltage or the missing number of turns: coil ondary sec turns number coil primary turns number coil ondary sec across difference potential coil primary across difference potentialTransformers and the turns-ratio equation (Higher)ScholaFly PH14-02
13.8Edexcel 1PH0Explain why, in the national grid, electrical energy is transferred at high voltages from power stations, and then transferred at lower voltages in each locality for domestic uses as it improves the efficiency by reducing heat loss in transmission linesThe National GridScholaFly PH11-09
13.9Edexcel 1PH0Explain where and why step-up and step-down transformers are used in the transmission of electricity in the national gridThe National GridScholaFly PH11-09
13.10Edexcel 1PH0Use the power equation (for transformers with100% efficiency): potential difference across primary coil (volt, V) × current in primary coil (ampere, A) = potential difference across secondary coil (volt, V) × current in secondary coil (ampere,The transformer power equation and high-voltage transmissionScholaFly PH14-03
13.11PEdexcel 1PH0Explain the advantages of power transmission in high- voltage cables, using the equations in 10.29, 10.31,The transformer power equation and high-voltage transmissionScholaFly PH14-03
14.1Edexcel 1PH0Use a simple kinetic theory model to explain the different states of matter (solids, liquids and gases) in terms of the movement and arrangement of particlesThe particle model and the states of matterScholaFly PH08-01
14.2Edexcel 1PH0Recall and use the equation: density (kilogram per cubic metre, kg/m3) = mass (kilogram, kg) ÷ volume (cubic metre, m3)DensityScholaFly PH08-02
14.3Edexcel 1PH0Core Practical: Investigate the densities of solid and liquidsPractical: density of solids and liquidsScholaFly PH24-02
14.4Edexcel 1PH0Explain the differences in density between the different states of matter in terms of the arrangements of the atoms or moleculesThe particle model and the states of matterScholaFly PH08-01
14.5Edexcel 1PH0Describe that when substances melt, freeze, evaporate, boil, condense or sublimate mass is conserved and that these physical changes differ from some chemical changes because the material recovers its original properties if the change is reversedChanges of state and conservation of massScholaFly PH08-03
14.6Edexcel 1PH0Explain how heating a system will change the energy stored within the system and raise its temperature or produce changes of stateInternal energy and what heating does to a systemScholaFly PH08-04
Specific heat capacityScholaFly PH08-05
Specific latent heat of fusion and of vaporisationScholaFly PH08-06
14.7Edexcel 1PH0Define the terms specific heat capacity and specific latent heat and explain the differences between themInternal energy and what heating does to a systemScholaFly PH08-04
Specific heat capacityScholaFly PH08-05
Specific latent heat of fusion and of vaporisationScholaFly PH08-06
14.8Edexcel 1PH0Use the equation: change in thermal energy (joule, J) = mass (kilogram, kg) × specific heat capacity (joule per kilogram degree Celsius, J/kg °C) × change in temperature (degree Celsius, °C)Specific heat capacityScholaFly PH08-05
14.9Edexcel 1PH0Use the equation: thermal energy for a change of state (joule , J) = mass (kilogram, kg) × specific latent heat (joule per kilogram, J/kg)Specific latent heat of fusion and of vaporisationScholaFly PH08-06
14.10Edexcel 1PH0Explain ways of reducing unwanted energy transfer through thermal insulationReducing unwanted energy transfersScholaFly PH06-02
14.11Edexcel 1PH0Core Practical: Investigate the properties of water by determining the specific heat capacity of water and obtaining a temperature-time graph for melting icePractical: specific heat capacityScholaFly PH24-01
14.12Edexcel 1PH0Explain the pressure of a gas in terms of the motion of its particlesGas particles, temperature and pressureScholaFly PH08-07
14.13Edexcel 1PH0Explain the effect of changing the temperature of a gas on the velocity of its particles and hence on the pressure produced by a fixed mass of gas at constant volume (qualitative only)Gas particles, temperature and pressureScholaFly PH08-07
14.14Edexcel 1PH0Describe the term absolute zero, −273 °C, in terms of the lack of movement of particlesAbsolute zero and the kelvin scaleScholaFly PH08-08
14.15Edexcel 1PH0Convert between the kelvin and Celsius scalesAbsolute zero and the kelvin scaleScholaFly PH08-08
14.16PEdexcel 1PH0Explain that gases can be compressed or expanded by pressure changesGases under pressure: pV = constant (triple)ScholaFly PH08-09
14.17PEdexcel 1PH0Explain that the pressure of a gas produces a net force at right angles to any surfaceGases under pressure: pV = constant (triple)ScholaFly PH08-09
14.18PEdexcel 1PH0Explain the effect of changing the volume of a gas on the rate at which its particles collide with the walls of its container and hence on the pressure produced by a fixed mass of gas at constant temperatureGases under pressure: pV = constant (triple)ScholaFly PH08-09
14.19PEdexcel 1PH0Use the equation: to calculate pressure or volume for gases of fixed mass at constant temperatureGases under pressure: pV = constant (triple)ScholaFly PH08-09
14.20PEdexcel 1PH0Explain why doing work on a gas can increase its temperature, including a bicycle pumpDoing work on a gas raises its temperature (triple, Higher)ScholaFly PH08-10
15.1Edexcel 1PH0Explain, using springs and other elastic objects, that stretching, bending or compressing an object requires more than one forceElastic and inelastic deformationScholaFly PH03-06
15.2Edexcel 1PH0Describe the difference between elastic and inelastic distortionElastic and inelastic deformationScholaFly PH03-06
15.3Edexcel 1PH0Recall and use the equation for linear elastic distortion including calculating the spring constant: force exerted on a spring (newton, N) = spring constant (newton per metre, N/m) × extension (metre, m)Hooke's law and the spring constantScholaFly PH03-07
15.4Edexcel 1PH0Use the equation to calculate the work done in stretching a spring: energy transferred in stretching (joules, J) = 0.5 × spring constant (newton per metre, N/m) × (extension (metre, m))2Elastic potential energyScholaFly PH05-07
15.5Edexcel 1PH0Describe the difference between linear and non-linear relationships between force and extensionHooke's law and the spring constantScholaFly PH03-07
15.6Edexcel 1PH0Core Practical: Investigate the extension and work done when applying forces to a springPractical: force and extension of a springScholaFly PH24-04
15.7PEdexcel 1PH0Explain why atmospheric pressure varies with height above the Earth’s surface with reference to a simple model of the Earth’s atmosphereAtmospheric pressure (triple)ScholaFly PH09-02
15.8PEdexcel 1PH0Describe the pressure in a fluid as being due to the fluid and atmospheric pressurePressure in a fluid: p = F/A (triple)ScholaFly PH09-01
15.9PEdexcel 1PH0Recall that the pressure in fluids causes a force normal to any surfacePressure in a fluid: p = F/A (triple)ScholaFly PH09-01
15.10PEdexcel 1PH0Explain how pressure is related to force and area, using appropriate examplesPressure in a fluid: p = F/A (triple)ScholaFly PH09-01
15.11PEdexcel 1PH0Recall and use the equation: pressure (pascal, Pa) = force normal to surface (newton, N) ÷ area of surface (square metre, m2)Pressure in a fluid: p = F/A (triple)ScholaFly PH09-01
15.12PEdexcel 1PH0Describe how pressure in fluids increases with depth and densityPressure, depth and density: p = h rho g (triple)ScholaFly PH09-03
15.13PEdexcel 1PH0Explain why the pressure in liquids varies with density and depthPressure, depth and density: p = h rho g (triple)ScholaFly PH09-03
15.14PEdexcel 1PH0Use the equation to calculate the magnitude of the pressure in liquids and calculate the differences in pressure at different depths in a liquid: pressure due to a column of liquid (pascal, Pa) = height of column (metre, m) × density of liquid (kilogram per cubic metre, kg/m3) × gravitational field strength (newton per kilogram, N/kg)Pressure, depth and density: p = h rho g (triple)ScholaFly PH09-03
15.15PEdexcel 1PH0Explain why an object in a fluid is subject to an upwards force (upthrust) and relate this to examples including objects that are fully immersed in a fluid (liquid or gas) or partially immersed in a liquidUpthrust, floating and sinking (triple, Higher)ScholaFly PH09-04
15.16PEdexcel 1PH0Recall that the upthrust is equal to the weight of fluid displacedUpthrust, floating and sinking (triple, Higher)ScholaFly PH09-04
15.17PEdexcel 1PH0Explain how the factors (upthrust, weight, density of fluid) influence whether an object will float or sinkUpthrust, floating and sinking (triple, Higher)ScholaFly PH09-04