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Mechanics & motion

Scalars and vectors

  • A scalar has magnitude only (speed, distance, energy, mass).
  • A vector has magnitude AND direction (velocity, displacement, force, acceleration).
  • Resolve vectors into perpendicular components using cos and sin of the angle from the reference axis.
  • Add vectors tip-to-tail or use Pythagoras and trigonometry for right-angle problems.

The suvat equations

  • v = u + at
  • s = ut + 0.5at^2
  • v^2 = u^2 + 2as
  • s = 0.5(u + v)t
  • These only work for CONSTANT acceleration in a straight line. Never use them if acceleration changes.
  • Take g = 9.81 m/s^2 on Earth unless told otherwise; it acts downwards.
  • Always define a positive direction first and keep signs consistent (e.g. up positive, so g = -9.81 m/s^2).

Projectile motion

  • Split motion into horizontal (constant velocity, a = 0) and vertical (constant acceleration g) components — they are independent.
  • Time of flight is set by the vertical motion only.
  • Horizontal velocity never changes if air resistance is ignored.
  • Common mistake: using the resultant speed in a suvat equation instead of splitting into components first.

Graphs of motion

  • Displacement-time graph: gradient = velocity. Curve means acceleration.
  • Velocity-time graph: gradient = acceleration; area under graph = displacement.
  • Acceleration-time graph: area under graph = change in velocity.
  • A negative gradient or negative area means motion/change in the opposite direction, not zero.

Newton's laws and forces

  • First law: an object stays at rest or constant velocity unless a resultant (net) force acts on it.
  • Second law: F = ma, where F is the resultant force in newtons, m in kg, a in m/s^2.
  • Third law: forces come in equal, opposite, same-type action-reaction pairs acting on DIFFERENT objects — never on the same object.
  • Weight W = mg, always acts vertically downwards through the centre of mass.

Momentum and impulse

  • Momentum p = mv, measured in kg m/s, is a vector.
  • Conservation of momentum: total momentum before = total momentum after, in a closed system with no external forces.
  • Impulse = change in momentum = Ft (force x time), measured in Ns, and equals the area under a force-time graph.
  • Elastic collisions conserve both momentum and kinetic energy; inelastic collisions conserve momentum only.

Common exam mistakes

  • Forgetting to resolve forces on an inclined plane using the correct sin/cos for parallel and perpendicular components.
  • Mixing up mass (kg, constant) and weight (N, depends on g).
  • Forgetting units or not converting cm/g into SI units (m/kg) before calculating.
  • Not showing that resultant force is zero before stating an object is in equilibrium.
  • g = 9.81 m/s^2 downwards on Earth's surface unless stated otherwise
  • The suvat equations only apply when acceleration is constant
  • s = ut + 0.5at^2 gives displacement from initial velocity, acceleration and time
  • v^2 = u^2 + 2as lets you find final velocity without knowing time
  • In projectile motion, horizontal and vertical components of motion are independent
  • Gradient of a displacement-time graph equals velocity; gradient of velocity-time equals acceleration
  • Area under a velocity-time graph equals displacement
  • Newton's second law: F = ma, with F in newtons, m in kg, a in m/s^2
  • Newton's third law pairs act on two different objects, are equal in size and opposite in direction
  • Momentum p = mv is conserved in any closed system with no external resultant force
  • Impulse equals change in momentum (Ft = mv - mu) and equals the area under a force-time graph
  • Elastic collisions conserve kinetic energy as well as momentum; inelastic collisions only conserve momentum
State the four suvat equations.
v = u + at; s = ut + 0.5at^2; v^2 = u^2 + 2as; s = 0.5(u+v)t
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What condition must hold for the suvat equations to be valid?
Acceleration must be constant and motion must be in a straight line
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What is the value and direction of g near Earth's surface?
9.81 m/s^2, directed vertically downwards
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In projectile motion, what happens to the horizontal velocity if air resistance is ignored?
It stays constant throughout the flight, since there is no horizontal force acting
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What does the gradient of a velocity-time graph represent?
Acceleration
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What does the area under a velocity-time graph represent?
Displacement (distance travelled in a given direction)
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State Newton's first law of motion.
An object remains at rest or moving at constant velocity unless a resultant force acts on it
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State Newton's second law as an equation, with units.
F = ma, where F is resultant force in newtons, m is mass in kg, a is acceleration in m/s^2
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State Newton's third law and a key rule about the force pairs.
Every action has an equal and opposite reaction; the two forces act on different objects, never the same one
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Define momentum and give its units.
Momentum p = mv (mass x velocity), measured in kg m/s; it is a vector
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State the principle of conservation of momentum.
In a closed system with no external resultant force, total momentum before an event equals total momentum after
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Define impulse and how it relates to a force-time graph.
Impulse = Ft = change in momentum (mv - mu); it equals the area under a force-time graph
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What distinguishes an elastic collision from an inelastic one?
Elastic collisions conserve both momentum and kinetic energy; inelastic collisions conserve only momentum
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How do you find the resultant of two perpendicular vectors?
Use Pythagoras for magnitude (root of sum of squares) and tan(angle) = opposite/adjacent for direction
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What is the weight of an object and how is it calculated?
Weight W = mg; it acts vertically downwards through the object's centre of mass, measured in newtons
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Materials & energy

Density and Hooke's Law

Density is mass per unit volume: rho = m / V, measured in kg per cubic metre.

Hooke's Law states that force is proportional to extension: F = k x, as long as the limit of proportionality is not exceeded.

The spring constant k is measured in newtons per metre (N/m).

Beyond the elastic limit the material no longer returns to its original shape when unloaded.

Stress, Strain and the Young Modulus

Stress = force / cross-sectional area, units pascals (Pa) or N/m^2.

Strain = extension / original length, and strain has no units (it is a ratio).

The Young modulus E = stress / strain, also measured in pascals.

On a stress-strain graph, the gradient of the straight-line (elastic) region gives the Young modulus.

The elastic limit is the point beyond which the material shows plastic deformation and will not return to its original length.

The UTS (ultimate tensile stress) is the maximum stress a material can withstand before breaking.

Brittle materials (like glass) snap suddenly with little plastic deformation; ductile materials (like copper) stretch a lot before breaking.

Energy Stored in a Stretched Material

Elastic potential energy = area under a force-extension graph.

For a material obeying Hooke's Law: E_el = 0.5 F x = 0.5 k x^2.

If a material is stretched beyond its elastic limit, the loading and unloading curves differ (hysteresis loop) — the area between the curves is the energy dissipated as heat.

Common mistakes

  • Mixing up stress (force per area) with pressure — they have the same units but different physical meaning.
  • Forgetting strain is dimensionless — never give strain a unit.
  • Using the wrong length (extension vs total length) in strain calculations.
  • Assuming F = kx applies everywhere on a stress-strain graph — it only holds up to the limit of proportionality.

Thermal Energy

Specific heat capacity c: energy to raise 1 kg of a substance by 1 K. Equation: Q = m c (delta)T, units J/(kg K).

Specific latent heat L: energy to change the state of 1 kg of a substance with no temperature change. Equation: Q = m L, units J/kg.

Specific latent heat of fusion applies to melting/freezing; specific latent heat of vaporisation applies to boiling/condensing — vaporisation is always larger than fusion for the same substance because more bonds must be broken.

Internal energy is the sum of the random distribution of kinetic and potential energies of the particles in a system; it increases when temperature rises OR when a substance changes state (even though temperature stays constant during a phase change).

Common mistakes

  • Forgetting temperature must be in kelvin for gas law work, though delta T is the same size in K and degrees C, so Q = mc(delta)T calculations can use either.
  • Believing temperature rises during melting or boiling — it does not; all the energy goes into breaking intermolecular bonds (increasing potential energy, not kinetic energy).
  • Confusing specific heat capacity with specific latent heat — one involves a temperature change, the other does not.
  • Hooke's Law: F = k x, valid only up to the limit of proportionality, k in N/m
  • The Young modulus E = stress / strain = (F/A) / (x/L), measured in pascals (Pa)
  • Strain is dimensionless — it is a ratio of extension to original length, never give it units
  • Elastic potential energy stored (Hooke's Law region) = 0.5 F x = 0.5 k x^2, joules
  • Elastic potential energy for any force-extension graph = area under the graph
  • UTS (ultimate tensile stress) is the maximum stress a material withstands before it breaks
  • Ductile materials show large plastic deformation before breaking; brittle materials snap with little warning
  • Specific heat capacity: Q = m c (delta)T, units J/(kg K)
  • Specific latent heat: Q = m L, units J/kg, applies only during a change of state at constant temperature
  • Specific latent heat of vaporisation is always greater than specific latent heat of fusion for the same substance
  • Temperature does NOT change during melting or boiling — the energy input increases potential, not kinetic, energy of particles
  • Density rho = m / V, measured in kg/m^3
State Hooke's Law and give the equation.
Force is proportional to extension up to the limit of proportionality: F = k x, where k is the spring constant in N/m.
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Define stress and give its units.
Stress = force / cross-sectional area, measured in pascals (Pa) or N/m^2.
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Define strain and state its units.
Strain = extension / original length. It is a ratio, so it has no units.
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What is the Young modulus and how do you find it from a graph?
E = stress / strain (Pa); it is the gradient of the straight-line (elastic) region of a stress-strain graph.
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How do you calculate elastic potential energy stored in a stretched spring obeying Hooke's Law?
E_el = 0.5 F x = 0.5 k x^2, in joules.
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How is elastic potential energy found for a graph that is NOT a straight line?
It equals the area under the force-extension graph, found by counting squares or integration.
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What does the elastic limit mean for a material?
Beyond it the material undergoes plastic deformation and will not return to its original length when unloaded.
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Define ultimate tensile stress (UTS).
The maximum stress a material can withstand before it breaks.
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Contrast brittle and ductile material behaviour under stress.
Brittle materials (e.g. glass) snap suddenly with little plastic deformation; ductile materials (e.g. copper) stretch and deform plastically a lot before breaking.
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State the equation for specific heat capacity and its units.
Q = m c (delta)T, where c is in J/(kg K).
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State the equation for specific latent heat and its units.
Q = m L, where L is in J/kg, used only during a change of state.
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Why is specific latent heat of vaporisation greater than specific latent heat of fusion?
Vaporisation requires completely separating particles (breaking all intermolecular bonds), which needs far more energy than the partial bond-breaking of melting.
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Does temperature change while a substance melts or boils? Explain.
No — all the energy input goes into increasing the potential energy of the particles (breaking bonds), not their kinetic energy, so temperature stays constant during a phase change.
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Define density and give its equation and units.
Density is mass per unit volume: rho = m / V, measured in kg/m^3.
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What does the area between the loading and unloading curves on a stress-strain hysteresis loop represent?
The energy dissipated as heat when a material is stretched beyond its elastic limit and then unloaded.
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Electricity & circuits

Current, Charge and Potential Difference

Current I is the rate of flow of charge: I = Q/t, measured in amperes (A). Charge Q is measured in coulombs (C), where 1 C = 1 A flowing for 1 s.

Potential difference (p.d.) is the energy transferred per unit charge: V = W/Q, measured in volts (V), where 1 V = 1 joule per coulomb.

Electromotive force (e.m.f.) is the energy given to each coulomb of charge by a source (like a cell), also in volts. E.m.f. and p.d. are NOT the same thing - e.m.f. includes energy 'lost' inside the source due to internal resistance.

Resistance and Ohm's Law

Resistance R = V/I, measured in ohms (Ω). Ohm's law states current through a conductor is directly proportional to p.d. across it, provided temperature stays constant - this only applies to ohmic conductors (like a resistor at constant temperature).

For a filament lamp, resistance increases as it heats up (curve flattens on an I-V graph). For a diode, current only flows one way past the threshold voltage (about 0.6 V for silicon).

Resistivity: R = ρL/A, where ρ (rho) is resistivity in Ω m, L is length, A is cross-sectional area. Resistivity depends on material and temperature, not on the shape of the sample - do not confuse ρ with R.

Power and Energy

Electrical power P = VI = I²R = V²/R. Energy transferred W = VIt = Pt, measured in joules.

Circuit Rules

Kirchhoff's first law: current into a junction equals current out (conservation of charge). Kirchhoff's second law: the sum of e.m.f.s around a closed loop equals the sum of p.d.s (conservation of energy).

Series circuits: current is the same everywhere; total resistance R = R1 + R2 + ...; p.d.s add up to the source e.m.f.

Parallel circuits: p.d. is the same across each branch; total resistance found from 1/R = 1/R1 + 1/R2 + ...; total current is the sum of branch currents.

Internal Resistance and Terminal p.d.

Every real cell has internal resistance r. E.m.f. ε = I(R + r), so terminal p.d. V = ε - Ir. On short circuit (R = 0), current is at its maximum, limited only by r.

Potential Dividers and Sensors

A potential divider splits voltage in proportion to resistance: Vout = V x (R2/(R1+R2)). LDRs (resistance falls as light increases) and thermistors (resistance falls as temperature increases) are common sensor components used in potential dividers.

Common Mistakes

  • Mixing up e.m.f. and terminal p.d. - they are only equal when no current flows.
  • Forgetting resistivity is a material property, not dependent on the wire's dimensions.
  • Using series formulas in a parallel circuit or vice versa.
  • Forgetting that ammeters should have (near) zero resistance and voltmeters should have (near) infinite resistance for accurate readings.
  • Current I = Q/t, where charge Q is measured in coulombs (1 C = 1 A for 1 s)
  • Potential difference V = W/Q, measured in volts (1 V = 1 joule per coulomb)
  • Resistance R = V/I, measured in ohms; Ohm's law only holds at constant temperature
  • Resistivity formula: R = ρL/A, with ρ in ohm metres (Ω m)
  • Electrical power: P = VI = I²R = V²/R
  • In series circuits, current is constant and resistances add: R = R1 + R2 + ...
  • In parallel circuits, p.d. is constant and 1/R = 1/R1 + 1/R2 + ...
  • E.m.f. equation with internal resistance: ε = I(R + r)
  • Terminal p.d. V = ε - Ir, so V equals ε only when current I is zero
  • Potential divider output: Vout = V x (R2/(R1+R2))
  • LDR resistance decreases as light intensity increases; thermistor resistance decreases as temperature increases
  • Kirchhoff's first law conserves charge at a junction; Kirchhoff's second law conserves energy around a loop
What is the equation linking current, charge and time?
I = Q/t
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Define potential difference in terms of energy.
V = W/Q, the energy transferred per unit charge, measured in volts
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What is the difference between e.m.f. and terminal p.d.?
E.m.f. is the total energy per coulomb supplied by the source; terminal p.d. is less than e.m.f. whenever current flows, due to energy lost across internal resistance
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State Ohm's law.
Current is directly proportional to p.d. across a conductor, provided temperature is constant
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Give the resistivity equation and units of resistivity.
R = ρL/A; resistivity ρ is measured in ohm metres (Ω m)
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How does resistance change for a filament lamp as current increases?
Resistance increases because the filament heats up, so the I-V graph curves and flattens
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What are the three equations for electrical power?
P = VI, P = I²R, P = V²/R
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How do you find total resistance for resistors in series?
Add them directly: R = R1 + R2 + ...
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How do you find total resistance for resistors in parallel?
1/R = 1/R1 + 1/R2 + ...
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State Kirchhoff's first law.
The total current entering a junction equals the total current leaving it (conservation of charge)
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State Kirchhoff's second law.
The sum of e.m.f.s around any closed loop equals the sum of p.d.s around that loop (conservation of energy)
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Give the equation relating e.m.f., current, load resistance and internal resistance.
ε = I(R + r)
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What happens to current when a cell is short-circuited?
Current reaches its maximum possible value, limited only by the internal resistance r
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What is the potential divider output equation?
Vout = V x (R2/(R1+R2))
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How does an LDR's resistance behave with light, and a thermistor's with temperature?
LDR resistance falls as light intensity rises; thermistor resistance falls as temperature rises
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Waves & optics

Wave basics

A wave transfers energy without transferring matter. Transverse waves (light, water, all EM waves) oscillate perpendicular to travel direction; longitudinal waves (sound) oscillate parallel to it.

  • Wave equation: v = f x lambda (speed = frequency x wavelength)
  • Period T = 1/f
  • Displacement-time graphs give period and amplitude; displacement-distance graphs give wavelength

Phase and superposition

Path difference in whole wavelengths (nlambda) gives constructive interference (in phase); path difference of (n + 1/2)lambda gives destructive interference (antiphase). Superposition is the addition of displacements when two waves meet.

Standing waves

Formed by two coherent waves of the same frequency travelling in opposite directions, usually a wave and its reflection. Nodes = zero amplitude, always; antinodes = maximum amplitude. Distance between adjacent nodes = lambda/2. Unlike progressive waves, no energy is transferred along a standing wave and all points between nodes are in phase.

Refractive index and Snell's law

n = c / v (c = speed of light in vacuum, 3.00 x 10^8 m/s). Snell's law: n1 sin(theta1) = n2 sin(theta2). Critical angle: sin(thetaC) = n2/n1 (going from dense to less dense). Total internal reflection happens only when going from a denser to a less dense medium AND the angle of incidence exceeds the critical angle — both conditions are needed, a common mistake is forgetting the direction requirement.

Diffraction grating

nlambda = d sin(theta), where d = 1/(lines per metre). More lines per mm gives wider-spaced maxima. Common error: forgetting to convert 'lines per mm' into d in metres before substituting.

Young's double-slit

fringe spacing w = lambda D / s (D = slit-to-screen distance, s = slit separation). Requires coherent, monochromatic light. This confirms light's wave nature via interference.

Polarisation

Only transverse waves can be polarised — this is definitive proof light is transverse, since sound (longitudinal) cannot be polarised. Malus's law: I = I0 cos^2(theta).

Stationary waves on strings and in pipes

String fixed both ends: fundamental has a node at each end, one antinode in the middle, length L = lambda/2. Closed pipe (one end closed): only odd harmonics, L = lambda/4 for fundamental. Open pipe: L = lambda/2 for fundamental, same as a string.

Common mistakes

  • Mixing up node and antinode definitions
  • Using degrees vs radians inconsistently in phase problems
  • Forgetting path difference must be measured in wavelengths, not metres, when checking constructive/destructive conditions
  • Wave speed equation: v = f x lambda, always true for any wave
  • Refractive index n = c / v, with c = 3.00 x 10^8 m/s in a vacuum
  • Snell's law: n1 sin(theta1) = n2 sin(theta2) at a boundary between two media
  • Total internal reflection needs light going from denser to less dense medium AND angle of incidence greater than the critical angle
  • Critical angle formula: sin(thetaC) = n2 / n1
  • Diffraction grating equation: nlambda = d sin(theta), where d is the slit spacing in metres
  • Young's double-slit fringe spacing: w = lambda D / s
  • Distance between adjacent nodes on a stationary wave is always lambda/2
  • Only transverse waves can be polarised — proof that light is a transverse wave
  • Malus's law for polarised light intensity: I = I0 cos^2(theta)
  • Closed pipe (one closed end) only produces odd harmonics; fundamental length is lambda/4
  • Standing waves store energy but do not transfer it along the medium, unlike progressive waves
State the wave equation linking speed, frequency and wavelength.
v = f x lambda
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What is the refractive index formula in terms of speed of light?
n = c / v, where c is the speed of light in a vacuum (3.00 x 10^8 m/s)
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State Snell's law.
n1 sin(theta1) = n2 sin(theta2)
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What two conditions must both be met for total internal reflection to occur?
Light must travel from a denser to a less dense medium, and the angle of incidence must exceed the critical angle
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Give the formula for the critical angle.
sin(thetaC) = n2 / n1
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State the diffraction grating equation.
nlambda = d sin(theta), where d is the distance between adjacent slits in metres
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State the fringe spacing formula for Young's double-slit experiment.
w = lambda D / s
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What is the distance between two adjacent nodes in a stationary wave?
lambda/2
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Why does polarisation prove light is a transverse wave?
Only transverse waves can be polarised; longitudinal waves like sound cannot, so the fact light can be polarised shows it must be transverse
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State Malus's law.
I = I0 cos^2(theta), where theta is the angle between the polariser and the light's plane of polarisation
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For a pipe closed at one end, which harmonics are present and what is the fundamental length in terms of wavelength?
Only odd harmonics; fundamental length L = lambda/4
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For a string fixed at both ends, what is the length of the pipe/string at the fundamental frequency in terms of wavelength?
L = lambda/2, with a node at each end and one antinode in the middle
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What condition on path difference gives constructive interference?
Path difference equals a whole number of wavelengths, nlambda
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What condition on path difference gives destructive interference?
Path difference equals (n + 1/2) wavelengths
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Does a standing wave transfer energy along its length?
No — unlike a progressive wave, a standing wave stores energy but does not transfer it along the medium
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Fields (gravitational, electric, magnetic)

Gravitational fields

A gravitational field is the region around a mass where another mass feels a force. Field strength g is force per unit mass, measured in N/kg.

  • Newton's law: F = Gm1m2/r2, where G = 6.67 x 10^-11 N m2 kg^-2.
  • Field strength around a point mass: g = GM/r2. This obeys an inverse square law, so doubling r cuts g to a quarter.
  • Gravitational potential V = -GM/r. It is always negative, zero at infinity, and represents work done per unit mass to bring a small mass from infinity to that point.
  • Escape velocity comes from equating kinetic energy to the potential well: v = sqrt(2GM/r).
  • For orbits, gravity provides centripetal force: GMm/r2 = mv2/r, giving orbital speed and period. Kepler's third law follows: T2 is proportional to r3.
  • Geostationary orbits have a period of exactly 24 hours and sit above the equator at about 35800 km altitude.

Electric fields

An electric field is the region around a charge where another charge feels a force. Field strength E is force per unit positive charge, in N/C or V/m.

  • Coulomb's law: F = Qq/(4 pi epsilon0 r2), where epsilon0 = 8.85 x 10^-12 F/m.
  • Field strength: E = Q/(4 pi epsilon0 r2), again inverse square.
  • Electric potential V = Q/(4 pi epsilon0 r). Unlike gravity, V can be positive or negative depending on charge sign.
  • Uniform fields, as between parallel plates, have E = V/d, constant strength, and straight parallel field lines.
  • Work done moving charge q through potential difference V is W = qV.
  • Common mistake: mixing up field strength (a vector, inverse square) with potential (a scalar, inverse to the power 1).

Magnetic fields

Magnetic fields exert forces only on moving charges or current-carrying conductors, never on stationary charges.

  • Force on a current-carrying wire: F = BIL sin theta, where theta is the angle between the wire and B. Maximum force when the wire is perpendicular to B.
  • Force on a moving charge: F = BQv sin theta. Direction found using Fleming's left-hand rule (current, or conventional positive charge motion, and field give force).
  • Magnetic flux density B is measured in tesla (T).
  • Charged particles moving perpendicular to B follow circular paths since the force is always perpendicular to velocity, providing centripetal force: BQv = mv2/r.
  • Common mistake: forgetting that a charge moving parallel to B feels zero force, since sin(0) = 0.

Comparing the three fields

All three follow similar mathematical patterns but differ in sign, source, and what feels the force. Always check whether a question wants field strength (vector) or potential/potential energy (scalar), and whether the field is radial (point source) or uniform (parallel plates, inside a solenoid).

  • Newton's law of gravitation is F = Gm1m2/r2 with G = 6.67 x 10^-11 N m2 kg^-2.
  • Gravitational field strength g = GM/r2 follows an inverse square law and is always attractive.
  • Gravitational potential V = -GM/r is always negative and zero only at infinity.
  • Escape velocity is v = sqrt(2GM/r), independent of the escaping object's mass.
  • Kepler's third law states T2 is proportional to r3 for orbiting bodies.
  • A geostationary satellite orbits in exactly 24 hours above the equator at about 35800 km altitude.
  • Coulomb's law is F = Qq/(4 pi epsilon0 r2) with epsilon0 = 8.85 x 10^-12 F/m.
  • Electric potential V = Q/(4 pi epsilon0 r) can be positive or negative depending on charge sign.
  • In a uniform field between parallel plates, E = V/d and field lines are straight and equally spaced.
  • Force on a current-carrying wire in a magnetic field is F = BIL sin theta, maximum when the wire is perpendicular to B.
  • Force on a moving charge in a magnetic field is F = BQv sin theta, found using Fleming's left-hand rule.
  • A charge moving parallel to a magnetic field feels zero force since sin(0) = 0.
  • Charged particles moving perpendicular to a uniform B field travel in circles, since BQv = mv2/r.
State Newton's law of gravitation.
F = Gm1m2/r2, with G = 6.67 x 10^-11 N m2 kg^-2.
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What is gravitational field strength and its formula near a point mass?
Force per unit mass, g = GM/r2, an inverse square law, always attractive.
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Define gravitational potential and give its sign.
Work done per unit mass bringing a small mass from infinity to a point; V = -GM/r, always negative, zero at infinity.
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How do you find escape velocity?
Set kinetic energy equal to the gravitational potential well: v = sqrt(2GM/r).
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State Kepler's third law relationship.
T2 is proportional to r3 for an orbiting body.
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What defines a geostationary orbit?
Period of exactly 24 hours, above the equator, at about 35800 km altitude.
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State Coulomb's law.
F = Qq/(4 pi epsilon0 r2), with epsilon0 = 8.85 x 10^-12 F/m.
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What is the formula for electric field strength around a point charge?
E = Q/(4 pi epsilon0 r2), an inverse square law; can be attractive or repulsive.
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What is electric potential and how does its sign behave?
V = Q/(4 pi epsilon0 r); positive around positive charge, negative around negative charge, unlike gravitational potential.
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Give the field strength formula for a uniform field between parallel plates.
E = V/d, constant magnitude, straight parallel field lines.
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What determines whether a magnetic field exerts a force on a charge?
Only moving charges feel a force; F = BQv sin theta, zero if the charge moves parallel to B.
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State the force on a current-carrying wire in a magnetic field.
F = BIL sin theta, maximum when the wire is perpendicular to the field.
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Which rule gives the direction of force on a current in a magnetic field?
Fleming's left-hand rule.
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Why do charged particles move in circles in a uniform perpendicular magnetic field?
The magnetic force is always perpendicular to velocity, so it provides centripetal force: BQv = mv2/r.
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What are the units of magnetic flux density?
Tesla (T).
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Nuclear & particle physics

Inside the atom

The nucleus contains protons and neutrons (nucleons), with electrons in shells around it.

  • Nucleon number A = protons + neutrons. Proton number Z = protons.
  • Isotopes: same Z, different A (different neutron number).
  • Nuclear radius follows R = R0 x A^(1/3), with R0 approximately 1.2 fm. This comes from electron diffraction experiments.
  • Nuclear density is roughly constant for all nuclei, around 10^17 kg/m3, showing the nucleus is a tightly packed ball of nucleons.

Radioactive decay

  • Alpha (helium nucleus, 2p+2n): stopped by paper or a few cm of air, heavily ionising.
  • Beta-minus (fast electron): stopped by a few mm of aluminium, from n to p + e- + antineutrino.
  • Beta-plus (positron): from p to n + e+ + neutrino, only seen in artificial/proton-rich isotopes.
  • Gamma (EM photon): needs thick lead or concrete to absorb, weakly ionising, no charge or mass change.
  • Decay is random and spontaneous: you cannot predict which nucleus decays next or when.
  • Activity A = lambda x N, where lambda is the decay constant (per second) and N is the number of undecayed nuclei.
  • Decay law: N = N0 e^(-lambda t). Half-life T(1/2) = ln(2) / lambda.
  • Common mistake: forgetting activity itself decays exponentially in the same way as N.

Nuclear energy

  • Mass-energy equivalence: E = mc^2. Mass defect is the 'missing' mass converted to binding energy when a nucleus forms.
  • Binding energy per nucleon peaks around iron-56 (about 8.8 MeV per nucleon) — the most stable nucleus.
  • Fusion (light nuclei joining) and fission (heavy nuclei splitting) both release energy because products end up further up the binding-energy-per-nucleon curve, closer to iron.
  • 1 unified atomic mass unit (u) = 1.66 x 10^-27 kg, equivalent to 931.5 MeV.

Particles and antiparticles

  • Every particle has an antiparticle with the same mass and rest energy but opposite charge (and opposite other quantum numbers).
  • Annihilation: particle + antiparticle to two gamma photons (energy conserved, momentum conserved).
  • Pair production: a photon converts into a particle-antiparticle pair, needs enough photon energy to supply both rest masses, and usually happens near a nucleus to conserve momentum.

Quarks, hadrons and leptons

  • Hadrons feel the strong force: baryons (3 quarks, e.g. proton = uud, neutron = udd) and mesons (quark + antiquark).
  • Leptons (electron, muon, tau and their neutrinos) do not feel the strong force.
  • Quark charges: up/charm/top = +2/3e; down/strange/bottom = -1/3e.
  • Conservation laws to apply in every particle interaction: charge, baryon number, lepton number, and strangeness (strangeness can change in weak interactions only).

Exam tip: always check conservation of charge, baryon number and lepton number when identifying an unknown particle in an equation — it's the fastest way to the answer.

  • Nuclear radius formula: R = R0 x A^(1/3), with R0 approximately 1.2 fm
  • Nuclear density is roughly constant across all nuclei, about 10^17 kg/m3
  • Alpha particles are stopped by paper; beta by a few mm of aluminium; gamma needs thick lead or concrete
  • Beta-minus decay: neutron to proton + electron + antineutrino
  • Beta-plus decay: proton to neutron + positron + neutrino
  • Activity equation: A = lambda x N; decay law: N = N0 e^(-lambda t)
  • Half-life relation: T(1/2) = ln(2) / lambda
  • Binding energy per nucleon is greatest for iron-56, around 8.8 MeV per nucleon
  • 1 u (unified atomic mass unit) = 1.66 x 10^-27 kg = 931.5 MeV
  • Annihilation produces two gamma-ray photons; pair production needs a nucleus nearby to conserve momentum
  • Baryons contain 3 quarks, mesons contain a quark and an antiquark
  • Up-type quarks (up, charm, top) have charge +2/3e; down-type quarks (down, strange, bottom) have charge -1/3e
  • In particle interactions, charge, baryon number and lepton number are always conserved; strangeness only changes in weak interactions
What is the formula linking nuclear radius R to nucleon number A?
R = R0 x A^(1/3), where R0 is approximately 1.2 fm
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Why is nuclear density roughly the same for all nuclei?
Because volume scales with A (via R proportional to A^(1/3)) at the same rate as mass, so density stays constant at about 10^17 kg/m3
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What stops alpha, beta and gamma radiation respectively?
Alpha: paper or a few cm of air. Beta: a few mm of aluminium. Gamma: thick lead or concrete
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Write the equation for beta-minus decay in words
Neutron decays to a proton plus an electron plus an antineutrino
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Write the equation for beta-plus decay in words
Proton decays to a neutron plus a positron plus a neutrino
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What is the decay constant lambda and what equation links it to activity?
Lambda is the probability of an individual nucleus decaying per unit time (per second); Activity A = lambda x N
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State the radioactive decay law for N over time
N = N0 e^(-lambda t)
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How do you find half-life from the decay constant?
T(1/2) = ln(2) / lambda
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Which nucleus has the highest binding energy per nucleon, and roughly what value?
Iron-56, about 8.8 MeV per nucleon
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Why do both fission and fusion release energy?
Both move nuclei up the binding-energy-per-nucleon curve towards iron, so the products are more tightly bound and energy is released
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What happens in annihilation?
A particle and its antiparticle collide and convert entirely into two gamma-ray photons, conserving energy and momentum
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What is pair production and what condition must be met?
A photon converts into a particle-antiparticle pair; the photon must have enough energy to cover both rest masses, and it usually happens near a nucleus to conserve momentum
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What quarks make up a proton and a neutron?
Proton = up, up, down (uud). Neutron = up, down, down (udd)
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What are the charges of up-type and down-type quarks?
Up-type (up, charm, top) = +2/3e. Down-type (down, strange, bottom) = -1/3e
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Which four quantities must always be conserved in particle interactions, and which one is an exception?
Charge, baryon number and lepton number are always conserved; strangeness is conserved in strong and EM interactions but can change in weak interactions
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