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Mechanics & motion

Describing motion

Displacement, velocity and acceleration are vectors - direction matters, so use +/- signs on a defined axis.

Speed is distance/time (scalar); velocity is displacement/time (vector).

Acceleration is the rate of change of velocity, measured in m/s^2. Constant gradient on a velocity-time graph means constant (uniform) acceleration.

The SUVAT equations

These only work for constant (uniform) acceleration:

  • v = u + at
  • s = ut + 0.5at^2
  • v^2 = u^2 + 2as
  • s = 0.5(u + v)t

Here s = displacement, u = initial velocity, v = final velocity, a = acceleration, t = time. Always write down what each symbol equals before substituting numbers - this catches sign errors early.

Graphs

On a displacement-time graph, gradient = velocity. On a velocity-time graph, gradient = acceleration and the area under the graph = displacement. A curved displacement-time graph means changing velocity (acceleration).

Projectile motion

Split motion into horizontal and vertical components - they are independent of each other. Horizontal velocity stays constant (no air resistance assumed) while vertical motion has constant acceleration g = 9.81 m/s^2 downward. Time of flight is found from the vertical SUVAT equations, then used to find horizontal range.

Forces and Newton's laws

Newton's First Law: an object stays at rest or constant velocity unless a resultant (net) force acts on it.

Newton's Second Law: F = ma, where F is the resultant force in newtons, m is mass in kg, a is acceleration in m/s^2.

Newton's Third Law: every action has an equal and opposite reaction force, acting on the OTHER object, same type of force, same line of action.

Common mistakes to avoid

  • Mixing up mass (kg, scalar) with weight (N, force = mg, vector, acts downward).
  • Forgetting g changes sign depending on your chosen positive direction.
  • Using SUVAT when acceleration is not constant (e.g. with air resistance) - it is invalid there.
  • Not resolving forces into components correctly on inclined planes (use sin for the component along the slope, cos for perpendicular, or vice versa depending on the angle defined).
  • Confusing average speed with average velocity when the path is not straight.

Terminal velocity

As speed increases, resistive forces (drag) increase until they equal the driving force. At this point resultant force = 0, so acceleration = 0 and velocity becomes constant - this is terminal velocity.

  • Acceleration due to gravity near Earth's surface is g = 9.81 m/s^2, directed downward.
  • SUVAT equations only apply when acceleration is constant - never use them if a is changing.
  • F = ma is Newton's Second Law; force in newtons, mass in kg, acceleration in m/s^2.
  • On a velocity-time graph, the gradient gives acceleration and the area under the line gives displacement.
  • On a displacement-time graph, the gradient gives velocity.
  • In projectile motion, horizontal and vertical components of motion are completely independent.
  • Newton's Third Law pairs act on two different objects, are the same type of force, equal in size, and opposite in direction.
  • Weight = mass x g; weight is a force measured in newtons, mass is measured in kg.
  • Terminal velocity is reached when resistive force equals driving force, giving zero resultant force and zero acceleration.
  • Velocity and displacement are vectors (have direction); speed and distance are scalars (no direction).
  • v^2 = u^2 + 2as is the SUVAT equation used when time is not known or not needed.
  • At the top of a vertical projectile's path, vertical velocity is zero but vertical acceleration is still g (9.81 m/s^2).
What are the four SUVAT equations?
v = u + at, s = ut + 0.5at^2, v^2 = u^2 + 2as, s = 0.5(u + v)t - valid only for constant acceleration.
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State Newton's First Law of Motion.
An object remains at rest or moving at constant velocity unless acted on by a resultant (net) force.
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State Newton's Second Law of Motion.
F = ma - the resultant force on an object equals its mass times its acceleration.
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State Newton's Third Law of Motion.
For every action force there is an equal and opposite reaction force, acting on a different object, of the same type.
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What is the value of g used in UK A-Level Physics?
9.81 m/s^2, directed vertically downward.
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What does the gradient of a displacement-time graph represent?
Velocity.
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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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Why can horizontal and vertical motion in a projectile be treated separately?
Because they are independent - horizontal velocity is unaffected by vertical acceleration due to gravity (assuming no air resistance).
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What is terminal velocity?
The constant velocity reached when resistive (drag) force equals the driving force, giving zero resultant force and zero acceleration.
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Difference between speed and velocity?
Speed is a scalar (distance/time, no direction); velocity is a vector (displacement/time, has direction).
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Difference between mass and weight?
Mass is a scalar measured in kg (amount of matter); weight is a vector force measured in newtons, calculated as weight = mass x g.
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When can you NOT use the SUVAT equations?
When acceleration is not constant, e.g. motion with significant air resistance or changing forces.
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At the peak of a projectile's flight, what is true about its velocity and acceleration?
Vertical velocity is zero, but vertical acceleration is still g (9.81 m/s^2) downward - it never becomes zero mid-flight.
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How do you resolve a force acting at angle theta to the horizontal?
Horizontal component = F cos(theta); vertical component = F sin(theta) (or swap sin/cos depending on which angle is defined).
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Materials & energy

Density and the Young Modulus

Density is mass per unit volume: rho = m / V, measured in kg/m3. For a wire under tension, stress = Force / cross-sectional Area (Pa), and strain = extension / original length (no units, or a ratio).

The Young modulus E = stress / strain = (F/A) / (x/L), measured in Pa. It only applies within the region where stress is proportional to strain, up to the limit of proportionality on a stress-strain graph. Beyond the elastic limit, the material stops returning to its original shape when unloaded - that is plastic deformation.

Stress-strain graphs

  • Limit of proportionality: point beyond which stress is no longer proportional to strain.
  • Elastic limit: just after, beyond which permanent deformation occurs.
  • Yield point: material suddenly extends with little extra load (seen clearly in mild steel).
  • Ultimate tensile stress (UTS): maximum stress the material can withstand.
  • Breaking stress: point of fracture.

Brittle materials (like glass) snap suddenly with almost no plastic region. Ductile materials (like copper) show a long plastic region before breaking.

Energy stored in a stretched wire

Work done stretching a wire = area under the force-extension graph. If the wire obeys Hooke's law (F = kx), elastic strain energy = 1/2 F x = 1/2 k x^2. This equals the elastic potential energy stored, released fully if the wire stays within its elastic limit.

Hooke's law and the spring constant

F = kx, where k is the spring constant (N/m) - the force needed per unit extension. Springs in series: 1/k_total = 1/k1 + 1/k2. Springs in parallel: k_total = k1 + k2. This is the reverse pattern to resistors in circuits, a very common exam trap.

Common mistakes to avoid

  • Mixing up stress (force per area, Pa) with pressure - same units, different physical meaning.
  • Using diameter instead of radius when calculating cross-sectional area (A = pi r^2).
  • Forgetting that E is only valid up to the limit of proportionality, not the whole graph.
  • Confusing energy stored (area under graph) with just F times x when the graph is not a straight line - only use 1/2 F x for a linear (Hookean) region.
  • Forgetting to convert mm to m before calculating area or extension.

Practical skills

You should be able to describe the Searle's apparatus method for measuring the Young modulus of a wire, including use of a Vernier scale, control of a reference wire to cancel out temperature effects and sag, and taking repeat readings to reduce random error.

  • Young modulus E = stress / strain = (F/A) / (x/L), measured in pascals (Pa)
  • Density rho = mass / volume, standard unit kg/m3
  • Hooke's law: F = kx, valid only up to the limit of proportionality
  • Energy stored in a stretched elastic wire or spring = 1/2 F x = 1/2 k x^2 (area under a linear force-extension graph)
  • Springs in series: 1/k_total = 1/k1 + 1/k2; springs in parallel: k_total = k1 + k2
  • Elastic deformation is fully reversible; plastic deformation leaves permanent extension once the elastic limit is passed
  • The yield point is where a material extends significantly for little or no increase in load
  • Ultimate tensile stress (UTS) is the maximum stress a material can withstand before failure begins
  • Brittle materials (e.g. glass, ceramics) fracture with little or no plastic deformation; ductile materials (e.g. copper) show large plastic extension before breaking
  • Cross-sectional area of a wire uses radius, not diameter: A = pi r^2
  • Stress and pressure share the unit Pa but are conceptually different quantities
  • Searle's apparatus uses a reference wire alongside the test wire to eliminate errors from temperature change and sag
What is the equation for the Young modulus, and what is its unit?
E = stress / strain = (F/A) / (x/L); unit is pascals (Pa)
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Define stress in materials physics.
Stress = force / cross-sectional area (F/A), measured in Pa
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Define strain.
Strain = extension / original length (x/L); it has no units, it is a ratio
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State Hooke's law and its limit.
F = kx; only valid up to the limit of proportionality
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How do you find the energy stored in a stretched wire or spring obeying Hooke's law?
Energy = area under the force-extension graph = 1/2 F x = 1/2 k x^2
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What happens to k for two springs in series versus parallel?
Series: 1/k_total = 1/k1 + 1/k2 (weaker overall); Parallel: k_total = k1 + k2 (stronger overall)
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What is the difference between the limit of proportionality and the elastic limit?
Limit of proportionality is where stress stops being proportional to strain; elastic limit is just beyond it, past which the material no longer returns to its original shape
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What is the yield point on a stress-strain graph?
The point where the material suddenly extends a lot for very little extra stress, seen clearly in mild steel
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What is ultimate tensile stress (UTS)?
The maximum stress a material can withstand before it starts to fail
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Give one key difference between brittle and ductile materials on a stress-strain graph.
Brittle materials fracture with almost no plastic region; ductile materials show a long plastic region before breaking
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What is the formula for density, and its standard SI unit?
rho = mass / volume (m/V); unit kg/m3
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Why is a reference wire used in Searle's apparatus?
To cancel out errors caused by temperature changes and sag in the support, since both wires experience the same conditions
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What common area mistake do students make when calculating stress in a wire?
Using the diameter instead of the radius in A = pi r^2, which gives a value four times too large
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Can you always use E = 1/2 F x to find energy stored?
No - only for a linear (Hookean) force-extension graph; otherwise you must find the actual area under the curve
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Electricity & circuits

Current, charge and potential difference

Charge Q = It, measured in coulombs (C). One coulomb is the charge passing a point when a current of 1 A flows for 1 second.

Potential difference V = W/Q, the energy transferred per coulomb of charge (volts, V).

Current is the rate of flow of charge: I = ΔQ/Δt.

Ohm's law and resistance

Resistance R = V/I, measured in ohms (Ω).

Ohm's law: current through a metallic conductor is proportional to pd if temperature stays constant, giving a straight line I-V graph through the origin.

A filament lamp curves as temperature rises (resistance increases). A diode conducts one way only, with near-zero current in reverse until breakdown.

Resistivity

R = ρL/A, where ρ is resistivity (Ω m), L is length and A is cross-sectional area.

Common mistake: forgetting to convert diameter to radius and to square it correctly when finding A = πr².

Power and energy

P = IV = I²R = V²/R.

Energy transferred W = Pt = IVt.

Series and parallel circuits

Series: same current everywhere, pds add up (V = V1 + V2 + ...), total resistance R = R1 + R2 + ...

Parallel: same pd across each branch, currents add up, 1/R = 1/R1 + 1/R2 + ...

Common mistake: mixing up which quantity is shared in series vs parallel.

EMF and internal resistance

EMF ε is the energy given per coulomb by the source, including energy wasted inside it.

ε = I(R + r), where r is internal resistance and R is external (load) resistance.

Terminal pd V = ε - Ir. Lost volts = Ir.

To find ε and r experimentally, plot V against I; the y-intercept is ε and the gradient is -r.

Potential dividers

Output voltage from a potential divider: Vout = (R2 / (R1 + R2)) × Vin.

Sensors (LDR, thermistor) used in one arm let the output vary with light or temperature.

Circuit rules (Kirchhoff)

Kirchhoff's first law: current into a junction equals current out (conservation of charge).

Kirchhoff's second law: the sum of emfs around a loop equals the sum of pd drops (conservation of energy).

Common exam mistakes

  • Forgetting internal resistance when a cell is under load, so calculated and measured emf disagree.
  • Using the wrong resistor combination formula for series vs parallel.
  • Not keeping the ammeter's resistance negligible and voltmeter's resistance very high when reasoning about circuit assumptions.
  • Confusing energy (joules) with power (watts) in calculations.
  • Charge Q = It, measured in coulombs, where 1 C is the charge from 1 A flowing for 1 second.
  • Potential difference V = W/Q is the energy transferred per coulomb, measured in volts.
  • Resistance R = V/I, measured in ohms, and Ohm's law holds only at constant temperature.
  • Resistivity formula is R = rho L / A, with resistivity measured in ohm metres.
  • Power can be found three ways: P = IV = I squared R = V squared / R.
  • In series circuits current is the same throughout and total resistance is R1 + R2 + ...
  • In parallel circuits pd is the same across each branch and 1/R total = 1/R1 + 1/R2 + ...
  • EMF equation is epsilon = I(R + r), where r is the internal resistance of the source.
  • Terminal pd equals emf minus lost volts: V = epsilon - Ir.
  • On an emf-internal resistance graph of V against I, the y-intercept gives emf and the gradient gives minus r.
  • Potential divider output is Vout = (R2 / (R1 + R2)) times Vin.
  • Kirchhoff's first law is conservation of charge at a junction; the second law is conservation of energy around a loop.
What is the equation linking charge, current and time?
Q = It, where Q is in coulombs, I in amps, t in seconds.
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Define the volt in terms of energy and charge.
One volt is one joule of energy transferred per coulomb of charge: V = W/Q.
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State Ohm's law and its condition.
Current is proportional to pd, provided temperature (and other physical conditions) stay constant: V = IR.
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Give the resistivity equation and its units.
R = rho L / A; resistivity rho is measured in ohm metres (Ohm m).
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Write the three forms of the power equation for a resistor.
P = IV = I squared R = V squared / R.
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How does total resistance combine for resistors in series?
They simply add: R total = R1 + R2 + R3 + ...
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How does total resistance combine for resistors in parallel?
Reciprocals add: 1/R total = 1/R1 + 1/R2 + ...
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What is emf and how does it differ from terminal pd?
Emf is the total energy per coulomb supplied by the source; terminal pd is emf minus the energy per coulomb lost to internal resistance (V = epsilon - Ir).
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Write the full emf equation including internal resistance.
epsilon = I(R + r), where R is external resistance and r is internal resistance.
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How do you find emf and internal resistance from a graph of V against I?
The y-intercept equals emf; the gradient equals minus the internal resistance r.
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State the potential divider output equation.
Vout = (R2 / (R1 + R2)) times Vin, where R2 is the resistor across which Vout is measured.
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State Kirchhoff's first law.
The sum of currents entering a junction equals the sum of currents leaving it (conservation of charge).
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State Kirchhoff's second law.
Around any closed loop, the sum of the emfs equals the sum of the pd drops (conservation of energy).
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What shape is the I-V graph for a filament lamp and why?
It curves and flattens as current increases, because the filament heats up and its resistance rises.
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What is 'lost volts' in a circuit with internal resistance?
The pd used up driving current through the internal resistance of the source, equal to Ir.
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Waves & optics

Wave basics

  • A wave transfers energy without transferring matter.
  • Key equation: v = f x wavelength (lambda), where v is speed in m/s, f is frequency in Hz, lambda is wavelength in m.
  • Transverse waves (e.g. light, water surface waves) oscillate perpendicular to the direction of travel; longitudinal waves (e.g. sound) oscillate parallel to it.
  • Only transverse waves can be polarised - this is strong evidence that light is transverse, not longitudinal.

Superposition and standing waves

  • Superposition: when two waves meet, the resultant displacement is the vector sum of the individual displacements.
  • Standing (stationary) waves form from two identical waves travelling in opposite directions, usually by reflection.
  • A standing wave has nodes (zero amplitude, always) and antinodes (maximum amplitude) that stay fixed in position - unlike a progressive wave, no energy is transferred along a standing wave.
  • Distance between adjacent nodes = lambda/2.
  • For a stretched string fixed at both ends, the fundamental frequency has a node at each end and one antinode in the middle: length L = lambda/2.

Interference and diffraction

  • Coherent sources have the same frequency and a constant phase difference.
  • Path difference of a whole number of wavelengths (n x lambda) gives constructive interference (in phase); path difference of (n + 1/2) x lambda gives destructive interference (antiphase).
  • Young's double-slit equation: lambda = ax/D, where a is slit separation, x is fringe spacing, D is slit-to-screen distance. Common mistake: mixing up a and x, or forgetting D must be much bigger than a.
  • Diffraction gratings: d sin(theta) = n x lambda, where d is the grating spacing (d = 1/N, N = lines per metre). More lines per mm gives wider-spaced, sharper maxima.
  • Diffraction is most noticeable when the gap size is close to the wavelength of the wave.

Refraction and refractive index

  • Snell's law: n1 sin(theta1) = n2 sin(theta2).
  • Absolute refractive index n = c/v (c = speed of light in vacuum, v = speed in the medium).
  • Total internal reflection occurs only when light travels from a denser to a less dense medium AND the angle of incidence exceeds the critical angle: sin(C) = 1/n (going from medium of refractive index n into air).
  • This is the basis of fibre optics - the core has a higher refractive index than the cladding so light is trapped by repeated total internal reflection.

Common exam mistakes

  • Confusing path difference (a distance) with phase difference (an angle or fraction of a cycle).
  • Forgetting units: theta in Snell's law and the grating equation is measured from the normal, not the surface.
  • Writing lambda = ax/D upside down - remember fringe spacing x increases if D increases or a decreases.
  • Stating standing waves 'transfer energy' - they do not, only progressive waves do.
  • Wave speed equation: v = f x lambda, with v in m/s, f in Hz, lambda in m.
  • Only transverse waves (like light) can be polarised - this proves light is transverse.
  • Standing waves have nodes and antinodes fixed in position; adjacent nodes are lambda/2 apart.
  • A standing wave transfers no net energy along its length, unlike a progressive wave.
  • Young's double-slit equation: lambda = ax/D (a = slit separation, x = fringe spacing, D = slit-to-screen distance).
  • Diffraction grating equation: d sin(theta) = n x lambda, where d = 1/N (N = lines per metre).
  • Constructive interference occurs at path difference n x lambda; destructive at (n + 1/2) x lambda.
  • Refractive index n = c/v, and Snell's law is n1 sin(theta1) = n2 sin(theta2).
  • Total internal reflection needs denser-to-less-dense travel AND angle of incidence greater than the critical angle C, where sin(C) = 1/n.
  • Diffraction is most significant when the gap width is similar in size to the wavelength.
  • All angles in Snell's law and the diffraction grating equation are measured from the normal, not the surface.
  • Coherent sources must have the same frequency and a constant phase difference for stable interference patterns.
State the wave speed equation and its units.
v = f x lambda; v in m/s, f in Hz, lambda in m.
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Why does polarisation prove light is a transverse wave?
Only transverse waves can be polarised; light can be polarised, so it must be transverse.
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What is a node and what is an antinode in a standing wave?
A node is a point of permanently zero amplitude; an antinode is a point of maximum amplitude. Both stay fixed in position.
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What is the distance between two adjacent nodes in a standing wave?
lambda/2 (half a wavelength).
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Does a standing wave transfer energy along its length?
No - unlike a progressive wave, a standing wave transfers no net energy.
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State Young's double-slit equation and define each symbol.
lambda = ax/D, where a = slit separation, x = fringe spacing, D = distance from slits to screen.
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State the diffraction grating equation.
d sin(theta) = n x lambda, where d is the grating spacing (d = 1/N, N = lines per metre), n is the order, theta is measured from the normal.
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What path difference gives constructive interference?
A whole number of wavelengths: path difference = n x lambda.
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What path difference gives destructive interference?
(n + 1/2) x lambda - i.e. an odd number of half wavelengths.
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Define absolute refractive index.
n = c/v, where c is the speed of light in a vacuum and v is the speed of light in the medium.
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State Snell's law.
n1 sin(theta1) = n2 sin(theta2), with angles measured from the normal.
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What two conditions are needed for total internal reflection?
Light must travel from a denser to a less dense medium, and the angle of incidence must exceed the critical angle C.
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How is the critical angle calculated?
sin(C) = 1/n, where n is the refractive index of the denser medium (light exiting into air).
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When is diffraction most noticeable?
When the gap or obstacle size is similar to the wavelength of the wave.
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What two conditions define coherent sources?
Same frequency and a constant (unchanging) phase difference.
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Fields (gravitational, electric, magnetic)

Gravitational fields

A gravitational field is a region where a mass feels a force. Field strength g = F/m, measured in N/kg. For a point (or spherical) mass, g = GM/r^2, where G = 6.67 x 10^-11 N m^2 kg^-2. This is an inverse-square law, so doubling r cuts g to a quarter.

Gravitational potential V at a point is the work done per unit mass bringing a small test mass from infinity to that point. V = -GM/r. It is always negative, and zero at infinity, because gravity is always attractive and does positive work as mass falls inwards. The gradient of a V against r graph gives -g.

Orbits: for a satellite in a circular orbit, gravitational force provides centripetal force, so GMm/r^2 = mv^2/r = m(4 pi^2/T^2)r. This rearranges to T^2 = (4 pi^2/GM) r^3, Kepler's third law. Geostationary orbits have T = 24 hours (23 h 56 min sidereal) and sit above the equator at radius about 4.2 x 10^7 m.

Electric fields

Electric field strength E = F/Q, in N/C or V/m. For a point charge, E = Q/(4 pi epsilon0 r^2), with epsilon0 = 8.85 x 10^-12 F/m. Coulomb's law gives the force F = Qq/(4 pi epsilon0 r^2). Electric potential V = Q/(4 pi epsilon0 r), zero at infinity, and can be positive or negative depending on the sign of the source charge.

Uniform fields exist between parallel plates: E = V/d, pointing from positive to negative plate. Work done moving charge q through potential difference V is W = qV. This underpins the electronvolt: 1 eV = 1.6 x 10^-19 J.

Comparing gravitational and electric fields

Both follow inverse-square force laws and have potentials that go as 1/r, so the equations are structurally identical (swap G and M for 1/(4 pi epsilon0) and Q). The key difference: gravity is always attractive, electric force can attract or repel depending on charge signs.

Magnetic fields

A moving charge in a magnetic field feels F = BQv sin(theta), maximum when velocity is perpendicular to B. A current-carrying wire feels F = BIL sin(theta). Flux density B is measured in tesla (T). Use Fleming's left-hand rule for force direction on a positive charge or conventional current.

A charged particle moving perpendicular to B follows a circular path, since the magnetic force is always perpendicular to velocity and does no work, so speed (and kinetic energy) stays constant. This is the basis of the mass spectrometer and cyclotron.

Common mistakes

  • Forgetting the minus sign in gravitational potential, or forgetting that electric potential can be negative.
  • Mixing up field strength (vector, force per unit charge/mass) with potential (scalar, energy per unit charge/mass).
  • Using g = GM/r^2 for objects inside a uniform sphere, where it does not apply in the same form.
  • Forgetting magnetic force does no work, so it cannot change a particle's speed, only its direction.
  • Newton's law of gravitation: F = GMm/r^2, with G = 6.67 x 10^-11 N m^2 kg^-2
  • Gravitational field strength g = GM/r^2 and is always directed towards the mass
  • Gravitational potential V = -GM/r, always negative, zero only at infinity
  • Kepler's third law from orbital mechanics: T^2 = (4 pi^2/GM) r^3 for a circular orbit
  • Geostationary satellites orbit in 24 hours above the equator at radius roughly 4.2 x 10^7 m
  • Coulomb's law: F = Qq/(4 pi epsilon0 r^2), with epsilon0 = 8.85 x 10^-12 F/m
  • Electric field strength between parallel plates is uniform: E = V/d
  • Electric potential V = Q/(4 pi epsilon0 r) can be positive or negative depending on charge sign
  • Work done moving charge q through potential difference V: W = qV, and 1 eV = 1.6 x 10^-19 J
  • Force on a moving charge in a magnetic field: F = BQv sin(theta), maximum at 90 degrees
  • Force on a current-carrying conductor in a field: F = BIL sin(theta)
  • A charged particle moving perpendicular to a uniform magnetic field travels in a circle at constant speed, since magnetic force does no work
What is the equation for gravitational field strength due to a point mass?
g = GM/r^2, an inverse-square law directed towards the mass
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What is the value of the gravitational constant G?
G = 6.67 x 10^-11 N m^2 kg^-2
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Why is gravitational potential always negative?
Because gravity is attractive, so work must be done to move a mass away to infinity (where V = 0); moving inward releases energy, giving negative potential
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State Kepler's third law as derived from circular orbits.
T^2 = (4 pi^2/GM) r^3, linking orbital period and orbital radius
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What defines a geostationary orbit?
Period of 24 hours, above the equator, orbital radius about 4.2 x 10^7 m, so it stays above the same point on Earth
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State Coulomb's law.
F = Qq/(4 pi epsilon0 r^2), the electrostatic force between two point charges
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What is the field strength between two parallel charged plates?
E = V/d, a uniform field pointing from the positive to the negative plate
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What is the equation for electric potential due to a point charge?
V = Q/(4 pi epsilon0 r); can be positive or negative depending on the sign of Q
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Define one electronvolt.
The energy gained by one electron accelerated through a potential difference of 1 volt: 1 eV = 1.6 x 10^-19 J
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What is the force on a charge moving through a magnetic field?
F = BQv sin(theta), maximum when velocity is perpendicular to the field (theta = 90 degrees)
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What is the force on a current-carrying wire in a magnetic field?
F = BIL sin(theta), found using Fleming's left-hand rule for direction
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Why does a charged particle move in a circle in a uniform magnetic field?
The magnetic force is always perpendicular to velocity, so it changes direction but not speed, providing centripetal force
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What key structural similarity links gravitational and electric field equations?
Both follow inverse-square force laws and 1/r potentials; swapping G and M for 1/(4 pi epsilon0) and Q converts one set of equations to the other
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What is the main difference between gravitational and electric forces?
Gravity is always attractive; electric force can be attractive or repulsive depending on the signs of the charges
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Nuclear & particle physics

Atomic structure

An atom has a tiny, dense, positively-charged nucleus (protons + neutrons) surrounded by orbiting electrons. Nuclide notation: A over Z, X, where Z = proton number (atomic number) and A = nucleon number (mass number, protons + neutrons). Isotopes have the same Z but different A (different neutron number).

Rutherford scattering

Alpha particles fired at thin gold foil mostly passed straight through, but a small fraction deflected through large angles, some straight back. This proved the atom is mostly empty space with a small, dense, positive nucleus (the 'plum pudding' model was disproved). Closest approach distance gives an estimate of nuclear radius.

Nuclear radius and density

Nuclear radius follows R = r0 A^(1/3), where r0 is about 1.2 fm (1.2 x 10^-15 m). This means nuclear density is roughly constant for all nuclei, around 10^17 kg per cubic metre, far denser than ordinary matter.

Radioactive decay

Alpha decay emits a helium nucleus (2 protons, 2 neutrons), reducing A by 4 and Z by 2. Beta-minus decay emits an electron and an antineutrino as a neutron converts to a proton, so Z increases by 1, A unchanged. Beta-plus decay emits a positron and a neutrino as a proton converts to a neutron. Gamma emission releases energy only, no change to A or Z.

Activity and half-life

Activity A = lambda N, where lambda is the decay constant and N is the number of undecayed nuclei. Decay is exponential: N = N0 e^(-lambda t). Half-life T(1/2) = ln2 / lambda. Common mistake: forgetting activity and count rate are proportional to N, not to A (mass number).

Particle physics basics

Matter is built from quarks (up, down, etc.) and leptons (electron, neutrino). Hadrons are made of quarks: baryons (3 quarks, e.g. proton = uud, neutron = udd) and mesons (quark-antiquark pair). Every particle has an antiparticle with opposite charge but equal mass.

Conservation rules

In all particle interactions, charge, baryon number, lepton number, and strangeness (in strong/EM interactions only) must be conserved. Common mistake: assuming strangeness is conserved in weak interactions - it isn't, which explains slow kaon decay.

Einstein's mass-energy equivalence

E = mc^2 links mass and energy. Binding energy is the energy needed to split a nucleus into separate nucleons; it corresponds to a mass defect (the nucleus has less mass than its separate parts). Binding energy per nucleon peaks around iron-56, which is why fusion releases energy for light nuclei and fission releases energy for heavy nuclei.

Common exam mistakes

Don't confuse mass number (A) with atomic mass in kg. Always balance both A and Z in decay equations. Remember antineutrinos/neutrinos carry away energy and momentum in beta decay, explaining the continuous energy spectrum of beta particles.

  • Nuclide notation is A over Z X: Z = proton number, A = nucleon number (protons + neutrons)
  • Nuclear radius R = r0 A^(1/3), with r0 approximately 1.2 x 10^-15 m (1.2 fm)
  • Nuclear density is roughly constant across all nuclei at about 10^17 kg per cubic metre
  • Alpha decay: A decreases by 4, Z decreases by 2 (emits a helium-4 nucleus)
  • Beta-minus decay: a neutron becomes a proton, emitting an electron and an antineutrino; Z increases by 1
  • Activity equation: A = lambda N, where lambda is the decay constant and N the number of undecayed nuclei
  • Half-life formula: T(1/2) = ln2 / lambda
  • Baryons contain 3 quarks (proton = uud, neutron = udd); mesons contain a quark and an antiquark
  • Charge, baryon number and lepton number are conserved in every particle interaction
  • Strangeness is conserved in strong and electromagnetic interactions but NOT in weak interactions
  • Binding energy per nucleon is highest for iron-56, which is why fusion suits light nuclei and fission suits heavy nuclei
  • E = mc^2 links the mass defect of a nucleus to its binding energy
What does the nuclide notation A over Z X tell you?
Z is the proton (atomic) number and A is the nucleon (mass) number, protons plus neutrons
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What did Rutherford's alpha scattering experiment prove about atomic structure?
The atom is mostly empty space with a tiny, dense, positively charged nucleus, disproving the plum pudding model
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State the equation for nuclear radius
R = r0 A^(1/3), where r0 is about 1.2 x 10^-15 m
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Why is nuclear density roughly constant across all elements?
Because volume scales with A (via R proportional to A^(1/3)) in the same way mass does, so density stays around 10^17 kg per cubic metre
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What is emitted in alpha decay and how do A and Z change?
A helium-4 nucleus is emitted; A decreases by 4 and Z decreases by 2
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What happens to a neutron during beta-minus decay?
It converts into a proton, emitting an electron and an antineutrino; Z increases by 1, A stays the same
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Give the equation linking activity, decay constant and number of nuclei
A = lambda N
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Give the equation linking half-life and decay constant
T(1/2) = ln2 / lambda
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What quarks make up a proton and a neutron?
Proton = uud (two up, one down); neutron = udd (one up, two down)
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What is the difference between a baryon and a meson?
A baryon is made of 3 quarks; a meson is made of a quark and an antiquark
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Which conservation laws must hold in every particle interaction?
Charge, baryon number and lepton number are always conserved
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Is strangeness conserved in weak interactions?
No, strangeness is only conserved in strong and electromagnetic interactions, not weak ones
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Around which nucleus does binding energy per nucleon peak, and why does this matter?
Iron-56; it is why fusion releases energy for light nuclei and fission releases energy for heavy nuclei
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What does E = mc^2 relate in the context of nuclear binding energy?
It links the mass defect (missing mass) of a nucleus to the binding energy holding its nucleons together
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Why does beta decay produce a continuous energy spectrum for the emitted electron?
Because the antineutrino (or neutrino) also carries away a variable share of the energy and momentum
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