ExaminerPrep · Formula handout · IB Physics HL
Equations Not in the Data Booklet: HL edition
For IB Diploma Physics HL (syllabus first assessed 2025): all SL equations plus the HL ones, with every symbol explained
examinerprep.comEvery equation below is one you must know or be able to derive yourself, because it is not printed in the data booklet you get in Papers 1 and 2. Under each one, a symbol key gives what every symbol means and its SI unit.
HL edition
This sheet has every SL equation plus the Additional Higher Level ones. HL-only topics and equations carry an HL tag, so you can see at a glance what SL students do not need.
Taking SL? The SL edition leaves the HL content out.
How to use this sheet
Learn these until you can write them from memory, and know where each one comes from: most are two lines of algebra away from a booklet equation, and a derivation is worth knowing in case the question asks you to show it.
- SL+HL = everyone needs it. HL = Additional Higher Level only.
- Derived = not printed, but follows from a booklet equation. Practise the derivation once.
- The symbol key under each box lists every symbol, what it stands for and its SI unit. “(no unit)” marks a dimensionless quantity.
- Exam tip and Common error boxes point out where marks are usually gained or lost.
- Equations are magnitudes unless a sign is shown. Use SI units throughout unless told otherwise.
- The data booklet can be revised between sessions. Check this sheet against the current version before your exams.
Given in the data booklet: know how to use it
These are printed, so they are not in the lists below, but you still need to recognise and rearrange them quickly: the period, frequency and angular frequency relation; linear speed from angular speed in circular motion; current as rate of flow of charge; resistance from potential difference and current; electric field strength as force per unit charge; the de Broglie relation (also used for photon momentum); the Doppler shift for light; heat-engine efficiency as useful work over energy input; orbital speed and escape speed (in the higher level part of the booklet); the energy equivalent of the atomic mass unit and the value of hc.
Tools: uncertainties, maths and graphs
Uncertainties SL+HL
The booklet gives the propagation rules (sums, products/quotients, powers). These are not given:
Fractional and percentage uncertainty
Symbolsx = measured value (any unit)Δx = absolute uncertainty in x (same unit as x)fractional, percentage = relative size of the uncertainty (no unit)
Uncertainty from repeated readings (half the range)
SymbolsΔx = absolute uncertainty (same unit as x)xmax, xmin = largest and smallest of the repeated readings (unit of x)
Multiplying by an exact constant
Symbolsy = calculated quantity (unit of y)k = exact constant, with no uncertainty of its own (unit of y/x)x = measured quantity (unit of x)Δx, Δy = absolute uncertainties in x and y (units of x, y)
Uncertainty in a gradient (from the steepest and shallowest lines through all error bars)
Symbolsm = gradient of the line of best fit (y-axis unit ÷ x-axis unit)mmax, mmin = gradients of the steepest and shallowest lines (same as m)Δm = uncertainty in the gradient (same as m)
Percentage difference from an accepted value
Symbolsxexp = your experimental value (any unit)xaccepted = accepted (literature) value (same unit)% difference = size of the discrepancy (no unit)
Exam tip
Quote the absolute uncertainty to 1 significant figure (2 is acceptable if the first digit is 1), then round the value to the same decimal place.
Maths not in the booklet SL+HL
The booklet gives the volume of a sphere but not its surface area. You need it for stars (E.5) and for radiation from spheres (B.1).
SymbolsAsphere = surface area of the sphere (m2)r = radius (m)
Small-angle approximation (θ in radians, roughly θ < 0.1 rad; behind s = λD/d and θ = λ/b)
Symbolsθ = angle (rad)
Arc length and angle
Symbolss = arc length (m)r = radius (m)θ = angle subtended at the centre (rad)ω = angular speed (rad s−1)Δθ = angle turned through (rad)Δt = time taken (s)
Linearising for graphs
Symbolsy, x = the two variables plotted (any units)k = constantn = power of x (no unit)A = value of y when x = 0 (unit of y)λ = decay constant of the exponential (unit of 1/x)e = base of natural logarithms, ≈ 2.718 (no unit)ln = natural logarithm (log to base e)
Graph relationships SL+HL
| Graph | Gradient gives | Area under it gives |
|---|---|---|
| displacement–time | velocity | — |
| velocity–time | acceleration | displacement |
| acceleration–time | — | change in velocity |
| force–time | rate of change of momentum | impulse (Δp) |
| force–extension | spring constant k | work done / elastic energy |
| pressure–volume HL | — | work done by or on the gas |
| power–time | — | energy transferred |
| current–time | — | charge |
SymbolsΔp = impulse, equal to the change in momentum (kg m s−1 or N s)k = spring constant (N m−1)
Common error
Reading the gradient of a curve from one point. Draw a tangent at the point asked for and use a large triangle.
A. Space, time and motion
A.1 Kinematics SL+HL
Definitions of average speed, average velocity and acceleration (the booklet gives only the four suvat equations)
Symbolsdistance, time = total path length and time taken (m, s)v = average velocity (m s−1)Δs = displacement (m)Δt = time interval (s)a = average acceleration (m s−2)Δv = change in velocity (m s−1)
Projectile components (launch speed u at angle θ above the horizontal)
Symbolsu = launch speed (m s−1)θ = launch angle above the horizontal (° or rad)ux, uy = horizontal and vertical components of the launch velocity (m s−1)ax, ay = horizontal and vertical acceleration (upward positive) (m s−2)g = gravitational field strength (m s−2 or N kg−1)
Derived Level ground, no air resistance: time of flight, maximum height, range
SymbolsT = time of flight (s)H = maximum height above the launch point (m)R = horizontal range (m)u = launch speed (m s−1)θ = launch angle above the horizontal (° or rad)g = gravitational field strength (m s−2 or N kg−1)
Exam tip
These three only hold for launch and landing at the same height. In any other case, apply suvat separately to the horizontal and vertical motion.
A.2 Forces and momentum SL+HL
Equilibrium (Newton’s first law)
SymbolsΣF = resultant (net) force (N)a = acceleration (m s−2)
Conservation of momentum (isolated system)
Symbolsm1, m2 = masses of the two objects (kg)u1, u2 = velocities before the interaction (signed) (m s−1)v1, v2 = velocities after the interaction (signed) (m s−1)
Elastic collision: kinetic energy is also conserved. Explosion from rest: total momentum after is zero.
Weight components on a slope (angle θ to the horizontal)
SymbolsF∥ = component of the weight down the slope (N)F⊥ = component of the weight perpendicular to the slope (N)m = mass (kg)g = gravitational field strength (m s−2 or N kg−1)θ = angle of the slope to the horizontal (° or rad)
Derived Centripetal force (from F = ma and a = v2/r)
SymbolsF = centripetal (resultant) force (N)m = mass (kg)v = speed (m s−1)r = radius of the circle (m)ω = angular speed (rad s−1)
Common error
Drawing a separate “centripetal force” on a free-body diagram. It is the resultant of the real forces (tension, gravity, friction, normal force).
Normal force in a lift (upward acceleration a positive)
SymbolsN = normal force from the floor (N)m = mass of the person or object (kg)g = gravitational field strength (m s−2 or N kg−1)a = acceleration of the lift, upward positive (m s−2)
Derived Terminal velocity of a sphere (weight = drag + buoyancy, using Stokes’ law)
Symbolsm = mass of the sphere (kg)g = gravitational field strength (m s−2 or N kg−1)η = viscosity of the fluid (Pa s)r = radius of the sphere (m)vt = terminal speed (m s−1)ρf = density of the fluid (kg m−3)V = volume of the sphere (m3)ρs = density of the sphere (kg m−3)
A.3 Work, energy and power SL+HL
Conservation of energy (no dissipative forces)
SymbolsEk = kinetic energy (J)Ep = gravitational potential energy (J)m = mass (kg)v = speed (m s−1)g = gravitational field strength (m s−2 or N kg−1)Δh = change in height (m)
Work–energy theorem
SymbolsWnet = work done by the resultant force (J)ΔEk = change in kinetic energy (J)
Power as rate of energy transfer (the booklet writes power in terms of work done; this is the energy form)
SymbolsP = power (W)E = energy transferred (J)t = time taken (s)
Exam tip
With friction, energy lost = friction force × distance along the path, not the vertical height.
A.4 Rigid body mechanics HL
Rolling without slipping (v = ωr is in the booklet under circular motion and also holds for the centre of a rolling object; the acceleration form is not printed)
Symbolsa = linear acceleration of the centre (m s−2)α = angular acceleration (rad s−2)r = radius of the rolling object (m)
Total kinetic energy of a rolling object
SymbolsEk = total kinetic energy (J)m = mass (kg)v = speed of the centre of mass (m s−1)I = moment of inertia about the axis through the centre (kg m2)ω = angular speed (rad s−1)
Derived Rolling down a height h from rest
Symbolsm = mass (kg)g = gravitational field strength (m s−2 or N kg−1)h = vertical height descended (m)v = speed of the centre at the bottom (m s−1)I = moment of inertia (kg m2)r = radius of the rolling object (m)
Rotational work and power
SymbolsW = work done by the torque (J)τ = torque (N m)Δθ = angle turned through (rad)P = power (W)ω = angular speed (rad s−1)
Rotational equilibrium (both conditions together)
SymbolsΣF = resultant force (N)Στ = resultant torque about any axis (N m)
Conservation of angular momentum (no external torque) and angular momentum of a point mass
SymbolsI1, I2 = moments of inertia before and after (kg m2)ω1, ω2 = angular speeds before and after (rad s−1)L = angular momentum (kg m2 s−1)m = mass of the point object (kg)v = its speed (m s−1)r = perpendicular distance from the axis to its line of motion (m)
Common error
Assuming rotational kinetic energy is conserved when I changes. Angular momentum is conserved; kinetic energy usually is not.
A.5 Galilean and special relativity HL
Inverse Lorentz transformations (from S′ back to S)
Symbolsx, t = position and time of an event in frame S (m, s)x′, t′ = position and time of the same event in frame S′ (m, s)v = velocity of S′ relative to S (m s−1)γ = Lorentz factor (no unit)c = speed of light in a vacuum (constant, m s−1)
Interval forms (use these for two events)
SymbolsΔx, Δt = distance and time between two events in S (m, s)Δx′, Δt′ = distance and time between the same events in S′ (m, s)v = velocity of S′ relative to S (m s−1)γ = Lorentz factor (no unit)c = speed of light in a vacuum (constant, m s−1)
Derived Relativity of simultaneity (events simultaneous in S, Δt = 0)
SymbolsΔt′ = time between the events in S′ (s)γ = Lorentz factor (no unit)v = velocity of S′ relative to S (m s−1)Δx = distance between the events in S (m)c = speed of light in a vacuum (constant, m s−1)
Exam tip
Proper time Δt0 is measured by the observer who sees both events at the same place; proper length L0 is measured in the frame where the object is at rest. Identify them before using the booklet equations.
B. The particulate nature of matter
B.1 Thermal energy transfers SL+HL
Heating with a known power (e.g. an electric heater, P = IV)
SymbolsP = power of the heater (W)t = heating time (s)m = mass heated (kg)c = specific heat capacity (J kg−1 K−1)ΔT = temperature change (K or °C)L = specific latent heat (J kg−1)
Mixing: energy lost by the hot body = energy gained by the cold body (no losses)
Symbolsm1, m2 = masses of the hot and cold bodies (kg)c1, c2 = their specific heat capacities (J kg−1 K−1)T1 = initial temperature of the hot body (K or °C)T2 = initial temperature of the cold body (K or °C)Tf = final common temperature (K or °C)
Derived Power radiated per unit area by a black body
SymbolsP = power radiated (W)A = surface area of the emitter (m2)σ = Stefan–Boltzmann constant (constant, W m−2 K−4)T = absolute temperature of the surface (K)
Exam tip
A temperature change is the same in K and °C, but σT4 and Wien’s law need absolute temperature in K.
B.2 Greenhouse effect SL+HL
Intensity
SymbolsI = intensity (W m−2)P = power (W)A = area perpendicular to the direction of energy flow (m2)
Mean incoming solar intensity on the whole Earth (disc area πR2 intercepts, sphere area 4πR2 shares)
SymbolsImean = incoming intensity averaged over the whole surface of the Earth (W m−2)S = solar constant: intensity arriving at the top of the atmosphere, on a surface facing the Sun (W m−2)
Derived Energy balance for an equilibrium planet (albedo α, emissivity e)
Symbolsα = albedo (fraction reflected) (no unit)S = solar constant (W m−2)e = emissivity (no unit)σ = Stefan–Boltzmann constant (constant, W m−2 K−4)T = mean surface temperature of the planet (K)
Common error
Forgetting the factor 4, or using α instead of (1 − α) for the absorbed fraction.
B.3 Gas laws SL+HL
Amount of substance from mass (M = molar mass in kg mol−1)
Symbolsn = amount of substance (mol)m = mass of gas (kg)M = molar mass (kg mol−1)
Derived Single-change gas laws (fixed amount of ideal gas)
Symbolsp1, p2 = pressure before and after (Pa)V1, V2 = volume before and after (m3)T1, T2 = absolute temperature before and after (K)
Link between the constants
SymbolsR = molar gas constant (constant, J mol−1 K−1)NA = Avogadro constant (constant, mol−1)kB = Boltzmann constant (constant, J K−1)
Derived rms speed of gas molecules (from p = ⅓ρv2 and pV = nRT)
Symbolsvrms = root mean square speed of the molecules (m s−1)R = molar gas constant (constant, J mol−1 K−1)T = absolute temperature (K)M = molar mass (kg mol−1)kB = Boltzmann constant (constant, J K−1)mmolecule = mass of one molecule (kg)
Common error
Using grams per mole for M. Convert to kg mol−1 first.
B.4 Thermodynamics HL
Sign convention with Q = ΔU + W: W is work done by the gas (positive on expansion).
Special processes
| Process | Condition | First law becomes |
|---|---|---|
| Isovolumetric (isochoric) | W = 0 | Q = ΔU |
| Isobaric | p constant | W = pΔV |
| Isothermal | ΔU = 0 | Q = W, and pV = constant |
| Adiabatic | Q = 0 | W = −ΔU |
| Complete cycle | ΔU = 0 | Qnet = Wnet = enclosed area on p–V |
SymbolsQ = energy transferred to the gas by heating (J)ΔU = change in internal energy of the gas (J)W = work done by the gas (J)p = pressure (Pa)ΔV = change in volume (m3)V = volume (m3)Qnet, Wnet = net energy in and net work out over one cycle (J)
Derived Adiabatic change for a monatomic ideal gas, in terms of T
SymbolsT = absolute temperature (K)V = volume (m3)2/3 = exponent for a monatomic gas (no unit)
Heat engines: energy in, work out and energy rejected (the booklet gives efficiency as useful work over energy input; combine it with the energy balance)
SymbolsQH = energy taken in from the hot reservoir (J)W = useful work done by the engine (J)QC = energy rejected to the cold reservoir (J)η = efficiency (no unit)
Second law (isolated system)
SymbolsΔS = change in entropy of the isolated system (J K−1)
Exam tip
No real engine can beat the Carnot efficiency between the same two temperatures. Use it as a check on your answer.
B.5 Current and circuits SL+HL
Kirchhoff’s laws
SymbolsΣIin, ΣIout = total current into and out of a junction (A)Σε = sum of the emfs around a closed loop (V)ΣIR = sum of the potential differences across the resistances in that loop (V)I = current (A)R = resistance (Ω)ε = emf (V)
Potential divider
SymbolsVout = output potential difference, across R2 (V)Vin = potential difference across the whole divider (V)R1, R2 = the two resistances (Ω)
Derived Terminal potential difference (lost volts = Ir)
SymbolsV = terminal potential difference (V)ε = emf of the cell (V)I = current (A)r = internal resistance (Ω)
Charge and energy (the booklet gives I = Δq/Δt; these are not printed)
SymbolsE = energy transferred (J)V = potential difference (V)I = current (A)t = time (s)P = power (W)q = charge (C)N = number of electrons (no unit)e = elementary charge (constant, C)
Exam tip
Treat an ideal ammeter as zero resistance and an ideal voltmeter as infinite resistance unless the question says otherwise.
C. Wave behaviour
C.1 Simple harmonic motion SL+HL
Derived ω for the two standard oscillators
Symbolsω = angular frequency (rad s−1)k = spring constant (N m−1)m = oscillating mass (kg)g = gravitational field strength (m s−2 or N kg−1)l = length of the pendulum (m)
Maximum acceleration (at the extremes, from a = −ω2x)
Symbolsamax = maximum magnitude of acceleration (m s−2)a = acceleration (m s−2)ω = angular frequency (rad s−1)x = displacement from equilibrium (m)x0 = amplitude (m)
HL Maximum speed (at the equilibrium position)
Symbolsvmax = maximum speed (m s−1)ω = angular frequency (rad s−1)x0 = amplitude (m)
HL Phase difference from a time difference
SymbolsΔϕ = phase difference (rad)Δt = time between corresponding points of the two oscillations (s)T = period (s)
HL Derived Kinetic energy at displacement x (the booklet gives ET and Ep only)
SymbolsEk = kinetic energy (J)m = mass (kg)ω = angular frequency (rad s−1)x0 = amplitude (m)x = displacement from equilibrium (m)
Exam tip
The pendulum period is independent of mass and (for small angles) of amplitude. The spring period is independent of g.
C.2 Wave model SL+HL
Phase difference between two points on a wave
SymbolsΔϕ = phase difference (rad)Δx = separation of the two points along the direction of travel (m)λ = wavelength (m)
Intensity and amplitude
SymbolsI = intensity (W m−2)A = amplitude (m, or unit of the oscillating quantity)
Inverse-square law for a point source
SymbolsI = intensity at distance r (W m−2)P = power emitted by the source (W)r = distance from the source (m)
Common error
Thinking that doubling the amplitude doubles the intensity. It quadruples it.
C.3 Wave phenomena SL+HL
Absolute refractive index
Symbolsn = absolute refractive index of the medium (no unit)c = speed of light in a vacuum (constant, m s−1)v = speed of light in the medium (m s−1)
Critical angle (light going from medium n1 into a less dense medium n2)
Symbolsθc = critical angle (°)n1 = refractive index of the medium the light is in (the denser one) (no unit)n2 = refractive index of the less dense medium (no unit)n = refractive index of the medium, with air taken as 1 (no unit)
HL Grating spacing and highest order visible (N lines per metre)
Symbolsd = grating spacing (distance between adjacent lines) (m)N = number of lines per metre (m−1)nmax = highest order seen, a whole number (no unit)λ = wavelength (m)
HL Single slit: width of the central maximum (screen at distance D)
Symbolsλ = wavelength (m)b = slit width (m)D = distance from slit to screen (m)angular width (rad)linear width (m)
Common error
Forgetting to convert lines per mm into lines per metre before finding d.
C.4 Standing waves and resonance SL+HL
The booklet gives no equations for this topic.
String fixed at both ends, or pipe open at both ends (n = 1, 2, 3, …)
Symbolsλn = wavelength of the nth harmonic (m)L = length of the string or pipe (m)n = harmonic number (no unit)fn = frequency of the nth harmonic (Hz)v = wave speed (m s−1)
Pipe closed at one end (odd harmonics only, n = 1, 2, 3, …)
Symbolsλ = wavelength (m)L = length of the pipe (m)n = counting number; 2n − 1 is the harmonic number (no unit)f = frequency (Hz)v = speed of sound in the air column (m s−1)
Spacings
Symbolsλ = wavelength (m)
Exam tip
Sketch the pattern first (nodes at fixed or closed ends, antinodes at open ends) and read λ off the sketch. This avoids errors in numbering harmonics.
C.5 Doppler effect
SL+HL Derived Reflection from a moving object (radar, ultrasound; v ≪ wave speed c)
SymbolsΔf = difference between emitted and received frequency (Hz)v = speed of the reflector along the line of sight (m s−1)c = wave speed (speed of light for radar, speed of sound for ultrasound) (m s−1)f = emitted frequency (Hz)
HL Source and observer both moving (upper signs when they approach each other)
Symbolsf′ = frequency received by the observer (Hz)f = frequency emitted by the source (Hz)v = speed of the wave in the medium (m s−1)uo = speed of the observer (m s−1)us = speed of the source (m s−1)
Common error
Getting the sign wrong. Check your answer: approaching means a higher received frequency.
D. Fields
D.1 Gravitational fields
SL+HL Orbital radius from the planet’s centre
Symbolsr = orbital radius, measured from the planet’s centre (m)Rplanet = radius of the planet (m)h = height above the surface (m)
SL+HL Derived Circular orbit (gravity provides the centripetal force; the orbital speed itself is printed in the higher level part of the booklet, but the derivation is not)
SymbolsG = gravitational constant (constant, N m2 kg−2)M = mass of the planet (central body) (kg)m = mass of the satellite (kg)r = orbital radius (m)v = orbital speed (m s−1)
SL+HL Derived Kepler’s third law
SymbolsT = orbital period (s)G = gravitational constant (constant, N m2 kg−2)M = mass of the central body (kg)r = orbital radius (m)
HL Derived Energies of a satellite in circular orbit
SymbolsEk = kinetic energy of the satellite (J)Etotal = total (kinetic + potential) energy (J)G = gravitational constant (constant, N m2 kg−2)M = mass of the planet (kg)m = mass of the satellite (kg)r = orbital radius (m)
HL Derived Energy needed to move to a higher circular orbit
SymbolsΔE = energy that must be supplied (J)G = gravitational constant (constant, N m2 kg−2)M = mass of the planet (kg)m = mass of the satellite (kg)r1 = initial orbital radius (m)r2 = final orbital radius (m)
Common error
Using the height above the surface as r. Always measure r from the centre of the planet.
Exam tip
A geostationary satellite has T = 24 h and orbits above the equator.
D.2 Electric and magnetic fields
SL+HL Derived Field of a point charge (from F = kq1q2/r2 and E = F/q)
SymbolsE = electric field strength (N C−1 or V m−1)k = Coulomb constant (constant, N m2 C−2)Q = the point charge creating the field (C)r = distance from the charge (m)
SL+HL Quantisation of charge and the electronvolt
Symbolsq = charge (C)n = number of elementary charges, a whole number (no unit)e = elementary charge (constant, C)eV = electronvolt, a unit of energy
SL+HL Derived Magnetic field of a long straight wire (from the force per unit length between two wires)
SymbolsB = magnetic flux density (T)μ0 = permeability of free space (constant, T m A−1)I = current in the wire (A)r = perpendicular distance from the wire (m)
Exam tip
Field lines meet equipotentials at right angles, and no work is done moving a charge along an equipotential.
D.3 Motion in electromagnetic fields SL+HL
Acceleration of a charge in an electric field (from E = F/q, which is in the booklet)
Symbolsa = acceleration (m s−2)q = charge of the particle (C)E = electric field strength (N C−1 or V m−1)m = mass of the particle (kg)
Acceleration through a potential difference V (from rest)
Symbolsq = charge of the particle (C)V = accelerating potential difference (V)m = mass of the particle (kg)v = final speed (m s−1)
Derived Circular motion in a uniform magnetic field (qvB = mv2/r)
Symbolsr = radius of the circular path (m)m = mass of the particle (kg)v = speed (m s−1)q = charge (C)B = magnetic flux density (T)T = period of the circular motion (s)
Derived Velocity selector (crossed fields, undeflected particle: qE = qvB)
Symbolsv = speed of the particles that pass undeflected (m s−1)E = electric field strength (V m−1)B = magnetic flux density (T)
Exam tip
The magnetic force is always perpendicular to the velocity, so it does no work and the speed stays constant. Between parallel plates, treat the motion like a projectile: constant velocity along the plates, constant acceleration across them.
D.4 Induction HL
Flux linkage
SymbolsN = number of turns (no unit)Φ = magnetic flux through one turn (Wb)flux linkage (Wb)
Coil of N turns, area A, rotating at ω in a uniform field B
Symbolsε = induced emf at time t (V)εmax = peak emf (V)N = number of turns (no unit)B = magnetic flux density (T)A = area of the coil (m2)ω = angular speed of the coil (rad s−1)t = time, from when the coil’s plane is perpendicular to the field (s)
Exam tip
Doubling the rotation speed doubles both the peak emf and the frequency of the output.
Common error
Dropping the minus sign without explanation. State Lenz’s law: the induced current opposes the change in flux that causes it.
E. Nuclear and quantum physics
E.1 Structure of the atom
SL+HL Photon energy from wavelength (the booklet gives E = hf and a value for hc, but not this form)
SymbolsE = photon energy (J)h = Planck constant (constant, J s)c = speed of light in a vacuum (constant, m s−1)λ = wavelength (m)
SL+HL Photon emitted or absorbed in a transition
SymbolsΔE = energy difference between the levels, equal to the photon energy (J or eV)Eupper, Elower = energies of the two levels (J or eV)h = Planck constant (constant, J s)f = photon frequency (Hz)c = speed of light in a vacuum (constant, m s−1)λ = photon wavelength (m)
HL Derived Distance of closest approach (head-on alpha scattering, all Ek becomes Ep)
SymbolsEk = initial kinetic energy of the alpha particle (J)k = Coulomb constant (constant, N m2 C−2)Q = charge of the nucleus (C)q = charge of the alpha particle (C)d = distance of closest approach (m)
HL Derived Hydrogen transition wavelength (from E = −13.6/n2 eV)
Symbolsh = Planck constant (constant, J s)c = speed of light in a vacuum (constant, m s−1)λ = wavelength of the photon (m)ni, nf = initial and final energy levels, whole numbers (no unit)13.6 eV = ionisation energy of hydrogen from the ground state
HL Derived Nuclear density is about the same for all nuclei (from R = R0A1/3)
Symbolsρ = nuclear density (kg m−3)mu = unified atomic mass unit (constant, kg)R0 = nuclear radius constant, about 1.2 × 10−15 m (m)
Common error
Leaving ΔE in eV when using it with h in J s. Convert, or use hc = 1.24 × 10−6 eV m.
E.2 Quantum physics HL
Threshold frequency and stopping potential
Symbolsf0 = threshold frequency (Hz)Φ = work function (J)h = Planck constant (constant, J s)e = elementary charge (constant, C)Vs = stopping potential (V)Emax = maximum kinetic energy of the photoelectrons (J)
Momentum of a photon (the booklet gives the de Broglie relation λ = h/p, not this energy form)
Symbolsp = momentum of the photon (kg m s−1)E = photon energy (J)c = speed of light in a vacuum (constant, m s−1)
Derived de Broglie wavelength from kinetic energy (non-relativistic; second form for a charge accelerated through V)
Symbolsλ = de Broglie wavelength (m)h = Planck constant (constant, J s)m = mass of the particle (kg)Ek = kinetic energy (J)e = charge of the particle (e for an electron or proton) (C)V = accelerating potential difference (V)
Exam tip
Intensity changes the number of photoelectrons, not their maximum kinetic energy. Frequency changes Emax.
E.3 Radioactive decay
SL+HL Mass defect and binding energy
SymbolsΔm = mass defect (kg or u)Z = proton number (no unit)mp = mass of a proton (kg or u)A = nucleon number (no unit)mn = mass of a neutron (kg or u)Mnucleus = mass of the nucleus (kg or u)EB = binding energy (J)c = speed of light in a vacuum (constant, m s−1)
SL+HL Binding energy per nucleon
SymbolsEB = binding energy of the nucleus (J or MeV)A = nucleon number (no unit)
SL+HL Unit shortcut (mass in u, energy in MeV; the booklet lists the energy equivalent of 1 u, this is how to use it)
SymbolsE = energy equivalent (MeV)Δm = mass difference (u)931.5 = energy equivalent of 1 u, in MeV
SL+HL Remaining fraction after n half-lives (n = t / T½)
SymbolsN = number of undecayed nuclei remaining (no unit)N0 = initial number of undecayed nuclei (no unit)n = number of half-lives elapsed (no unit)t = time elapsed (s)T½ = half-life (s)
In every decay or reaction equation, nucleon number A and charge (proton) number Z are each conserved.
HL Mass and count rate decay the same way
Symbolsm = mass of the radioactive isotope remaining (kg)m0 = initial mass (kg)C = count rate (s−1)C0 = initial count rate (s−1)λ = decay constant (s−1)t = time (s)e = base of natural logarithms, ≈ 2.718 (no unit)
HL Linear form for graphs (gradient = −λ)
SymbolsN = number of undecayed nuclei (no unit)N0 = initial number (no unit)λ = decay constant (minus the gradient) (s−1)t = time (s)ln = natural logarithm
Common error
Using atomic mass instead of nuclear mass without accounting for the electrons. Check which one the question gives.
E.4 Fission SL+HL
Energy released in a reaction
SymbolsQ = energy released (J)Σmbefore, Σmafter = total rest mass before and after the reaction (kg)c = speed of light in a vacuum (constant, m s−1)
Power output of a reactor or power station
SymbolsPout = useful (electrical) output power (W)η = overall efficiency (no unit)fissions per second (s−1)energy per fission (J)
E.5 Fusion and stars SL+HL
Derived Comparing two stars (from L = σAT4 with A = 4πR2)
SymbolsL1, L2 = luminosities of the two stars (W)R1, R2 = their radii (m)T1, T2 = their surface temperatures (K)
Derived Radius of a star
SymbolsR = radius of the star (m)L = luminosity (W)σ = Stefan–Boltzmann constant (constant, W m−2 K−4)T = surface temperature (K)
Derived Distance from apparent brightness
Symbolsd = distance to the star (m)L = luminosity (W)b = apparent brightness (W m−2)
Exam tip
In ratio questions the constants cancel. Write the ratio first and substitute last.
Prepared by Evan Kotronis · ExaminerPrep · examinerprep.com