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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

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Every 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

fractional = Δxxpercentage = Δxx × 100%

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)

Δx ≈ xmax − xmin2

SymbolsΔx = absolute uncertainty (same unit as x)xmax, xmin = largest and smallest of the repeated readings (unit of x)

Multiplying by an exact constant

y = kx  ⇒  Δy = |k| Δx

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)

Δm ≈ mmax − mmin2

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

% difference = |xexp − xaccepted|xaccepted × 100%

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).

Asphere = 4πr2

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)

sin θ ≈ tan θ ≈ θ

Symbolsθ = angle (rad)

Arc length and angle

s = rθω = ΔθΔt

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

y = kxn : plot ln y against ln x, gradient = ny = Ae−λx : plot ln y against x, gradient = −λ

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

GraphGradient givesArea under it gives
displacement–timevelocity—
velocity–timeaccelerationdisplacement
acceleration–time—change in velocity
force–timerate of change of momentumimpulse (Δp)
force–extensionspring constant kwork 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)

average speed = distancetimev = ΔsΔta = ΔvΔt

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)

ux = u cos θuy = u sin θax = 0ay = −g

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

T = 2u sin θgH = u2 sin2 θ2gR = u2 sin 2θg

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)

ΣF = 0  ⟺  a = 0

SymbolsΣF = resultant (net) force (N)a = acceleration (m s−2)

Conservation of momentum (isolated system)

m1u1 + m2u2 = m1v1 + m2v2

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)

F∥ = mg sin θF⊥ = mg cos θ

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)

F = mv2r = mω2r

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)

N = m(g + a)

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)

mg = 6πηrvt + ρfVg  ⇒  vt = 2r2g(ρs − ρf)9η

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)

Ek + Ep = constant12mv2 = mgΔh

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

Wnet = ΔEk

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)

P = Et

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)

a = αr

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

Ek = 12mv2 + 12Iω2

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

mgh = 12mv2(1 + Imr2)

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

W = τΔθP = τω

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)

ΣF = 0  and  Στ = 0

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

I1ω1 = I2ω2L = mvr

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)

x = γ(x′ + vt′)t = γ(t′ + vx′c2)

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)

Δx′ = γ(Δx − vΔt)Δt′ = γ(Δt − vΔxc2)

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)

Δt′ = −γv Δxc2

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)

Pt = mcΔTPt = mL

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)

m1c1(T1 − Tf) = m2c2(Tf − T2)

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

PA = σT4

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

I = PA

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)

Imean = S4

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)

(1 − α)S4 = eσT4

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)

n = mM

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)

p1V1 = p2V2 (T const)V1T1 = V2T2 (p const)p1T1 = p2T2 (V const)

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

R = NAkB

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)

vrms = square root of 3RTM = square root of 3kBTmmolecule

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

ProcessConditionFirst law becomes
Isovolumetric (isochoric)W = 0Q = ΔU
Isobaricp constantW = pΔV
IsothermalΔU = 0Q = W, and pV = constant
AdiabaticQ = 0W = −ΔU
Complete cycleΔU = 0Qnet = 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

TV2/3 = constant

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)

QH = W + QCη = 1 − QCQH

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)

ΔS ≥ 0

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

junction: ΣIin = ΣIoutloop: Σε = ΣIR

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

Vout = Vin R2R1 + R2

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)

V = ε − 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)

E = VIt = Ptq = Ne

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

ω2 = km (mass–spring)ω2 = gl (pendulum)

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)

amax = ω2x0

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)

vmax = ωx0

Symbolsvmax = maximum speed (m s−1)ω = angular frequency (rad s−1)x0 = amplitude (m)

HL Phase difference from a time difference

Δϕ = 2π ΔtT

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)

Ek = 12mω2(x02 − x2)

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

Δϕ = 2π Δxλ

SymbolsΔϕ = phase difference (rad)Δx = separation of the two points along the direction of travel (m)λ = wavelength (m)

Intensity and amplitude

I ∝ A2

SymbolsI = intensity (W m−2)A = amplitude (m, or unit of the oscillating quantity)

Inverse-square law for a point source

I = P4πr2

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

n = cv

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)

sin θc = n2n1into air: sin θc = 1n

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)

d = 1Nnmax ≤ dλ (round down)

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)

angular width = 2λblinear width ≈ 2λDb

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, …)

λn = 2Lnfn = nv2L

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, …)

λ = 4L2n − 1f = (2n − 1)v4L

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

node to node = λ2node to adjacent antinode = λ4

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)

Δf ≈ 2vc f

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)

f′ = f v ± uov ∓ us

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

r = Rplanet + h

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)

GMmr2 = mv2r  ⇒  v = square root of GMr

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

T2 = 4π2GM r3

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

Ek = GMm2rEtotal = −GMm2r

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

ΔE = GMm2(1r1 − 1r2)

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)

E = kQr2

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

q = ne1 eV = 1.60 × 10−19 J

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)

B = μ0I2πr

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)

a = qEm

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)

qV = 12mv2

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)

r = mvqBT = 2πmqB

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)

v = EB

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

flux linkage = NΦ

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

ε = NBAω sin ωtεmax = NBAω

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)

E = hcλ

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

ΔE = Eupper − Elower = hf = hcλ

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)

Ek = kQqd

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)

hcλ = 13.6 eV (1nf2 − 1ni2)

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)

ρ ≈ 3mu4πR03

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

f0 = ΦheVs = Emax

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)

p = Ec

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)

λ = hsquare root of 2mEk = hsquare root of 2meV

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

Δm = Zmp + (A − Z)mn − MnucleusEB = Δm c2

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

EBA

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)

E (MeV) = Δm (u) × 931.5

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)

N = N0(12)n

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

m = m0e−λtC = C0e−λt

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)

ln N = ln N0 − λt

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

Q = (Σmbefore − Σmafter)c2

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

Pout = η × (fissions per second) × (energy per fission)

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)

L1L2 = (R1R2)2(T1T2)4

SymbolsL1, L2 = luminosities of the two stars (W)R1, R2 = their radii (m)T1, T2 = their surface temperatures (K)

Derived Radius of a star

R = square root of L4πσT4

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

d = square root of L4πb

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