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ExaminerPrep · Formula handout · IB Physics SL

Equations Not in the Data Booklet: SL edition

For IB Diploma Physics SL (syllabus first assessed 2025), 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.

SL edition

This sheet contains only what Physics SL students need. The Additional Higher Level topics (A.4, A.5, B.4, D.4, E.2) and the HL-only equations inside other topics are left out.

Taking HL? Use the HL edition, which has everything here plus the HL equations.

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.

  • 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 Doppler shift for light; the energy equivalent of the atomic mass unit and the value of hc.

Tools: uncertainties, maths and graphs

Uncertainties

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

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)

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

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
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

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

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

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.

B. The particulate nature of matter

B.1 Thermal energy transfers

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

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

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.5 Current and circuits

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

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)

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

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

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)

C.4 Standing waves and resonance

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

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)

Common error

Getting the sign wrong. Check your answer: approaching means a higher received frequency.

D. Fields

D.1 Gravitational fields

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)

Derived Circular orbit (gravity provides the centripetal force; this is the first step towards Kepler’s third law)

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)

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)

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

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)

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

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 show the direction of the force on a positive test charge, and closer lines mean a stronger field. Square the distance: doubling r divides E by four.

D.3 Motion in electromagnetic fields

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.

E. Nuclear and quantum physics

E.1 Structure of the atom

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)

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)

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.3 Radioactive decay

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)

Binding energy per nucleon

EBA

SymbolsEB = binding energy of the nucleus (J or MeV)A = nucleon number (no unit)

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

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.

Common error

Using atomic mass instead of nuclear mass without accounting for the electrons. Check which one the question gives.

E.4 Fission

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

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