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IB Physics Formula Booklet: Equations Explained by Theme

Physics formula sheetsIB DiplomaSL and HLUpdated 1 Nov 2026

b=L4πd2b = \frac{L}{4\pi d^2}
where
  • b apparent brightness (intensity received) W/m²
  • L luminosity, total power emitted W
  • d distance from the source m

This IB physics formula booklet guide explains the equations of the IB Diploma physics course theme by theme, using the inverse square law for brightness, b=L4πd2b = \frac{L}{4\pi d^2}, as an example of how one short line links energy, waves and astrophysics. The IB supplies its own physics data booklet for the exams; this page is a separate study aid that says what each equation means, when it applies and which unit each symbol takes.

The current course is organised into five themes: space, time and motion; the particulate nature of matter; wave behaviour; fields; and nuclear and quantum physics. Some subtopics are for Higher Level only, so check your syllabus to see which apply to you. IB symbols are close to the ones Indian students use: s for displacement, u and v for initial and final velocity. Other course guides are on the formula sheets hub.

Quick facts

  • What this is

    A study guide, not the IB data booklet
  • Themes

    A space, time, motion; B matter; C waves; D fields; E nuclear and quantum
  • Symbols

    s, u, v, a, t for motion
  • First law

    Q = ΔU + W, with W done by the gas
  • Levels

    SL and HL, with extra HL subtopics
  • Example equation

    b=L4πd2b = \frac{L}{4\pi d^2}

Theme A: space, time and motion

Kinematics, forces, energy and momentum
EquationIn wordsUnitTopic page
s=(u+v)t2s = \frac{(u + v)t}{2}displacement is average velocity times timemDisplacement topic
v=u+at, s=ut+12at2v = u + at,\ s = ut + \frac{1}{2}at^2uniform accelerationm/s, mMotion topic
F=ma=ΔpΔtF = ma = \frac{\Delta p}{\Delta t}resultant force and momentum changeNForce topic
Ek=p22mE_k = \frac{p^2}{2m}kinetic energy written with momentumJKinetic energy topic
ΔEp=mg Δh\Delta E_p = mg\,\Delta hchange in gravitational potential energyJPotential energy topic
P=FvP = Fvpower delivered by a force at speed vWWork and energy topic
τ=Frsin⁡θ, L=Iω\tau = Fr\sin\theta,\ L = I\omegatorque and angular momentum (HL)N m, kg m²/sTorque topic

The relativity subtopic uses γ=(1−v2/c2)−1/2\gamma = (1 - v^2/c^2)^{-1/2} for time dilation and length contraction; see the relativity formula page.

Theme B: the particulate nature of matter

Thermal physics, gases and circuits
EquationIn wordsUnitTopic page
Q=mc ΔT, Q=mLQ = mc\,\Delta T,\ Q = mLwarming a sample, then melting or boiling itJHeat topic
L=σAT4L = \sigma AT^4luminosity of a black body (Stefan Boltzmann)WHeat transfer topic
pV=nRT=NkBTpV = nRT = Nk_BTideal gas equationJThermodynamics topic
Eˉk=1.5 kBT\bar{E}_k = 1.5\,k_BTaverage translational energy per particleJEnergy topic
Q=ΔU+WQ = \Delta U + Wenergy balance for a gas that does work W (HL)JFirst law topic
V=IR, P=VIV = IR,\ P = VIcircuit basicsV, WOhm's law topic
ε=I(R+r)\varepsilon = I(R + r)cell with internal resistanceVEMF topic

Example 1: brightness of a star

A star of luminosity 3.8 × 10²⁶ W is 1.5 × 10¹¹ m away. Find its apparent brightness.

b=3.8×10264π(1.5×1011)2=3.8×10262.83×1023=1.3×103 W/m2b = \frac{3.8 \times 10^{26}}{4\pi(1.5 \times 10^{11})^2} = \frac{3.8 \times 10^{26}}{2.83 \times 10^{23}} = 1.3 \times 10^{3}\ \text{W/m}^2.

Answer: about 1.3 × 10³ W/m², roughly the intensity of sunlight above the atmosphere of our planet.

Theme C: wave behaviour

Oscillations and waves
EquationIn wordsUnitTopic page
T=1fT = \frac{1}{f}period and frequencysPeriod topic
a=−ω2xa = -\omega^2 xdefining condition for simple harmonic motionm/s²Amplitude topic
v=fλv = f\lambdawave equationm/sWave velocity topic
n1sin⁡θ1=n2sin⁡θ2n_1\sin\theta_1 = n_2\sin\theta_2bending of light at a boundaryno unitRefraction topic
s=λDds = \frac{\lambda D}{d}fringe spacing for two slitsmWavelength topic
Δff≈vc\frac{\Delta f}{f} \approx \frac{v}{c}Doppler shift for light at low speedno unitFrequency topic
IB writes s for fringe spacing. Do not confuse it with displacement in theme A.

Theme D: fields

Gravitational, electric and magnetic fields
EquationIn wordsUnitTopic page
F=Gm1m2r2, g=GMr2F = G\frac{m_1m_2}{r^2},\ g = \frac{GM}{r^2}gravitational force and field strengthN, N/kgGravitation topic
v=GMrv = \sqrt{\frac{GM}{r}}how fast a satellite circles at radius rm/sOrbital velocity topic
F=kq1q2r2, E=FqF = k\frac{q_1q_2}{r^2},\ E = \frac{F}{q}electric force and fieldN, N/CElectric field topic
F=qvBsin⁡θ, F=BILsin⁡θF = qvB\sin\theta,\ F = BIL\sin\thetamagnetic force on a charge and on a wireNMagnetic force topic
Φ=BAcos⁡θ, ε=−NΔΦΔt\Phi = BA\cos\theta,\ \varepsilon = -N\frac{\Delta\Phi}{\Delta t}flux and induced emf (HL)Wb, VMagnetic flux topic

Example 2: a satellite in low orbit

A satellite circles 600 km above the ground. Find its orbital speed and period. Take M = 5.97 × 10²⁴ kg for the Earth, whose radius is 6.37 × 10⁶ m.

Orbit radius: r = 6.37 × 10⁶ + 6.0 × 10⁵ = 6.97 × 10⁶ m.

v=(6.674×10−11)(5.97×1024)6.97×106=5.72×107=7.56×103 m/sv = \sqrt{\frac{(6.674 \times 10^{-11})(5.97 \times 10^{24})}{6.97 \times 10^{6}}} = \sqrt{5.72 \times 10^{7}} = 7.56 \times 10^{3}\ \text{m/s}.

T=2πrv=2π(6.97×106)7.56×103=5.79×103 sT = \frac{2\pi r}{v} = \frac{2\pi(6.97 \times 10^6)}{7.56 \times 10^3} = 5.79 \times 10^{3}\ \text{s}, about 97 minutes.

Theme E: nuclear and quantum physics

Atoms, nuclei and photons
EquationIn wordsUnitTopic page
E=hfE = hfphoton energyJPhotons topic
Emax=hf−ΦE_{max} = hf - \Phiphotoelectric effect (HL)JWork function topic
λ=hp\lambda = \frac{h}{p}de Broglie wavelength (HL)mMatter waves topic
E=mc2E = mc^2mass defect and binding energyJMass energy topic
N=N0e−λt, T1/2=ln⁡2λN = N_0e^{-\lambda t},\ T_{1/2} = \frac{\ln 2}{\lambda}radioactive decay (decay law at HL)sNuclear physics topic

The stars subtopic ties back to theme B: luminosity from L=σAT4L = \sigma AT^4 and peak wavelength from Wien's law, λmaxT=2.9×10−3 m K\lambda_{max}T = 2.9 \times 10^{-3}\ \text{m K}.

Using the IB physics formula booklet in practice

  • Know where each line lives. In timed papers you lose minutes searching. Practise with the official booklet from the start of the course.
  • Learn what is not listed. Definitions, such as what a field strength or a half life means, and unit conversions are rarely given.
  • Watch the symbols. s, Φ and λ each have more than one meaning in different themes.
  • Show working in the internal assessment. Uncertainty propagation follows the same rules as error analysis in other courses.

To compare with other courses, see the AP Physics 1 formula sheet or the Class 12 physics sheet.

Frequently asked questions

Is this the official IB physics data booklet?

No. It is a study guide written for this site. The IB provides its own data booklet for exams, so download the current version and practise with it.

What is in the physics formula booklet IB students use?

In general it contains fundamental constants, unit prefixes and the equations of each theme, grouped by topic. It does not explain the equations or list every definition.

Do SL and HL students use the same formula booklet?

Usually one booklet covers both, with HL only equations marked or grouped separately. Check the version for your exam session.

How is IB physics different from AP physics?

IB is a two year course organised into themes with SL and HL options, while AP splits physics into separate courses. Much of the core physics and many equations are the same.