Physics Ontology

One map of physics, three ways in. Drill down on any quantity to see its units, the equations it lives in, and how its values span the universe.

Browse physics field by field. Each equation is interactive — click any symbol chip to drill into the underlying quantity, its units, and the equations it appears in.

Mechanics

Motion, forces, energy and the dynamics of bodies.

Newtonian dynamics

Newton's Second Law

Newtonian dynamics
F=ma\vec{F} = m\vec{a}

The net force on a body equals its mass times its acceleration.

Isaac Newton

Linear Momentum

Newtonian dynamics
p=mv\vec{p} = m\vec{v}

Momentum is the product of mass and velocity.

Isaac Newton

Impulse

Newtonian dynamics
FΔt=ΔpF\Delta t = \Delta p

Impulse equals change in momentum.

Isaac Newton

Energy

Kinetic Energy

Energy
Ek=12mv2E_k = \tfrac{1}{2} m v^2

The energy a body possesses due to its motion.

James Prescott Joule

Work Done by a Force

Energy
W=FdcosθW = F d \cos\theta

Work equals force times displacement along the force.

James Prescott Joule

Power

Energy
P=WtP = \dfrac{W}{t}

Power is the rate at which work is done.

James Watt

Gravitation

Newton's Law of Gravitation

Gravitation
F=Gm1m2r2F = G\dfrac{m_1 m_2}{r^2}

Every mass attracts every other with a force following an inverse-square law.

Isaac Newton · Henry Cavendish

Gravitational Field (radial)

Gravitation
g=GMr2g = \dfrac{GM}{r^2}

Magnitude of gravitational field strength at distance r from a point mass.

Isaac Newton · Henry Cavendish

Gravitational Potential

Gravitation
V=GMrV = -\dfrac{GM}{r}

Gravitational potential in a radial field (zero at infinity).

Isaac Newton

Fluids & solids

Pressure

Fluids & solids
p=FAp = \dfrac{F}{A}

Pressure is force distributed over an area.

Density

Fluids & solids
ρ=mV\rho = \dfrac{m}{V}

Density is mass per unit volume.

Oscillations

Hooke's Law

Oscillations
F=kxF = -k x

The restoring force of a spring is proportional to extension.

Robert Hooke

SHM Acceleration

Oscillations
a=ω2xa = -\omega^2 x

Acceleration in simple harmonic motion is proportional to displacement.

Robert Hooke

SHM Period (mass–spring)

Oscillations
T=2πmkT = 2\pi\sqrt{\dfrac{m}{k}}

Period of oscillation for a mass on a spring.

Robert Hooke

SHM Period (simple pendulum)

Oscillations
T=2πlgT = 2\pi\sqrt{\dfrac{l}{g}}

Period of a simple pendulum for small oscillations.

Isaac Newton

Rotation

Torque

Rotation
τ=rFsinθ\tau = r F \sin\theta

Torque is the rotational effect of a force about a pivot.

Angular Momentum

Rotation
L=JωL = J \omega

Angular momentum equals moment of inertia times angular velocity.

Kinematics

SUVAT (velocity)

Kinematics
v=u+atv = u + at

Final velocity after uniform acceleration.

Isaac Newton

SUVAT (displacement)

Kinematics
s=ut+12at2s = ut + \tfrac{1}{2}at^2

Displacement under uniform acceleration.

SUVAT (velocity squared)

Kinematics
v2=u2+2asv^2 = u^2 + 2as

Links velocities, acceleration and displacement without time.

Circular motion

Centripetal Acceleration

Circular motion
a=v2r=rω2a = \dfrac{v^2}{r} = r\omega^2

Acceleration directed towards the centre of a circular path.

Centripetal Force

Circular motion
F=mv2r=mrω2F = \dfrac{mv^2}{r} = mr\omega^2

Net force required for circular motion.

Isaac Newton

Materials

Young Modulus

Materials
E=σεE = \dfrac{\sigma}{\varepsilon}

Ratio of tensile stress to tensile strain.

Thomas Young

Tensile Stress

Materials
σ=FA\sigma = \dfrac{F}{A}

Force per unit cross-sectional area.

Thomas Young

Tensile Strain

Materials
ε=Δxx\varepsilon = \dfrac{\Delta x}{x}

Fractional change in length under load.

Thomas Young

Elastic Strain Energy

Materials
ΔEel=12FΔx\Delta E_{el} = \tfrac{1}{2} F \Delta x

Energy stored in a stretched material within the elastic limit.

Robert Hooke

Electromagnetism

Charges, currents, and electric and magnetic fields.

Circuits

Ohm's Law

Circuits
V=IRV = I R

Voltage equals current times resistance.

Georg Ohm

Electrical Power

Circuits
P=VIP = V I

Power dissipated equals voltage times current.

James Prescott Joule

Capacitance

Circuits
C=QVC = \dfrac{Q}{V}

Capacitance is charge stored per unit voltage.

Michael Faraday

Resistivity

Circuits
R=ρlAR = \dfrac{\rho l}{A}

Resistance of a wire depends on resistivity, length and area.

Georg Ohm

Capacitor Energy Stored

Circuits
W=12CV2W = \tfrac{1}{2} C V^2

Energy stored in a charged capacitor.

Michael Faraday

Capacitor Discharge

Circuits
Q=Q0et/RCQ = Q_0 e^{-t/RC}

Exponential decay of charge on a discharging capacitor.

Georg Ohm · Michael Faraday

Electrostatics

Coulomb's Law

Electrostatics
F=14πε0q1q2r2F = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1 q_2}{r^2}

The electrostatic force between two charges follows an inverse-square law.

Charles-Augustin de Coulomb

Electric Field (point charge)

Electrostatics
E=14πε0Qr2E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q}{r^2}

Electric field strength at distance r from a point charge.

Charles-Augustin de Coulomb

Electric Potential (point charge)

Electrostatics
V=14πε0QrV = \dfrac{1}{4\pi\varepsilon_0}\dfrac{Q}{r}

Electric potential at distance r from a point charge.

Charles-Augustin de Coulomb

Fields

Lorentz Force

Fields
F=q(E+v×B)\vec{F} = q(\vec{E} + \vec{v} \times \vec{B})

The force on a charge moving through electric and magnetic fields.

Hendrik Lorentz

Faraday's Law of Induction

Fields
ε=dΦdt\varepsilon = -\dfrac{d\Phi}{dt}

A changing magnetic flux induces an electromotive force.

Michael Faraday · James Clerk Maxwell

Magnetic Flux

Fields
Φ=BAcosθ\Phi = B A \cos\theta

Flux is the magnetic field passing through an area.

Michael Faraday

Magnetic Force on a Wire

Fields
F=BIlsinθF = BIl\sin\theta

Force on a current-carrying conductor in a magnetic field.

André-Marie Ampère · Michael Faraday

AC circuits

RMS Voltage

AC circuits
Vrms=V02V_{\mathrm{rms}} = \dfrac{V_0}{\sqrt{2}}

Root-mean-square voltage of an alternating supply.

Thermodynamics

Heat, temperature, entropy and energy transfer.

Gas laws

Ideal Gas Law

Gas laws
pV=nRTp V = n R T

Relates pressure, volume, amount and temperature of an ideal gas.

Ludwig Boltzmann · Amedeo Avogadro

Ideal Gas Law (Boltzmann form)

Gas laws
pV=NkBTpV = Nk_BT

Ideal gas law in terms of particle number and Boltzmann constant.

Ludwig Boltzmann

Laws

First Law of Thermodynamics

Laws
ΔU=QW\Delta U = Q - W

The change in internal energy equals heat added minus work done.

James Prescott Joule · Sadi Carnot

Entropy Change

Laws
ΔS=QT\Delta S = \dfrac{Q}{T}

Entropy change for a reversible heat transfer.

Ludwig Boltzmann · Sadi Carnot

Statistical mechanics

Boltzmann's Entropy Formula

Statistical mechanics
S=kBlnWS = k_B \ln W

Entropy is proportional to the logarithm of the number of microstates.

Ludwig Boltzmann

Calorimetry

Heat Transfer

Calorimetry
Q=CΔTQ = C \, \Delta T

Heat absorbed equals heat capacity times temperature change.

James Prescott Joule

Specific Heat Capacity

Calorimetry
ΔE=mcΔθ\Delta E = mc\,\Delta\theta

Energy to raise temperature depends on mass and specific heat capacity.

James Prescott Joule

Latent Heat

Calorimetry
ΔE=LΔm\Delta E = L\Delta m

Energy absorbed or released during a change of state.

James Prescott Joule

Kinetic theory

Molecular Kinetic Energy

Kinetic theory
12mc2=32kBT\tfrac{1}{2}m\langle c^2\rangle = \tfrac{3}{2}k_BT

Average translational kinetic energy per molecule of an ideal gas.

Ludwig Boltzmann

Thermal radiation

Stefan–Boltzmann Law

Thermal radiation
L=σAT4L = \sigma A T^4

Power radiated by a black body is proportional to T⁴.

Ludwig Boltzmann · Josef Stefan

Wien's Displacement Law

Thermal radiation
λmaxT=b\lambda_{\max} T = b

Wavelength of peak emission is inversely proportional to temperature.

Wilhelm Wien

Waves

Oscillations and the propagation of disturbances.

Wave basics

Wave Speed Relation

Wave basics
v=fλv = f \lambda

Wave speed equals frequency times wavelength.

Frequency and Period

Wave basics
f=1Tf = \dfrac{1}{T}

Frequency is the reciprocal of the period.

Intensity

Wave basics
I=PAI = \dfrac{P}{A}

Intensity is power per unit area.

Optics

The behaviour and properties of light.

Refraction

Snell's Law

Refraction
n1sinθ1=n2sinθ2n_1 \sin\theta_1 = n_2 \sin\theta_2

Describes how light bends when passing between media of different index.

Critical Angle

Refraction
sinC=1n\sin C = \dfrac{1}{n}

Critical angle for total internal reflection in an optically denser medium.

Diffraction

Diffraction Grating

Diffraction
nλ=dsinθn\lambda = d\sin\theta

Condition for constructive interference from a diffraction grating.

Thomas Young

Lenses

Thin Lens Equation

Lenses
1u+1v=1f\dfrac{1}{u} + \dfrac{1}{v} = \dfrac{1}{f}

Relates object distance, image distance and focal length.

Quantum

Physics at the smallest scales, where action is quantised.

Quantisation

Planck–Einstein Relation

Quantisation
E=hfE = h f

The energy of a photon is proportional to its frequency.

Max Planck · Albert Einstein

Photoelectric Effect

Quantisation
Ek=hfϕE_k = h f - \phi

The kinetic energy of emitted electrons depends on photon frequency.

Albert Einstein · Robert Millikan

Wave–particle duality

de Broglie Wavelength

Wave–particle duality
λ=hp\lambda = \dfrac{h}{p}

Matter has a wavelength inversely proportional to momentum.

Louis de Broglie

Nuclear decay

Radioactive Decay

Nuclear decay
N=N0eλtN = N_0 e^{-\lambda t}

Number of undecayed nuclei decreases exponentially with time.

Ernest Rutherford

Activity

Nuclear decay
A=λNA = \lambda N

Activity is the product of decay constant and number of nuclei.

Ernest Rutherford

Half-life and Decay Constant

Nuclear decay
λ=ln2t1/2\lambda = \dfrac{\ln 2}{t_{1/2}}

Links decay constant to half-life.

Ernest Rutherford

Relativity

Space, time and gravity at high speeds and large scales.

Special relativity

Mass–Energy Equivalence

Special relativity
E=mc2E = m c^2

Mass and energy are equivalent and interconvertible.

Albert Einstein

Lorentz Factor

Special relativity
γ=11v2/c2\gamma = \dfrac{1}{\sqrt{1 - v^2/c^2}}

Quantifies time dilation and length contraction at speed v.

Albert Einstein · Hendrik Lorentz

Cosmology

Hubble's Law

Cosmology
v=H0dv = H_0 d

Recession velocity of a galaxy is proportional to its distance.

Edwin Hubble