Chapter Zero — Introduction

A living archive of fifty moving equations — from fluid dynamics to fields and quanta — each explained, simulated, and ready to solve.

Chapter Zero — Introduction


A short introduction to fluid dynamics — what it is, the ideas that carry it, and how to read the fifty moving figures below.

Fluid dynamics is the study of how liquids and gases move, and of the forces that make them move. It is one continuous story told in many dialects: pressure and viscosity in a pipe, buoyancy in an ocean, shock waves in air, surface tension in a single droplet. This archive walks that story one figure at a time — each with a live simulation, a tuneable parameter, a practice problem and a tutorial.

56 Figures8 Genres56 Problems56 Tutorials
Six ideas that carry the whole subject
01

What a fluid is

Anything that keeps deforming under shear — water, air, honey, magma, even crowds. Fluids have no fixed shape, only a history of motion.

02

Conservation first

Every equation here descends from three bookkeeping rules: mass, momentum and energy are never created, only moved around.

03

Viscosity vs inertia

Thick, slow flows are ruled by friction; fast, thin flows are ruled by momentum. The Reynolds number is the referee between them.

04

Laminar to turbulent

Push a flow hard enough and neat layers break into eddies. Turbulence is deterministic, yet practically unpredictable.

05

Boundaries matter

At a solid wall the fluid sticks. That thin boundary layer decides drag, lift, mixing and most of engineering.

06

Dimensionless thinking

Re, Fr, Ma, We, Pr — ratios that let a bathtub vortex and a hurricane share one equation.

Symbol glossary — 65 symbols, their meaning and their function
Operators
Partial derivative
Rate of change of a quantity with one variable, holding the others fixed.Function: Builds the local time and space terms, e.g. ∂v/∂t is acceleration at a fixed point.
d
Total derivative
Change of a quantity with respect to a single independent variable.Function: Used for one-variable relations such as df/dc in phase-separation energy.
D/Dt
Material derivative
Rate of change following a fluid parcel as it drifts along.Function: Combines local change and advection: D/Dt = ∂/∂t + v · ∇.
Nabla / gradient
Direction and steepness of the fastest increase of a field.Function: ∇p turns a pressure map into the force that pushes fluid downhill.
∇ ·
Divergence
Net outflow of a vector field from a point.Function: ∇ · v = 0 is the incompressibility condition — nothing is created or lost.
∇ ×
Curl
Local spinning of a vector field.Function: Generates vorticity ω = ∇ × v, the raw material of eddies.
∇²
Laplacian
How much a value at a point differs from its surroundings.Function: The diffusion term — smooths velocity, heat and concentration over time.
Δ
Delta (difference)
A finite change or drop between two states.Function: Δp is the pressure difference that drives flow through a pipe.
Square root
The inverse of squaring.Function: Appears whenever energy converts to speed, as in v = √(2gh).
Integral
Accumulated total over a length, area or volume.Function: Sums local contributions into net force, flux or circulation.
| |
Magnitude
Size of a vector or complex quantity, ignoring direction.Function: |ψ|² gives the local density of a quantum fluid.
Fluid properties
ρ
Rho — density
Mass contained in a unit volume of fluid.Function: Sets inertia: the heavier the fluid, the harder it is to accelerate.
μ
Mu — dynamic viscosity
Internal friction resisting shear between fluid layers.Function: Multiplies ∇²v to damp motion and create the boundary layer.
ν
Nu — kinematic viscosity
Viscosity per unit density, ν = μ/ρ.Function: Acts as the diffusion rate of momentum through the fluid.
γ, σ
Surface tension
Energy stored in a fluid interface per unit area.Function: Pulls droplets spherical and lifts liquid up narrow tubes.
α
Alpha — thermal diffusivity
How quickly heat spreads through a material.Function: Controls the speed of the heat equation ∂u/∂t = α∇²u.
β
Beta — thermal expansion
Fractional volume change per degree of heating.Function: Converts a temperature difference into buoyancy for convection.
k
Conductivity / permeability
Ease of transporting heat, or of letting fluid through a porous solid.Function: Scales heat flux, and sets flow rate in Darcy's law.
c_p
Specific heat
Energy needed to raise one unit of mass by one degree.Function: Links thermal energy to temperature in the Prandtl number.
M
Mobility
How readily a component migrates under a chemical gradient.Function: Sets the coarsening speed in the Cahn-Hilliard equation.
Flow variables
v, u
Velocity
Speed and direction of the fluid at each point.Function: The unknown most equations solve for — the flow field itself.
p
Pressure
Normal force per unit area inside the fluid.Function: Its gradient pushes fluid from high to low pressure.
ω
Omega — vorticity
Local rate of rotation of fluid parcels.Function: Tracks the birth, stretching and decay of vortices.
Ω
Angular velocity
Rotation rate of a boundary such as a spinning cylinder.Function: Drives Taylor-Couette vortices between rotating walls.
ψ
Psi — stream function
A scalar whose contours are the streamlines of the flow.Function: Guarantees incompressibility: u = ∂ψ/∂y, v = −∂ψ/∂x.
φ
Phi — potential
A scalar field whose gradient gives velocity or force.Function: Solves ∇²φ = 0 for ideal, irrotational flow.
Γ
Gamma — circulation
Total swirl integrated around a closed loop.Function: Sets aerodynamic lift through L = ρVΓ.
Q
Volumetric flow rate
Volume of fluid passing a section per second.Function: Connects pipe geometry to pressure drop in Hagen-Poiseuille.
q
Flux (specific discharge)
Flow per unit area through a surface.Function: The output of Darcy's law in groundwater flow.
c
Concentration / wave speed
Amount of a solute, or the speed a wave travels.Function: Diffuses in transport equations; sets c² in the wave equation.
T
Temperature
Thermal state of the fluid.Function: Gradients in T create buoyancy, convection and Marangoni flow.
τ
Tau — shear stress
Tangential force per unit area between layers.Function: The friction the wall exerts on the passing fluid.
F, f
Force / body force
External push per unit volume, such as gravity.Function: The source term added to the momentum balance.
Geometry & time
t
Time
The evolution variable.Function: Everything with ∂/∂t is an unsteady, time-marching term.
x, y, z
Coordinates
Position in space.Function: Directions along which gradients and derivatives are taken.
r, R
Radius
Distance from an axis, or the size of a pipe, bubble or sphere.Function: Shapes parabolic pipe profiles and droplet curvature.
L
Characteristic length
The size that matters for the problem at hand.Function: The yardstick inside every dimensionless number.
h
Height / depth / gap
Vertical extent of fluid or spacing between plates.Function: Converts potential energy into pressure and outflow speed.
A
Area
Cross-section the fluid passes through.Function: Ties velocity to flow rate: Q = vA.
δ
Delta — boundary layer
Thickness of the slowed layer next to a wall.Function: Grows as √(νx/U) along a flat plate.
λ
Lambda — wavelength
Spatial period of a wave or instability finger.Function: Selects which disturbance grows fastest.
k (wave)
Wavenumber
Number of wave cycles per unit length, 2π/λ.Function: Sets growth rates in Kelvin-Helmholtz and Rayleigh-Taylor.
g
Gravity
Acceleration due to gravity, ≈ 9.81 m/s².Function: Drives buoyancy, hydrostatics and free-surface waves.
n
Manning roughness
How rough an open channel bed is.Function: Slows the average velocity in open-channel flow.
S
Slope
Fall of a channel per unit length.Function: Supplies the gravitational driving force in Manning's equation.
Dimensionless numbers
Re
Reynolds number
Inertia divided by viscous force, ρuL/μ.Function: Predicts laminar (low) versus turbulent (high) flow.
Fr
Froude number
Inertia divided by gravity, u/√(gL).Function: Separates tranquil subcritical from rapid supercritical flow.
Ma, M
Mach number
Flow speed divided by the speed of sound.Function: Above 1 the flow is supersonic and forms shock cones.
We
Weber number
Inertia divided by surface tension.Function: Decides whether a droplet holds together or shatters.
Pr
Prandtl number
Momentum diffusivity over thermal diffusivity, ν/α.Function: Says whether the velocity or thermal boundary layer is thicker.
Gr
Grashof number
Buoyancy divided by viscous force.Function: Measures the strength of natural convection plumes.
Ra
Rayleigh number
Product of Grashof and Prandtl numbers.Function: Past 1708 a heated layer breaks into convection cells.
Ta
Taylor number
Rotational inertia versus viscous damping.Function: Predicts the onset of Taylor vortices between cylinders.
Ca
Capillary number
Viscous force divided by surface tension.Function: Controls finger width in viscous fingering.
Kn
Knudsen number
Molecular mean free path over system size.Function: Above ~0.01 the no-slip wall condition starts to fail.
f_D
Darcy friction factor
Dimensionless pipe friction coefficient.Function: Converts pipe length and roughness into head loss.
C_L
Lift coefficient
Normalised lift produced by a shape.Function: Scales lift with ½ρv²A.
Constants & notation
π
Pi
Ratio of circumference to diameter, ≈ 3.14159.Function: Appears wherever the geometry is round.
e
Euler's number
Base of natural growth and decay, ≈ 2.71828.Function: Describes exponential decay of vortices and spirals.
i
Imaginary unit
√(−1).Function: Encodes oscillation and phase in stability analysis.
Reduced Planck constant
Quantum of action divided by 2π.Function: Sets the scale of quantum fluid behaviour.
Infinity
Far field, away from any boundary.Function: Subscript ∞ marks ambient conditions, as in p_∞.
₀, ₁, ₂
Subscript indices
Labels for states or fluids: initial, upstream, downstream.Function: Let one equation compare two points or two fluids.
ẋ, ẍ
Dot notation
First and second time derivatives.Function: Compact form for bubble wall speed Ṙ and acceleration R̈.
|_w
Evaluated at
The quantity measured at a specific place, here the wall.Function: Pins a gradient to the boundary, as in (∂u/∂y)|_w.
How to use this archive
  1. 01Search or filter by genre to find the flow you care about.
  2. 02Drag the parameter slider and watch the simulation respond in real time.
  3. 03Open the problem, write or upload your answer, then unlock the solution.
  4. 04Stuck? Tap the tiny ? dot for nudges, or open the tutorial video.
Principia56 Figures
Fluid Dynamics Archive


Fifty equations of flow, each rendered live and tuneable in real time. Drag a parameter, watch the fluid answer. Bring headphones.

Made by tonkao
Scroll to begin ↓Est. 2026
What's inside

Browse the archive

  • 56Interactive figures
  • 8Genres
  • 27Fluid flow
  • 9Wave functions
  • 10Vortices & turbulence
  • 9Heat & thermodynamics
  • 14Pressure & surface
  • 8Dimensionless numbers

Showing 56 of 56 figures

Use the Sections (1–56) button, bottom left, to jump to any equation.

Figure 01Fluid MechanicsFlow & Motion

Describes the motion of viscous fluid substances, balancing momentum, pressure, and viscous shear forces.

ρ (∂v∂t + v · ∇v) = −∇p + μ ∇²v + f
Viscosity (μ)0.5
Scroll down ↓Interactive simulation
Figure 02ConservationFlow & Motion

States that mass is conserved in a flow system. For an incompressible fluid, the divergence of velocity is strictly zero.

∂ρ∂t + ∇ · (ρv) = 0
Compression Ratio0
Scroll down ↓Interactive simulation
Figure 03Energy BalancePressure & Statics

An increase in the speed of a fluid occurs simultaneously with a decrease in static pressure or fluid potential energy.

p + ½ ρv² + ρgh = const
Flow Velocity2
Scroll down ↓Interactive simulation
Figure 04HydrostaticsPressure & Statics

The upward buoyant force exerted on a body immersed in a fluid is equal to the weight of the fluid that the body displaces.

F_b = ρ_f V_d g
Fluid Density1
Scroll down ↓Interactive simulation
Figure 05Pipe FlowFlow & Motion

Laminar flow of a Newtonian fluid in a cylindrical pipe creates a perfectly parabolic velocity distribution.

v(r) = Δp(4μL) (R² − r²)
Pressure Gradient5
Scroll down ↓Interactive simulation
Figure 06MicrofluidicsPressure & Statics

Describes the frictional force exerted on spherical objects with very small Reynolds numbers in a viscous fluid.

F_d = 6π μ R v
Particle Radius5
Scroll down ↓Interactive simulation
Figure 07Open ChannelsFlow & Motion

A dimensionless number comparing inertial and gravitational forces, determining if flow is subcritical or supercritical.

Fr = u√(gL)
Flow Speed (u)1.5
Scroll down ↓Interactive simulation
Figure 08Dimensionless NumbersAero & Gas Dynamics

Predicts flow patterns in different fluid situations. Low values indicate laminar flow; high values indicate turbulence.

Re = ρuLμ
Inertial Factor2000
Scroll down ↓Interactive simulation
Figure 09Compressible FlowAero & Gas Dynamics

When an object moves faster than the speed of sound in a fluid, it generates a conical shock wave boundary.

sin(μ) = cv = 1M
Mach Number (M)2
Scroll down ↓Interactive simulation
Figure 10HydrodynamicsFlow & Motion

The speed of fluid flowing out of an opening under gravity is the same as if it dropped from the same height in free fall.

v = √(2gh)
Fluid Height (h)50
Scroll down ↓Interactive simulation
Figure 11Shear FlowFlow & Motion

The laminar flow of a viscous fluid in the space between two parallel plates, one of which is moving relative to the other.

u(y) = U yh
Top Plate Velocity2.5
Scroll down ↓Interactive simulation
Figure 12InstabilitiesInstability & Turbulence

Occurs when there is velocity shear in a single continuous fluid, or a velocity difference across the interface of two fluids.

ω = k (ρ₁U₁ + ρ₂U₂)(ρ₁ + ρ₂) ± ik …
Shear Velocity1.5
Scroll down ↓Interactive simulation
Figure 13Density CurrentsInstability & Turbulence

An instability at an interface between two fluids of different densities which occurs when the lighter fluid pushes the heavier fluid.

γ = √( kg (ρ₂ − ρ₁)(ρ₂ + ρ₁) )
Density Ratio2
Scroll down ↓Interactive simulation
Figure 14Surface TensionPressure & Statics

The ability of a liquid to flow in narrow spaces without the assistance of, or even in opposition to, external forces like gravity.

h = 2γ cos θ(ρgr)
Tube Radius (r)0.5
Scroll down ↓Interactive simulation
Figure 15TransientsWaves & Oscillation

A pressure surge or wave caused when a fluid in motion is forced to stop or change direction suddenly.

ΔP = ρ c Δv
Valve Closure Speed5
Scroll down ↓Interactive simulation
Figure 16AerodynamicsAero & Gas Dynamics

The observable phenomenon that is commonly associated with a spinning object moving through a fluid. The path curves due to pressure differences.

F_L = ½ ρv² A C_L
Spin Rate5
Scroll down ↓Interactive simulation
Figure 17Pressure GradientsPressure & Statics

The reduction in fluid pressure that results when a fluid flows through a constricted section of a pipe.

p₁ − p₂ = (ρ2) (v₂² − v₁²)
Constriction Width20
Scroll down ↓Interactive simulation
Figure 18Viscous BoundaryFlow & Motion

The steady 2D laminar boundary layer that forms on a semi-infinite plate held parallel to a constant velocity flow.

δ = 5.0 √(νxU)
Distance (x)100
Scroll down ↓Interactive simulation
Figure 19Friction LossFlow & Motion

An empirical equation that relates the head loss due to friction along a given length of pipe to the average velocity of the fluid.

Δp = f_D (LD) (ρv²2)
Friction Factor0.05
Scroll down ↓Interactive simulation
Figure 20HydrologyFlow & Motion

Estimates the average velocity of a liquid flowing in a conduit that does not completely enclose the liquid (open channel).

v = (1n) R_h^(23) S^(12)
Channel Slope (S)0.01
Scroll down ↓Interactive simulation
Figure 21Fluid StaticsPressure & Statics

A pressure change occurring anywhere in a confined incompressible fluid is transmitted throughout the fluid such that the same change occurs everywhere.

Δp = ρ g Δh
Applied Force50
Scroll down ↓Interactive simulation
Figure 22Interface PhysicsPressure & Statics

Describes the capillary pressure difference sustained across the interface between two static fluids due to surface tension.

Δp = γ ( 1R₁ + 1R₂ )
Droplet Radius25
Scroll down ↓Interactive simulation
Figure 23OceanographyWaves & Oscillation

A set of hyperbolic partial differential equations that describe the flow below a pressure surface in a fluid.

∂h∂t + ∂(hu)∂x = 0
Wave Amplitude5
Scroll down ↓Interactive simulation
Figure 24Inviscid FlowFlow & Motion

A set of quasilinear hyperbolic equations governing adiabatic and inviscid flow. They represent conservation of mass, momentum, and energy.

∂v∂t + (v · ∇)v = −(1ρ) ∇p
Grid Resolution20
Scroll down ↓Interactive simulation
Figure 25Rotational DynamicsInstability & Turbulence

Fluid flow in the gap between two rotating cylinders. At specific speeds, toroidal Taylor vortices form.

Ta = r_i (r_o − r_i)³ Ω_i²ν²
Inner Rotation2
Scroll down ↓Interactive simulation
Figure 26TurbulenceInstability & Turbulence

Describes the evolution of the curl of the velocity field. Vortices stretch, tilt, and diffuse over time.

Dt = (ω · ∇)v + ν ∇²ω
Vortex Strength5
Scroll down ↓Interactive simulation
Figure 27AeronauticsAero & Gas Dynamics

A fundamental theorem that relates the lift generated by an airfoil to the speed of the fluid and the circulation around the body.

L = ρ V Γ
Circulation (Γ)5
Scroll down ↓Interactive simulation
Figure 28Volumetric FlowFlow & Motion

Calculates the pressure drop in an incompressible and Newtonian fluid in laminar flow flowing through a long cylindrical pipe.

Δp = 8π μ L Q
Volumetric Rate (Q)10
Scroll down ↓Interactive simulation
Figure 29Potential FlowFlow & Motion

In 2D incompressible flows, the stream function contours represent fluid streamlines, and its gradient gives velocity components.

u = ∂ψ∂y, v = −∂ψ∂x
Dipole Strength50
Scroll down ↓Interactive simulation
Figure 30Spray DynamicsFlow & Motion

A dimensionless number used to analyze fluid flows where there is an interface between two different fluids, especially for droplet formation.

We = ρv² lσ
Impact Velocity5
Scroll down ↓Interactive simulation
Figure 31Heat TransferHeat & Thermodynamics

The ratio of momentum diffusivity (kinematic viscosity) to thermal diffusivity. Defines boundary layer dominance.

Pr = να = c_p μk
Thermal Diffusivity0.7
Scroll down ↓Interactive simulation
Figure 32Natural ConvectionHeat & Thermodynamics

Approximates the ratio of the buoyancy to viscous force acting on a fluid. Drives thermal plume mechanics.

Gr = g β (T_s − T_∞) L³ν²
Temp Gradient50
Scroll down ↓Interactive simulation
Figure 33Phase ChangeHeat & Thermodynamics

An ordinary differential equation governing the dynamics of a spherical cavitation bubble in an infinite body of liquid.

R R̈ + (32) Ṙ² = (p_B − p_∞)ρ
External Pressure1
Scroll down ↓Interactive simulation
Figure 34GeophysicsPlanetary & Quantum

A structure of currents or winds near a horizontal boundary in which the flow direction rotates as one moves away from the boundary.

u + iv = V₀ e^((1+i)πzD)
Coriolis Force5
Scroll down ↓Interactive simulation
Figure 35Porous MediaFlow & Motion

Viscous fingering occurs when a less viscous fluid is injected into a porous medium displacing a more viscous fluid.

λ = b√(Ca)
Injection Pressure2.4
Scroll down ↓Interactive simulation
Figure 36Linear StabilityInstability & Turbulence

An eigenvalue equation describing the linear two-dimensional modes of disturbance superimposed on a viscous parallel flow.

(U − c)(φ″ − α²φ) − U″φ = …
Wavenumber (α)1
Scroll down ↓Interactive simulation
Figure 37Rarefied GasAero & Gas Dynamics

When the mean free path of molecules approaches the physical scale of the system, the no-slip boundary condition fails.

u_s = ((2 − σ_v)σ_v) λ (∂u∂y)|_w
Knudsen Number0.1
Scroll down ↓Interactive simulation
Figure 38Mass TransferHeat & Thermodynamics

Mass transfer along an interface between two fluids due to a gradient of the surface tension (e.g. tears of wine).

τ = (∂γ∂T) ∇T + (∂γ∂c) ∇c
Solute Gradient5
Scroll down ↓Interactive simulation
Figure 39Shock DynamicsWaves & Oscillation

The jump conditions across a shock wave in a compressible 1D flow, conserving mass, momentum, and energy.

ρ₁u₁ = ρ₂u₂
Upstream Velocity3
Scroll down ↓Interactive simulation
Figure 40HydrogeologyFlow & Motion

Describes the flow of a fluid through a porous medium, foundational to groundwater flow and petroleum engineering.

q = −(kμ) ∇p
Permeability (k)50
Scroll down ↓Interactive simulation
Figure 41Thermal DynamicsHeat & Thermodynamics

A parabolic partial differential equation that describes the distribution of heat (or variation in temperature) in a given region over time.

∂u∂t = α ∇²u
Thermal Diffusion (α)2
Scroll down ↓Interactive simulation
Figure 42OscillationWaves & Oscillation

A second-order linear partial differential equation for the description of waves, such as sound waves, light waves, or water waves.

∂²u∂t² = c² ∇²u
Wave Speed (c)5
Scroll down ↓Interactive simulation
Figure 43Non-linear PhysicsWaves & Oscillation

A fundamental partial differential equation from fluid mechanics, exhibiting shock wave formation and dissipation.

∂u∂t + u ∂u∂x = ν ∂²u∂x²
Viscous Damping0.5
Scroll down ↓Interactive simulation
Figure 44Phase SeparationInstability & Turbulence

Describes the process of phase separation, by which two components of a binary fluid spontaneously separate and form pure domains.

∂c∂t = ∇ · ( M ∇ ( dfdc − K ∇²c ) )
Mobility Factor10
Scroll down ↓Interactive simulation
Figure 45Coastal EngineeringWaves & Oscillation

The effect by which surface waves entering shallower water change in wave height to conserve energy flux.

HH₀ = √( C_g₀C_g )
Bottom Depth50
Scroll down ↓Interactive simulation
Figure 46Potential FlowFlow & Motion

A second-order partial differential equation whose solutions are harmonic functions, depicting steady-state heat or ideal fluid flow.

∇²φ = 0
Boundary Voltage50
Scroll down ↓Interactive simulation
Figure 47Gravity & ElectromagnetismPlanetary & Quantum

A generalization of Laplace's equation, used when the field has a local source or sink (like charge or mass density).

∇²φ = f
Source Intensity10
Scroll down ↓Interactive simulation
Figure 48Thermal ConvectionHeat & Thermodynamics

A type of natural convection occurring in a planar layer of fluid heated from below, forming beautiful rotating cells.

Ra = g β ΔT L³(ν α) > 1708
Heat Flux5
Scroll down ↓Interactive simulation
Figure 49Vortex DecayInstability & Turbulence

An exact solution to the incompressible Navier-Stokes equations, commonly used to test computational fluid dynamics.

u = sin x cos y e^(−2νt)
Decay Time (t)1
Scroll down ↓Interactive simulation
Figure 50Quantum FluidsPlanetary & Quantum

Models the ground state of a quantum system of identical bosons using the pseudopotential interaction approximation (Bose-Einstein condensate).

iℏ ∂ψ∂t = ( −(ℏ²2m) ∇² + V_ext + g|ψ|² ) ψ
Interaction (g)1.5
Scroll down ↓Interactive simulation
Figure 51Analytical MechanicsFields & Quanta

A conservative system travels the path between times t₁ and t₂ that makes the action — the time integral of the Lagrangian L = T − V — stationary, giving the Euler-Lagrange equations of motion.

S = ∫ L(q, q̇, t) dt from t₁ to t₂, δS = 0
Gravity (g)1
Scroll down ↓Interactive simulation
Figure 52ElectrostaticsFields & Quanta

In a vacuum the divergence of the electric field at any point is set entirely by the local charge density there, so the flux out of a closed surface counts the charge it encloses.

∇ · E = ρε₀
Enclosed Charge1.5
Scroll down ↓Interactive simulation
Figure 53ElectrostaticsFields & Quanta

The total field of a discrete set of point charges is the vector sum of each individual Coulomb field, an exact consequence of the linearity of Maxwell's equations.

E(r) = (14πε₀) Σᵢ qᵢ (r − rᵢ) / |r − rᵢ|³
Charge Strength1
Scroll down ↓Interactive simulation
Figure 54Quantum MechanicsFields & Quanta

The Hamiltonian operator generates the time evolution of the wavefunction Ψ, so the complex amplitude — not a trajectory — carries every prediction the theory can make.

iℏ ∂Ψ∂t = Ĥ Ψ
Wavenumber (k)2
Scroll down ↓Interactive simulation
Figure 55Quantum MechanicsFields & Quanta

When two coherent states overlap, the probability density picks up a cross term 2Re(Ψ₁*Ψ₂). It has no classical analogue and is exactly what paints the fringes.

|Ψ₁ + Ψ₂|² = |Ψ₁|² + |Ψ₂|² + 2 Re(Ψ₁* Ψ₂)
Source Frequency1.5
Scroll down ↓Interactive simulation
Figure 56Statistical MechanicsFields & Quanta

Entropy counts possibilities: it is the logarithm of the number of microstates Ω consistent with a macrostate, which is why isolated systems drift toward the roomiest configuration.

S = k_B ln Ω
Temperature (T)1
End of archiveInteractive simulation
End of archive

Fifty figures, one continuous current. Thanks for scrolling all the way down here.

Made by tonkao
Battle arena