Physics

Physics keeps discovering that unrelated things obey the same equation. A pendulum, a spring and a tuned circuit are one problem wearing three costumes, and you can drive all three here.

Newest in this category

Chapters

Short sequences rather than single tools. Each step hands the next one something specific, so they are worth doing in order.

L2: school

Bending light

PHYA lens is a boundary that somebody curved, and no page on this path introduces physics the first one does not already contain. What changes is how much is asked of it: one surface, then an ideal lens, then a piece of glass.

  1. 01Snell's law
  2. 02Ray-tracing a lens
  3. 03Real lenses

L2: school

Resistance, then reactance

PHYA capacitor has no resistance and limits the current anyway, and what it sets is a time rather than a number of ohms. The second page shows that the time belongs to any system with one store and one drain. The third adds a second store, and the time becomes a frequency.

  1. 01RC circuit
  2. 02Step response
  3. 03RLC resonance

L2: school

Throwing things

PHYThree tools, and the third one breaks the first two. Constant acceleration has a closed-form answer, so the first two steps are algebra. Air resistance is not constant, and from there the only honest method is to integrate it step by step.

  1. 01SUVAT
  2. 02Projectile motion
  3. 03Drag and wind

L2: school

Wave optics

PHYRay optics says light goes straight and an edge casts a sharp shadow. Each page here draws that answer as a ghost beside the wave answer, and what stands in the light's way changes from page to page: two surfaces, one slit, a round aperture, and finally an opaque disc whose shadow is bright at its centre.

  1. 01Thin films
  2. 02Single slit
  3. 03The diffraction limit
  4. 04The spot of Arago

L2: school

Least time, least action

PHYThe path a light ray takes, a sliding bead follows and a thrown ball flies is the one along which a small change makes no first-order change in a total: time for the first two, action for the ball. Every page lets you bend the path and watch the total barely move, and two of them find a path whose total is stationary without being least.

  1. 01Fermat's principle
  2. 02Mirages
  3. 03The brachistochrone
  4. 04Least action

L2: school

What is not a resistor

PHYOhm's law describes one kind of part. The five here store energy in a voltage or a current, conduct in one direction, amplify, and amplify precisely, and each is unreliable on its own: a transistor's current gain β varies threefold between samples of the same type. The circuit around a component is what makes it predictable, and every page shows how.

  1. 01Capacitor
  2. 02Inductor
  3. 03Diode
  4. 04Transistor amplifier
  5. 05Op-amp

L2: school

Quantum mechanics: matter as waves

PHYLight arrives in packets, and the same constant h then gives every particle a wavelength. The rest follows from taking that wave seriously: made to fit a box, it has a lowest energy that is not zero; it leaks through walls it cannot climb; and squeezed into a small space it spreads over many wavenumbers, which is the uncertainty principle.

  1. 01The photoelectric effect
  2. 02Matter waves
  3. 03Particle in a box
  4. 04Quantum tunnelling
  5. 05Uncertainty and wave packets

L3: undergraduate

How a weather forecast is made

GEOA forecast is a model run forward from a starting state nobody knows exactly, so forecasters run it many times and let the disagreement say how far to trust it. The second page opens the model and finds a way to fail that has nothing to do with chaos. The third goes back to Lorenz's equations of 1963, where the run's position is soon lost and the shape it draws never is.

  1. 01Ensemble forecasting
  2. 02Weather on a grid
  3. 03The Lorenz attractor

Problems solved in full

What you find out here

Articles written from these tools

Every tool on this shelf

Mechanics & Motion

Angular Momentum
Pull two 2 kg dumbbells from 0.8 m to 0.2 m on a turntable and your spin triples, 1 to 3 rev/s. So does your kinetic energy, 71.06 J to 213.18 J, and your arms do the 142.12 J. With zero angular momentum you can still turn 25° a stroke.
Arches, Cables & the Line of Thrust
A semicircular stone arch 10 m across stands at 0.54 m thick and falls at 0.45 m, while the stone is barely stressed. Turn a hanging chain upside down and you get the arch that stands at almost no thickness at all.
Banked Curves
A 200 m bend banked at 8% needs no friction at 45.09 km/h. Slower, friction pushes the car outwards; on wet black ice a stopped car slides down a 10% bank; and past 51.34° on a dry road no speed is too fast.
Beam Deflection Calculator
The same 5 m beam under the same load sags 4.885 mm on two pins, 0.977 mm clamped and 46.894 mm as a cantilever. Nothing was added to the beam; only the ends changed.
Bernoulli & the Venturi Effect
Narrow a pipe and watch speed square while pressure falls as the fourth power, until the water reaches its vapour pressure and cavitates instead of going faster.
Brachistochrone: the Fastest Slide
A bead let go 1 m above and 1 m to the side of its finish takes 0.6387 s down a straight ramp and 0.5830 s down a cycloid 0.060 m longer. Put the finish 4 m away and the fastest path dips half a metre below it before climbing back.
Buoyancy & Archimedes' Principle
Let a 40 kg iron anchor go from a boat to the bottom of a pond and the pond goes down 5.83 mm while the boat rises 25.0 mm. A floating body displaces its weight of water and a sunk one only its volume.
Coriolis Effect and Foucault's Pendulum
In Paris a Foucault pendulum's swing turns 11.32° an hour and takes 31.79 h to go round; on the equator it never turns. Water in a sink feels about 10⁻⁶ g of Coriolis, and a stone dropped 158.5 m down a mine shaft at Freiberg lands 27.65 mm east.
Darcy's Law & Groundwater Flow
How much water crosses gravel, sand or clay, how fast the water itself travels through the pores, and the gradient at which the law stops being linear.
Efflux Jets from a Tank
The bottom hole leaves at 4.20 m/s and the top at 2.43 m/s, and both land at 1.039 m. The middle one beats them at 1.200 m, which is exactly the water depth, and no tank throws further than it is deep.
Euler Buckling & the Slender Column
A 3 m steel strut buckles at 8.72 kN. Swap it for steel nearly three times as strong and it buckles at 8.72 kN — the same number to the last digit, because Euler's formula contains the stiffness and not the strength.
Free-Fall Calculator
Calculate fall time, impact speed, and kinetic energy for an object dropped from a given height under any gravity.
Gear Train Ratio & Speed Simulator
Four gears, two ways to arrange them. Set the tooth counts and see which of them reach the output ratio and which are only along for the ride.
Gyroscope
A bicycle wheel spinning at 10 rev/s, let go with its axle level on a pivot, drops 0.597° as it starts to turn sideways, once every 18.12 s. Spin it twice as fast and it turns half as fast and drops a quarter as far.
Inclined Plane, Screw & Wedge
A ramp, a screw and a wedge are one shape used three ways. Set the angle and the friction, and watch the advantage the geometry offers drift away from the one you actually get.
Kinematics (SUVAT) Calculator
Solve the SUVAT equations of motion for constant acceleration. Enter any 3 of displacement, initial velocity, final velocity, acceleration, and time to find the other 2.
Lever Classes & Mechanical Advantage
Set the two arms and the load, and watch the effort, the mechanical advantage and the distance the effort end has to travel. The class is decided by the geometry, not by the button you pressed.
Mohr's Circle & Stress on a Tilted Plane
Pull a steel bar at 100 MPa and its cross-section carries no shear at all, while a plane at 45° carries 50 MPa. Turn the element by θ and its point moves 2θ round the circle.
Momentum & Collision Lab
Simulate 1D cart collisions to explore conservation of momentum, kinetic energy changes, and the coefficient of restitution.
Navier–Stokes: Flow Past a Cylinder
Below about Re 47 the wake behind a cylinder settles and stays still; above it the same equations swing for ever. Solve Navier–Stokes live, find the threshold, and see why a frictionless cylinder would feel no drag at all.
Newton's Second Law (F=ma) Simulator
Push a block with friction and an optional incline, and watch Newton's laws play out: net force, F=ma, and a full free-body diagram, animated live.
Poiseuille's Law & Pipe Flow
Flow through a pipe from Poiseuille's law, with the fourth power made visible: halve the radius and the flow divides by 16. Shows where the law stops being valid.
Pressure at Depth
Four vessels over one base, filled to 0.5 m: they hold anything from 1.606 to 68.068 litres, and every one of them reads 4.896 kPa and pushes on its base with 153.8 N.
Projectile Drag/Wind Simulator
Projectile motion with air drag and wind.
Projectile Motion Simulator
A 45° launch is always four times as wide as it is tall, and a 5° aiming error costs 62 cm out of 40.775 m. From an 18 m cliff the best angle drops to 37.248°, and keeping 45° throws away 1.532 m.
Pulley Systems & Mechanical Advantage
Count the rope sections holding the load and you have the mechanical advantage. Change the efficiency and watch where the loss actually shows up.
Reynolds Number & Flow Regime
Laminar or turbulent, for any fluid, speed and pipe. Water and honey sit either side of the line at the same speed in the same pipe, and household plumbing is almost never laminar.
Roller Coaster Energy Simulator
See kinetic and potential energy exchange on a customisable roller coaster track
Rolling Race & Moment of Inertia
Release a solid ball and a hoop together down a 2 m ramp and when the ball reaches the bottom the hoop is still 0.600 m behind, whatever either weighs and however big it is. Two cylinders of 5 kg and 0.2 kg finish in the same 1.537 s.
Screw Thread
Across the 116,280 combinations of radius, pitch and friction the sliders reach, the best any self-locking screw manages is 49.86% efficiency. And 6.64 N on a spanner holds 1,000 N in the air.
Shaft Torsion: Solid and Hollow Shafts
A hollow shaft with its bore at 80% of the diameter keeps 59% of the solid shaft's torque capacity for 36% of the steel. Carry the same power at a tenth of the speed and the shaft has to be 2.15 times as thick.
Statically Indeterminate Truss & the Redundant Bar
Three steel bars hold 150 kN, and statics has only two equations for them. The third comes from how the bars stretch, which is why warming the centre bar by 40 K compresses it by 19.88 kN with nothing hanging from the truss.
Tank Drain & Torricelli Decay
Watch a tank empty under Torricelli's law, with the level falling as a parabola because the outflow follows the square root of the depth.
Terminal Velocity & Stokes' Law
How fast a sphere settles, from Stokes' law and quadratic drag, with the radius where Stokes stops being true solved in closed form and shaded on the chart.
The Principle of Least Action
A ball thrown 20 m and caught 2 s later has an action of 67.9432 J·s; staying level would score 100. Bend its path 1 m either way and the action rises by the same 1.2337 J·s. On a spring the same rule fails after half a period.
The Tennis Racket Theorem
Spin a body with three different moments of inertia about its middle axis and it turns over every few seconds while its angular momentum never moves: every 4.38 s for a 1 : 2 : 3 body at 1 rev/s with a wobble of 10⁻³. A thousand times less wobble buys only 3.81 s more, and a body that leaks energy ends up spinning about the axis of its largest moment.
Truss Analysis & the Method of Joints
A Pratt and a Howe truss are the same 21 members on the same 12 nodes. Mirror the diagonals and the long members go from tension to compression, which is why steel bridges are Pratt.
Wheel & Axle Mechanical Advantage
Two radii on one shaft. Set them and read the advantage, the effort, and how much rope each radius winds in a single turn.

Oscillations, Waves & Optics

Bragg's Law & X-ray Diffraction
How the distance between two atoms gets measured to five decimal places without anyone seeing either of them. Bragg's law turns an angle you can read off a dial into a spacing you cannot reach.
Chaos Bouncing Balls Lab
Many-ball gravity and collision sandbox with twin-run divergence tracking.
Circular Motion Lab
The first preset holds 3.00 m/s from start to finish and still reads 6.00 m/s² of acceleration the whole way round. Raise the spin from 2.0 to 4.5 rad/s and that becomes 30.38 m/s², about 3.1 g.
Diffraction Grating
Two slits or six hundred, green light through 300 lines/mm reaches its first order at 9.18°. See why a DVD shows fewer orders than a CD, and why the sodium doublet splits in the second order and not the first.
Doppler Effect Simulator
A 700 Hz siren moving at 30 m/s reads 767.1 Hz ahead and 643.7 Hz behind, averaging 705.4. Move the listener at the same speed instead and the average is exactly 700: the air knows which of you moved.
Double Pendulum Explorer
Interactive double pendulum chaos simulation.
Fermat's Principle: the Lifeguard Problem
A lifeguard who runs straight at the swimmer takes 22.90 s; the fastest path takes 19.48 s and is longer. Go in a metre from the best point and you lose 16 ms. A corgi measured on Lake Michigan was never more than a tenth of a second off.
Hooke's Law & Spring Lab
Two 150 N/m springs joined end to end make 75 N/m. Read that backwards and any spring is its own two halves in series, so cutting a spring in half makes it stiffer, not weaker.
Lens and Imaging Studio
Move object and lens parameters to see real/virtual image formation with principal rays and lens equation updates.
Malus's Law & Crossed Polarisers
Stack polarising filters and watch Malus's law decide what survives. Two crossed filters pass nothing; slide a third between them at 45° and 12.500% comes back; ten across the same quarter turn reach 37.957%.
Mirages: Light Bent by Hot and Cold Air
Over a road 20 °C hotter than the air, every downward line of sight shallower than 0.33° is turned back up, so the puddle starts 209 m ahead and drives away as fast as you do. Its light takes a path that is not even locally the quickest.
SHM Resonance Lab
The two driven presets are identical except for the rhythm, 4.00 against 2.2 rad/s, and amplification moves from 6.667 to 1.424. At resonance a 0.0750 m static push becomes a 0.5000 m swing.
Signal Sampling & Nyquist Theorem
A 30 kHz tone nobody can hear, sampled at 44.1 kHz with nothing filtering it first, comes back as an audible 14,100 Hz whistle at full strength. No processing afterwards can separate it out again.
Simple Pendulum / SHM
A 1 m pendulum released at 20° has a period of 2.021 s, not the textbook 2.006 s. That 0.76% is 11 minutes a day on a clock, which is why Huygens went to a cycloidal suspension in 1656.
Single-Slit Diffraction
Shine a laser through a fine slit and narrow it: the light on the wall spreads wider, not narrower. The pattern is computed from Fresnel's integrals beside the band ray optics predicts, and a hair in the beam makes the same pattern, which is how to measure one.
Snell's Law Refraction Simulator
Light entering water at 30° bends to 22.08° and reflects 2.11%. A fish sees the whole sky squeezed into a cone of about 98°, and at 53.06° the reflected light is completely polarised.
Standing Waves Explorer
A 1 m string at 343 m/s sounds 171.5 Hz, and the third harmonic lands on exactly 514.5 Hz rather than near it. Stress caps the wave speed, so no 1 m steel string reaches much above 265 Hz at any gauge.
The Diffraction Limit
Two points of light through a round opening: each spreads into an Airy disc, and once the two discs merge into one peak no magnification can split them. See why Hubble's 2.4 m mirror blurs every point on the Moon into a disc 107 m in radius, and why the larger JWST is blurrier in the infrared.
The Spot of Arago
Ray optics says a round disc casts a dark round shadow. In Fresnel's theory, which holds while the light bends through small angles, a spot at its centre is as bright as the open beam for a disc of any size. Compute the shadow by Fresnel diffraction, see why the spot needs a point of light and a true edge, and turn the disc into a lens.
The Wave Equation in One, Two and Three Dimensions
Strike a string, a sheet and a space with the same kick and listen 5a away. The string stays lifted by 0.5333 for ever, the sheet still holds 9.93% of its peak at ct = 20a, and space is silent the moment the wave has passed.
Thin Lens Ray Tracer
Trace rays through converging and diverging lenses with real-time image position and magnification.
Thin-Film Interference
Why a soap film turns black just before it bursts, why a thick film is colourless, and why a lens coating works. Every colour on the page is computed from the film's reflected spectrum, beside what ray optics would predict.
Wave Interference / Two-Source
Explore two-source wave interference with adjustable wavelength, source separation, and fringe order in a live 2D pattern.

Thermodynamics

Carnot Engine Simulator
Explore the Carnot cycle: PV diagram, efficiency η = 1 − Tc/Th, and energy flow
Heat Loss Through a Wall: U-values
Layers of a wall add like resistors in series and a window sits beside them in parallel. Why the first 50 mm of insulation saves the most, why the window decides the heat loss, and why single glazing insulates with air.
Ideal Gas Law Calculator
PV = nRT with an interactive piston diagram and isotherm curves
Latent Heat: Ice in a Drink
Mix ice into water and read the temperature they settle at. Specific heat capacity, latent heat of fusion, and the 0 °C plateau where more ice changes nothing.
The Heat Equation
A rod with its ends in ice and a hot stretch in the middle. Watch the profile relax into a single sine arch as its sharp detail dies first, see why twice the length takes four times as long, and draw your own starting temperature.
The Lorenz Attractor
Two runs a billionth apart end 16 units apart and still put every maximum of z on the same curve. The 1963 equations, the volume that contracts to 10⁻³⁵⁶, and the object left behind.
Thermal Touch: Why Metal Feels Colder Than Wood
A 20 °C aluminium block takes the surface of your skin to 20.61 °C and a 20 °C oak table leaves it at 29.30 °C. Thermal effusivity √(kρc), the contact temperature, and how deep the heat gets in a second.
Van der Waals Equation & the Critical Point
Where the ideal gas law stops being true, and by how much. Two fitted constants give an equation that grows a liquid phase nobody put into it, and that predicts the same critical compressibility, 3/8, for every gas there is.

Electricity, Magnetism & Circuits

AC Voltage: RMS, Peak and What Your Meter Reads
A cheap multimeter reads a square wave 11.0721% high and a triangle 3.8088% low, and tells you neither. It multiplies by 1.110721 because that is right for a sine, and applies it to whatever it is given.
Capacitors & Stored Energy
Charge a capacitor from a fixed supply through any resistor and half the energy becomes heat. Raise the supply in ten steps instead and the loss is a tenth as large.
Charged Particles in a Magnetic Field
A proton in a 1.5 T field laps its circle in 43.73 ns at 10 keV and again at 40 keV, on a circle twice the size. Why the cyclotron works, why relativity stops it, and how a magnet sorts uranium.
Electric Field Visualiser
Place point charges and see field lines, vectors, and equipotential contours
Faraday's Law: a Simple Generator
Spin a generator with nothing connected and it turns freely while making a peak of 9.425 V. Connect a 12 Ω lamp and the same coil pushes back with a mean torque of 0.009425 N·m, because every watt of light has to come from the hand turning it.
Inductors & the Switch-Off Spike
Open the switch on a 12 V coil carrying 30 mA and the switch sees 360.2 V, because the current cannot stop at once. A diode across the coil holds it to 12.74 V and, in this model, lets the coil go sooner as well.
Internal Resistance & EMF
The most power you can draw from any source arrives at exactly 50% efficiency — half of it is burned inside the source. Nine times the load and a ninth of the load deliver the same watts, at 90% and 10%.
Inverse Square Law Explorer
See how gravity, light intensity, and electric force all decay as 1/r² — a geometric consequence of spreading over a sphere.
Kirchhoff's Laws & the Wheatstone Bridge
Five resistors, and no two of them are in series or in parallel — the combination rules have nothing to grab. Take the detector out and two series pairs appear at once.
Ohm's Law Calculator
This page's own LED preset is the trap: 3.3 V across 220 Ω gives 15 mA, but a red LED holds about 2 V itself, leaving the resistor 1.3 V and 0.005909 A, under half the preset's answer.
Op-Amp & Negative Feedback
An op-amp with a gain of 100,000 makes a ×10 stage of 9.9990, and halving that gain only moves it to 9.9980. The two inputs sit 100.49 µV apart at 1 Hz and 9.999 mV apart at 1 kHz.
RC Circuit Simulator
τ = RC contains no voltage. Change the supply from 5 V to 12 V and the time to 63.2% does not shift by a millisecond. A resistor-fed capacitor is also 50% efficient however it is designed.
Resistors in Series and Parallel
A 100 W and a 60 W bulb wired in series draw 37.500 W between them, not 160, and the 60 W one is the brighter of the two.
RLC Resonance Analyser
The default components are barely resonant: Q = 0.6287 puts a 1.59 kHz bandwidth around a 1.00 kHz centre. Reaching the Q ≈ 111 that AM tuning needs would take the series resistance down to 0.57 Ω.
Smith Chart & RF Black Magic Lab
Interactive Smith Chart tool for RF impedance matching, reflection coefficient visualization, and understanding microwave black magic
The Diode and the 0.7 V Rule
A diode's current rises tenfold every 59 mV at room temperature, from picoamps up, with no voltage at which it switches on. Where the curve seems to bend is set by how the axis is drawn, and the 0.7 V rule is 0.27% out at 5 V and 19.89% out at 1 V.
Transistor Amplifier
Two transistors with the same part number can differ threefold in β. Bias the base with a divider and add an emitter resistor, and the gain moves less than 1% across that spread; feed it through a single resistor, and the gain moves threefold.
Wire Resistance & Resistivity
Aluminium needs 57.7% more cross-section than copper to match it, and still weighs 47.5% as much. Of the six other metals on the page it is the only one that comes out lighter, and every overhead line is made of it.

Control Systems & Modern Physics

de Broglie Wavelength & Matter Waves
A 54-volt electron has a wavelength of 0.1669 nm, the size of the gaps between atoms, which is why a nickel crystal diffracts it. See why a neutron at room temperature does the same, and where the textbook formula goes wrong.
Missile Interception & Proportional Navigation
See how a guided interceptor homes in on a moving target. Compare pure pursuit with proportional navigation and watch the guidance equation a = N·Vc·λ̇ compute live, frame by frame.
Nuclear Binding Energy and the Mass Defect
An atom weighs less than its protons and neutrons, and the missing mass is the binding energy. Why nickel-62, not iron-56, tops the curve, why beryllium-8 falls apart, and why fusion beats fission per kilogram.
Particle in a Box
An electron in a 1 nm box can never have less than 0.3760 eV, and in its lowest level it is in the middle third 60.9% of the time. See why the same box comes within 6% of butadiene's absorption and misses a carrot's by a factor of three.
Photoelectric Effect & the Threshold
Double the brightness of violet light on sodium and twice as many electrons come off, each no faster than before. Swap it for red light sixteen times as plentiful and not one electron leaves the metal.
PID Control Tuner
Tune PID gains and inspect step response.
Quantum Tunnelling
An electron with half the energy it needs gets through a 1 eV, 0.5 nm barrier 10.14% of the time, and a proton 1.535×10⁻⁶⁷. Exact transmission through a rectangular barrier, and why each 0.1 nm of gap costs a tunnelling microscope a factor of 8.8.
Radar Physics Simulator
Received power falls as 1/R⁴, so the presets' 100,000-fold span in radar cross-section becomes only 17.8× in range. Cutting cross-section 500-fold buys 4.7×, and each further halving costs another 16.
Special Relativity Explorer
Two boosts of 0.5c compose to 0.8c, because rapidity adds where speed does not. The muon preset thins 650 m of atmosphere to 25.995 m; the GPS preset reads γ = 1 while an uncorrected fix walks 11 km a day.
Uncertainty Principle & Wave Packets
Build a wave packet from plane waves and the product of its two widths never falls below ½. A Gaussian reaches it and a box never comes close. An electron held to 1 nm doubles its width in 29.92 fs; a 1 µg grain held to 1 µm takes a million years.
Related categories: Mathematics, Astronomy & Space, Computing