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Physics (Feynman Lectures)

Richard Feynman's physics, one big idea at a time — for curious K-12 minds.

Feynman Vol I5-6

Atoms in Motion

If you had to pass on just one sentence of scientific knowledge to the next generation, it would be the atomic hypothesis: all things are made of atoms —…

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Feynman Vol I5-6

Basic Physics

Before about 1920 we thought we understood the world: a three-dimensional stage, things changing in time, and particles pushed and pulled by forces like…

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Feynman Vol I5-6

The Relation of Physics to Other Sciences

A poet once said, 'The whole universe is in a glass of wine.' Look closely enough and it is true. The swirling liquid and evaporating alcohol are…

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Feynman Vol I5-6

Conservation of Energy

There is a law that, as far as we know, is never broken: energy is conserved. But what is energy? Imagine a child with 28 indestructible blocks. Each day…

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Feynman Vol I5-6

Time and Distance

Time is what a clock reads; distance is what a ruler reads. But how do you measure the age of the Earth or the distance to a galaxy? You cannot use a…

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Feynman Vol I5-6

Probability

We make guesses because we rarely have all the information. Probability is a system for making better guesses. Picture a drunk man taking steps at…

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Feynman Vol I6-7

The Theory of Gravitation

For centuries the motion of the planets was a mystery. Kepler found the pattern — planets trace ellipses, sweeping out equal areas in equal times — but…

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Feynman Vol I6-7

Motion

The world is always changing — how do we describe change precisely? The ancient Greeks tied themselves in knots over this. The answer required a new…

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Feynman Vol I6-7

Newton's Laws of Dynamics

Newton gave us a program for predicting the future. His second law, F = ma, is really a rule about change: it does not tell you where something is, but…

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Feynman Vol I6-7

Conservation of Momentum

Newton's third law says that for every action there is an equal and opposite reaction: push on me and I push back just as hard. A wonderful consequence…

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Feynman Vol I6-7

Vectors

The laws of physics do not care whether you run an experiment here or there, facing north or facing east — they must be the same regardless of how you…

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Feynman Vol I6-7

Characteristics of Force

What is a force? Saying it equals ma is only a definition; the real content of Newton's laws is that forces have simple, independent properties. The…

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Feynman Vol I6-7

Work and Potential Energy (Part A)

When a force moves an object, we say it does work, transferring energy. For some forces, like gravity, the work to move from A to B does not depend on…

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Feynman Vol I6-7

Work and Potential Energy (Conclusion)

The power of potential energy is that it lets us use conservation of energy directly. For a conservative force — gravity, or an ideal spring — the sum of…

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Feynman Vol I7-8

The Special Theory of Relativity

Nature has a strange rule: the speed of light is the same for all observers, no matter how fast they move. This simple fact has enormous consequences. If…

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Feynman Vol I7-8

Relativistic Energy and Momentum

If space and time are relative, other quantities must change too, and Newton's laws need modifying. An object's mass increases with its speed; as it…

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Feynman Vol I7-8

Space-Time

Minkowski said it best: space by itself and time by itself fade into shadows, and only their union survives. We live in a four-dimensional world. An…

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Feynman Vol I7-8

Rotation in Two Dimensions

Spinning motion can be described with perfect analogs of ordinary straight-line ideas. Instead of distance we use angle; instead of velocity, angular…

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Feynman Vol I7-8

Center of Mass; Moment of Inertia

A thrown wrench tumbles in a complicated way, yet one special point — the center of mass — flies in a simple parabola, as if all the mass were…

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Feynman Vol I7-8

Rotation in Space

In three dimensions, rotation gets wonderfully counter-intuitive. Torque and angular momentum become vectors. Push on the axis of a spinning gyroscope…

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Feynman Vol I8-9

The Harmonic Oscillator

The simple back-and-forth of a mass on a spring is one of the most important problems in all of physics, because its equation of motion shows up…

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Feynman Vol I8-9

Algebra

Mathematics is the language of physics and algebra is its grammar. Starting from simple counting and a few rules, we abstract them and demand they keep…

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Feynman Vol I8-9

Resonance

Push a child on a swing at just the right moments and she goes higher and higher — that is resonance. A system with a natural frequency responds…

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Feynman Vol I8-9

Transients

Strike a bell and it does not instantly ring a pure tone; first there is a complicated 'clank' before it settles. That start-up behavior is a transient.…

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Feynman Vol I8-9

Linear Systems and Review

Many systems are 'linear,' which simply means double the cause and you double the effect. The magic of linear systems is superposition: break a…

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Feynman Vol I8-9

Optics: The Principle of Least Time

Here is a completely different way to see physics. Instead of saying light bends because it hits water, we can say light checks all possible paths from A…

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Feynman Vol I8-9

Geometrical Optics

Using least time we can understand lenses and mirrors. A converging lens is thicker in the middle, so light through the center travels a shorter distance…

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Feynman Vol I8-9

Electromagnetic Radiation

An accelerating electric charge disturbs the electric and magnetic fields around it, and Maxwell's equations say that disturbance spreads outward as a…

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Feynman Vol I8-9

Interference

Light is a wave, and waves can add up or cancel out. Crest meets crest and they build a bigger wave — constructive interference. Crest meets trough and…

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Feynman Vol I8-9

Diffraction

When light passes through a small opening it spreads out — that is diffraction. It looks like a separate effect from interference but is really the same…

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Feynman Vol I8-9

The Origin of the Refractive Index

Why does light seem to slow down in glass? The light itself is not slowing; rather, its electric field makes the electrons in the glass jiggle, and those…

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Feynman Vol I8-9

Radiation Damping; Light Scattering

An accelerating electron radiates light, and therefore radiates energy, so it must be losing energy — an effect that acts like a friction, or 'radiation…

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Feynman Vol I8-9

Polarization

Light is a transverse wave: its electric field oscillates perpendicular to the direction it travels. Polarization is simply the direction of that…

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Feynman Vol I8-9

Relativistic Effects in Radiation

When a source of radiation moves near the speed of light, spectacular things happen. The radiation gets beamed into a narrow forward cone and its…

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Feynman Vol I8-9

Color Vision

Color is not in the light itself — it is in your eyes and brain. Your retina holds three kinds of cone cells, each most sensitive to a different range of…

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Feynman Vol I8-9

Mechanisms of Seeing

The eye is far more than a camera; the retina is part of the brain, and a great deal of computation happens there before any signal leaves the eye.…

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Feynman Vol I8-9

Sound. The Wave Equation

Sound is a wave of pressure ripples traveling through a medium like air. We can derive the equation governing it — the wave equation — directly from…

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Feynman Vol I8-9

Beats

Add two sound waves of slightly different frequencies and you get a wave at the average frequency whose loudness pulses up and down. Those pulses are…

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Feynman Vol I8-9

Modes

When a wave is confined — like a wave on a guitar string — it cannot have just any frequency; it is forced into specific patterns called modes, each with…

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Feynman Vol I8-9

Harmonics

For a simple vibrating string, the mode frequencies are whole-number multiples of the lowest one — these are the harmonics. The particular mixture of…

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Feynman Vol I8-9

Waves

Here we meet some of the richest wave phenomena in nature. When something moves faster than the waves it makes — a boat on water or a jet in air — it…

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Feynman Vol I8-9

Symmetry in Physical Laws

There is a deep, beautiful link between the symmetries of the universe and its conservation laws. Because the laws are the same everywhere (symmetry…

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Feynman Vol II9-10

Electromagnetism

Matter is held together by enormous electrical forces, but they are so perfectly balanced between positive protons and negative electrons that we never…

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Feynman Vol II9-10

Differential Calculus of Vector Fields

To talk about fields that vary from point to point, we need a new calculus and a special operator. The gradient of a field points the way of steepest…

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Feynman Vol II9-10

Vector Integral Calculus

Differential laws describe what happens at each point; integral laws describe the overall behavior. Gauss's theorem says the total flux of a field…

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Feynman Vol II9-10

Electrostatics

The world of stationary charges runs on two simple laws. First, electric field lines start on positive charges and end on negative ones, so the total…

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Feynman Vol II9-10

Application of Gauss' Law

Gauss's law is a powerful shortcut for finding electric fields where there is symmetry, avoiding hard integrals. For a uniformly charged sphere, symmetry…

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Feynman Vol II9-10

The Electric Field in Various Circumstances

When conductors are present, charges shuffle around until the surface is all at one potential, which makes problems tricky. A clever fix is the 'method…

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Feynman Vol II9-10

The Electric Field in Various Circumstances (Continued)

The equations of electrostatics turn up far beyond charges. For two-dimensional problems there is a powerful method using functions of a complex…

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Feynman Vol II9-10

Electrostatic Energy

It takes work to push charges together against their repulsion, and that work is stored as potential energy. But where is the energy? A very useful idea…

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Feynman Vol II9-10

Electricity in the Atmosphere

On a clear day there is a downward electric field of about 100 volts per meter in the air — the Earth itself is negatively charged. This drives a small…

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Feynman Vol II9-10

Dielectrics

Put an insulating material — a dielectric — into an electric field and the field inside it weakens. This is because the field polarizes the atoms,…

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Feynman Vol II9-10

Magnetostatics

Magnetostatics studies the magnetic fields of steady currents. Two laws rule it: magnetic field lines never start or stop but form closed loops, and the…

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Feynman Vol II9-10

The Vector Potential

Just as the electric field comes from a voltage, the magnetic field can be derived from a 'vector potential.' Is it a real field or just a math…

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Feynman Vol II9-10

Induced Currents

Faraday discovered that a changing magnetic field creates an electric field — the principle of induction. Move a magnet near a wire loop, or change a…

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Feynman Vol II9-10

The Maxwell Equations

This is the great moment of synthesis. Maxwell noticed the known laws of electricity and magnetism were inconsistent with conservation of charge, and…

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Feynman Vol II9-10

The Principle of Least Action

Like mechanics, all of electrodynamics can be summed up in one powerful principle: least action. The motion of a charged particle and the behavior of the…

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Feynman Vol II9-10

AC Circuits

The laws of electromagnetism let us analyze alternating-current circuits. For smoothly oscillating voltages and currents there is a beautiful trick using…

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Feynman Vol II9-10

Waveguides

To send high-frequency waves like microwaves from place to place you cannot just use wires — they would act as antennas and radiate the energy away.…

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Feynman Vol I10-11

The Kinetic Theory of Gases

A gas is a vast swarm of tiny molecules in constant, random motion, and its properties follow from that picture. Pressure on the container walls is just…

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Feynman Vol I10-11

The Principles of Statistical Mechanics

Kinetic theory generalizes into a powerful framework: statistical mechanics. Its core is Boltzmann's law — in a system at thermal equilibrium, the chance…

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Feynman Vol I10-11

The Brownian Movement

Watch a tiny smoke particle under a microscope and you see it jiggle in a jerky, random dance — Brownian motion. It is direct, visible proof that atoms…

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Feynman Vol I10-11

Applications of Kinetic Theory

Statistical ideas reach far and wide. The rate a liquid evaporates, the way electrons boil off a hot filament, the ionization of a hot gas, and the speed…

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Feynman Vol I10-11

Diffusion

Open a bottle of perfume in the corner of a still room and the scent eventually spreads everywhere — that is diffusion. No force pushes the molecules…

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Feynman Vol I10-11

The Laws of Thermodynamics

Thermodynamics rests on a few sweeping laws. The First Law is conservation of energy: you cannot get something for nothing. The Second Law is deeper…

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Feynman Vol I10-11

Illustrations of Thermodynamics

Thermodynamics is abstract but yields surprising, exact relationships between the properties of materials. For example, it can prove that heating a…

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Feynman Vol I10-11

Ratchet and Pawl

Imagine a tiny paddle wheel in a box of gas, attached to a ratchet that lets it turn only one way. Won't random molecular hits be rectified into useful…

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Feynman Vol II10-11

Inside Dielectrics

A material can polarize in two ways. In nonpolar molecules a field distorts the electron cloud to induce a dipole; in polar molecules like water, which…

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Feynman Vol II10-11

Reflection from Surfaces

The laws of reflection and refraction can be derived straight from Maxwell's equations by matching the fields at the boundary between two materials. This…

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Feynman Vol II10-11

The Internal Geometry of Crystals

Most solids are crystals: their atoms sit in a regular, repeating three-dimensional lattice. That hidden geometric order is responsible for a crystal's…

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Feynman Vol II10-11

Tensors

How do you describe a material that behaves differently in different directions? A single number is not enough, and often neither is a vector — you need…

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Feynman Vol II10-11

The Magnetism of Matter

Most materials are only weakly magnetic. Paramagnetism happens when atoms carry permanent magnetic moments that a field tends to line up, slightly…

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Feynman Vol II10-11

Paramagnetism and Magnetic Resonance

Treated with quantum mechanics, paramagnetism reveals that atomic magnetic moments can only point in a discrete set of directions relative to a field.…

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Feynman Vol II10-11

Ferromagnetism

Ferromagnetism is the strong magnetism of iron. It springs from a purely quantum effect, the 'exchange interaction,' which makes the spins of electrons…

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Feynman Vol II10-11

Elasticity

Elasticity is the way solids deform under stress and spring back when it is released. For small deformations, the strain (fractional change in size) is…

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Feynman Vol II10-11

The Flow of Dry Water

Fluid dynamics studies liquids and gases in motion. The simplest case is an ideal fluid — incompressible and with no internal friction — playfully called…

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Feynman Vol II10-11

The Flow of Wet Water

Real fluids have viscosity — internal friction — which makes things much harder and far more interesting, and is the source of drag on a moving object.…

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Feynman Vol II10-11

Curved Space

Einstein's general relativity gives a new view of gravity: not a force, but a property of space-time itself. Mass and energy curve space-time, and…

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Feynman Vol III11-12

Quantum Behavior

Here is the heart of modern physics, and it is a true mystery. Send electrons through two slits and they arrive one by one, like particles — yet the…

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Feynman Vol III11-12

The Relation of Wave and Particle Viewpoints

The wave and particle natures are two complementary sides of one reality, tied together by Heisenberg's uncertainty principle: you cannot know both a…

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Feynman Vol III11-12

Probability Amplitudes

Quantum mechanics never predicts a single outcome with certainty; it predicts probabilities, computed from a new kind of number called a probability…

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Feynman Vol III11-12

Identical Particles

There is a strange, beautiful rule for identical particles like electrons or photons. If a process can happen two ways that differ only by swapping two…

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Feynman Vol III11-12

Spin One-Half

Particles carry an intrinsic angular momentum called spin. The electron is a spin-one-half particle, meaning its spin along any axis can only be +half or…

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Feynman Vol III11-12

The Dependence of Amplitudes on Time

How do quantum states change over time? The amplitudes to be in different base states evolve according to equations governed by a grid of numbers called…

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Feynman Vol III11-12

The Ammonia Maser

The ammonia molecule is a perfect real-world two-state system: its nitrogen atom can sit on either side of the plane of three hydrogen atoms, and quantum…

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Feynman Vol III11-12

The Hyperfine Splitting in Hydrogen

Even hydrogen's ground state is not a single level. The magnetic moments of its electron and proton interact, and the energy differs slightly depending…

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Feynman Vol III11-12

Propagation in a Crystal Lattice

How does an electron move through the perfectly regular lattice of a crystal? It has some amplitude to tunnel, or hop, from one atom to the next, and…

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Feynman Vol III11-12

Semiconductors

Energy bands explain insulators, conductors, and semiconductors. In an insulator, a band is completely full and a big gap separates it from the next…

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Feynman Vol III11-12

The Dependence of Amplitudes on Position

So far we described states by amplitudes for a set of discrete base states. But to describe a particle that can be anywhere in continuous space, we…

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Feynman Vol III11-12

Symmetry and Conservation Laws

The deep link between symmetry and conservation, first seen in classical physics, is even more profound in quantum mechanics. If a system is unchanged by…

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Feynman Vol III11-12

Angular Momentum

In quantum mechanics angular momentum is quantized: its component along any axis can only take a discrete ladder of values separated by whole units.…

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Feynman Vol III11-12

The Hydrogen Atom and the Periodic Table

Solving the Schrodinger equation for hydrogen was one of quantum theory's first great triumphs. It correctly predicts the atom's discrete energy levels —…

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Feynman Vol III11-12

The Schrodinger Equation in a Classical Context: Superconductivity

Superconductivity is a spectacular, large-scale quantum effect. Below a critical temperature, some metals lose all electrical resistance and expel…

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