Chapter 4
Introductory Quantum Mechanics · Chapter 4

The Schrödinger Equation

We have a wave, a meaning for its strength, and a rule for its odds – but no law telling it how to move. In the winter of 1926 an Austrian physicist wrote that law down. Everything in chemistry follows from it.

Every physics revolution gets its equation. Newton’s tells forces how to move things; Maxwell’s tells light how to travel. Quantum mechanics got its own in early 1926, when Erwin Schrödinger – challenged, the story goes, by a colleague who scoffed that a proper wave deserves a proper wave equation – went on a winter retreat in the Alps and came back with the law that drives ψ\psi.

You have already watched it at work without knowing: every packet, fringe and corkscrew in the last three chapters obeyed it. This chapter puts it in charge openly, in three classic arenas: a particle trapped in a box, a particle in a valley, and – the showstopper – a particle walking through a wall.

4.1Standing waves, again – but exact this time

Before solving anything, one idea unlocks all three arenas. Ask: are there wave shapes that don’t change as time passes – shapes where the arrows underneath all turn in step, so the strength ψ2|\psi|^2 freezes? There are. They are called stationary states, and each one comes with a definite energy: the faster its arrows turn, the higher the energy. They are the quantum version of a guitar string’s pure notes – §1.4’s hunch, now made exact.

Confine a wave – in a box, in a – and only certain notes fit: energy comes in rungs. Every other motion, it turns out, is just a chord: several notes sounding at once, beating against each other. Find the notes and you have solved the system completely.

4.2The particle in a box

The simplest cage: a particle stuck between two impenetrable walls. The wave must vanish at both walls, so – exactly like a guitar string pinned at both ends – a whole number of half-waves must fit. One bump, two bumps, three: that integer nn is the only choice left, and each choice has its energy rung. Notice the rungs in the figure spread apart as you climb – and notice there is no rung at zero. A confined quantum particle cannot sit still: perfect stillness would mean perfect position and perfect (zero) speed, which Chapter 3’s uncertainty floor forbids.

Then tick the superposition box. One pure note holds perfectly still; two notes at once slosh side to side. That slosh is what “motion” is in quantum mechanics.

Particle in a box – the quantum guitar string
FIG. 4.1
one pure note → the shape holds perfectly stillonly the hidden wave underneath keeps turning
The eigenstates of a box are standing waves – §1.4's guitar-string picture made exact: n half-wavelengths must fit, so energy comes in rungs E_n = n²E₁. A single rung is a stationary state: its density is frozen for all time even though the phase underneath turns constantly. Mix two rungs and the interference cross-term oscillates at the difference frequency ΔE/ħ – motion in quantum mechanics is always a superposition beating against itself. Units: ħ = m = L = 1.

4.3The harmonic oscillator

Replace the box with a smooth valley – a marble in a bowl, . This one potential is physics’ favourite, because near the bottom every smooth valley looks like it: vibrating molecules, atoms in crystals, even light waves are “springs” in disguise. Its rungs hold a surprise: they are perfectly evenly spaced. Climbing any rung costs exactly the same energy packet, ω\hbar\omega – and that is where Chapter 0’s light-comes-in-packets rule was hiding all along.

Then switch to the coherent state: a lump displaced up the valley wall and released. It swings back and forth exactly in step with a classical marble – the red dot – and never spreads out. After four chapters of quantum strangeness, this is the familiar world being handed back: it was a special superposition all along.

The harmonic oscillator – nature's favourite ladder
FIG. 4.2
rung 2: the shape stands still – and even rung 0 can’t lie flat at the bottomevery rung costs the same extra energy
Every smooth valley looks like a parabola near its bottom, so this one potential describes vibrating molecules, crystal lattices, and light itself. Its rungs are evenly spaced – emitting or absorbing always costs the same quantum ħω, which is where Chapter 0's photons came from. Eigenstates stand still and spill past the classical turning points; the coherent state (a displaced ground state) swings like a pendulum with constant width – the classical world recovered as a special superposition. Units: ħ = m = ω = 1.

4.4Tunnelling: walking through walls

Now the flagship. Roll a ball at a hill too tall for its speed and it comes back – always, guaranteed. Send a quantum particle at a wall too tall for its energy and something impossible happens: a sliver of the wave seeps through, and the particle is sometimes found on the far side, having crossed a region it never had the energy to be in. Inside the wall the wave cannot ripple, so it fades – but a wall of finite thickness can’t quite fade it to nothing.

This is not a curiosity; it runs the universe. The Sun shines because protons tunnel through their electric repulsion. Radioactive atoms decay when a fragment tunnels out of the nucleus. Your phone’s flash memory writes bits by pushing electrons through an insulating wall. Watch the split in the figure – and mind how violently the leak responds to the width slider.

Quantum tunnelling – a packet meets a barrier it cannot climb
FIG. 4.3
the wall is too tall to climb – yet 213 in 1,000 get throughmade it so far: 0.0%
A wave packet (E₀ = 1.125, ħ = m = 1) integrated with the split-step Fourier method – unitary by construction, so ‖ψ‖² holds at 1. With V₀ > E₀ a classical particle always bounces; the wave leaks an exponentially thin tail through the barrier, and the transmitted fraction matches the analytic barrier formula averaged over the packet's momentum spectrum. Widen the barrier and watch T collapse – that exponential sensitivity is why alpha-decay half-lives span 40 orders of magnitude.

4.5Where this leaves us

The machine is complete. A wave of arrows (Chapter 2), odds from its strength (Chapter 3), and now the engine that drives it – notes, chords, and walls that leak. With these four chapters you can honestly say you know how quantum mechanics works. What’s left is what the world does with it: the strange two-valued compass inside every electron called spin, measurements that scramble each other, and – at the end of the road – the full quantum atom.

Next chapter
Chapter 5 – Spin & Measurement
The Bloch sphere, Stern–Gerlach chains, and why measuring one thing scrambles another.
Chapter 5 of 7