Research explained · · Deep Quantum Science

Perturbation theory explained like you’re 10

Tiny magnets on a bumpy road: how physicists estimate energies when the exact problem is too hard, step by step and with real numbers.

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Most quantum problems cannot be solved exactly. Perturbation theory is the art of starting from an easy problem and adding small corrections, one at a time. Here is the idea, using the disordered spin chain from our paper.

The easy world: nobody moves

Take a row of six tiny magnets, each sitting on a random magnetic field (a "bump" in the road), with neighbours that feel each other. If the magnets cannot swap places, every arrangement has one fixed energy: a step on a ladder. With two magnets pointing down there are 15 arrangements, and we can compute every step exactly.

Frozen arrangements and their energy ladder
The unperturbed problem: each frozen arrangement is a step on an energy ladder.

Small hops

Now neighbouring up and down magnets may swap, with a small strength J. Draw each arrangement as a dot and each possible swap as a link: from any dot you can only hop to a few neighbouring dots. Because J is small, the system mostly stays home and only peeks next door.

The recipe

  1. Step 0 is the height of your own ladder step.
  2. Step 1 is zero. After a single hop you are somewhere else, and only trips that come back home change the energy.
  3. Step 2: go and come back. Each neighbour m gives a push |Vnm|² / (En − Em). Far-away energies barely matter; close energies matter a lot. Levels repel each other.
Second-order correction: hop to a neighbour and back
Second order: hop and come back. Here all neighbours sit higher and push the level down.

A chessboard trick

Colour the arrangements like a chessboard. Every hop changes the colour (the graph is bipartite), so after an odd number of hops you can never be home. Steps 1 and 3 vanish exactly, and two simple terms already give the energy with an error of order J4.

Does it work?

We compared the two-term recipe with exact diagonalisation. The largest error over all 15 levels is 0.0005 at J = 0.2 and 0.0068 at J = 0.4: doubling J multiplies the error by about 16, exactly the J4 we predicted. For large J the recipe breaks down, as expected for a small-J theory.

Exact energies versus perturbation theory as a function of J
Exact energies (green) and the two-term recipe (yellow, dashed), with the error growing as J4.
Why it matters: the same hop-and-return picture explains when strong disorder traps a quantum system near its starting point, the physics of many-body localisation.
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