• Pixel-art sticker of Tunnelia, personifying Quantum Tunnelling, with the caption “Walls Are Suggestions.”

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Tunnelia

Quantum Tunnelling Physics

\[T \approx e^{-2\kappa L}\]
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Meet Tunnelia, a quantum particle for whom walls are suggestions: she can cross a barrier she classically could not climb. Inside the barrier her wavefunction decays exponentially, so a thin enough wall lets a smaller wave of the same wavelength through. Pixel-art kiss-cut sticker in 2, 3, 4 and 6 inches; equation, symbols and sources in the physics panel below.

Size
Surface

Flat $6 shipping worldwideMade to order, ships in 2–5 business days

Details

Size3″ × 3″

3″ × 3″ kiss-cut sticker.

Shipping

Flat $6 shipping on every order, worldwide, whatever's in it.

Delivery times & where we ship

Returns & replacements21 days

Every item is printed to order, so we can’t accept returns or exchanges for change of mind, or if you ordered the wrong size or colour.

Print defect, misprint, damage or the wrong item? We’ll send a free replacement, or a refund if you prefer. Report it within 21 days of delivery with a photo; no need to send it back.

Full refund & replacement policy

The physics

Meet Tunnelia, a quantum particle who gets through walls she could never climb.

In classical physics a ball with energy E cannot cross a hill of height V > E. In quantum mechanics a particle is a wave, and a wave hitting a barrier does not stop dead. Inside the barrier it decays exponentially, falling off with the decay constant κ = √(2m(V − E))/ħ. If the barrier is thin enough, some of the wave is still there on the far side, and the particle has a chance of turning up there. For a thick barrier that chance is roughly e^(−2κL).

Because the dependence is exponential, small changes matter enormously. Doubling the barrier width squares the already small transmission, and heavier particles tunnel far less than light ones like electrons.

Tunnelling is not a curiosity. It explains alpha decay of nuclei, lets the scanning tunnelling microscope image single atoms, and is how flash memory stores and erases charge. In the Sun's core it helps protons get close enough to fuse.

The e^(−2κL) form is an approximation for wide barriers; exact results include a prefactor and depend on the barrier's shape.

Equations

\[T \approx e^{-2\kappa L}\]
\[\kappa=\frac{\sqrt{2m(V-E)}}{\hbar}\]
Symbols
SymbolMeaningUnit
\(T\) transmission probability (thick-barrier approximation) —
\(\kappa\) decay constant inside the barrier \(\mathrm{m⁻¹}\)
\(L\) barrier width \(\mathrm{m}\)
\(m\) mass of the particle \(\mathrm{kg}\)
\(V\) barrier height (potential energy) \(\mathrm{J}\)
\(E\) energy of the particle (E < V) \(\mathrm{J}\)
\(\hbar\) reduced Planck constant \(\mathrm{J·s}\)