Quantum tunneling is a quantum mechanical phenomenon where particles pass through energy barriers.Imagine you're rolling a ball over a hill, but it miraculously appears on the other side without even climbing over the top. For microscopic particles, this is routine – it's called quantum tunneling.
The first theoretical explanation of tunneling was given in 1928 independently by George Gamow, and also by Ronald Gurney and Edward Condon for alpha decay of nuclei. Subsequently, the phenomenon was applied in solid-state physics: Leo Esaki in 1958 created the tunnel diode, for which he received the Nobel Prize. In astrophysics, tunneling explained the mechanism of stellar nucleosynthesis (Hans Bethe, 1938). Later, Stephen Hawking used the concept of tunneling to describe black hole radiation.
Within nonrelativistic quantum mechanics, tunneling is described by solving the stationary Schrödinger equation for a potential with a barrier. The wavefunction inside the barrier (E < V₀) has the form ψ(x) ∝ e^{-κx}, where κ = √(2m(V₀−E))/ħ. The transmission coefficient (tunneling probability) for a rectangular barrier of width L: T ≈ e^{-2κL}. The Heisenberg uncertainty principle allows a temporary violation of energy conservation, making tunneling possible. This effect is also used to explain the cosmological birth of the Universe and Hawking radiation.
Quantum tunneling is like walking through a wall without breaking it. Electrons do this constantly in microchips, seeping through barriers.
| T | variable | tunneling probability — transmission probability |
| z1 | variable | left turning point of the barrier — position metre |
| z2 | variable | right turning point of the barrier — position metre |
| m | variable | mass of the tunneling particle — mass kilogram |
| V | variable | potential energy as a function of position — potential energy joule |
| E | variable | energy of the particle — energy joule |
| ħ | constant | fundamental quantum of action divided by 2π — reduced planck constant = 1.054571817e-34 joule second |
| ∫ | operator | sums the integrand over the interval — integral |
| √ | operator | takes the non-negative root — square root |
| exp | operator | raises e to the given power — exponential |
| \Gamma | variable | Tunneling rate (probability per unit time) — rate per second |
| S | variable | Euclidean action of the bounce solution — action joule second |
| \propto | operator | Indicates proportionality — proportional to |
| e^{-S} | operator | Exponential function with exponent -S — exponential |
























