A horizontal neutron-reflecting mirror supplies the lower boundary of a quantum bouncer, with the Earth's approximately linear gravitational potential above it. An absorber above the mirror removes neutrons with sufficient vertical extent. Scanning the mirror-absorber gap and counting transmitted neutrons probes the lowest allowed gravitational states. The 2002 work led by Valery V. Nesvizhevsky reported this confinement; a subsequent detailed report describes suppression below the lowest-state height.[ref][ref]
This is a count-versus-gap experiment, not a direct image of a wavefunction. Surface scattering, absorption and the incident vertical-motion distribution enter a quantitative transmission model.
The hard wall imposes , while the increasing linear potential requires decay as . Set
The stationary Schrödinger equation becomes . The growing Airy function solution is excluded, leaving
This is the quantum bouncer. For the first four states, . Their interior node counts are respectively zero, one, two and three. Each wavefunction starts at zero at the wall, oscillates in the classically allowed interval, and crosses smoothly into an exponentially decaying tail beyond the turning point . The turning point is not an extra hard wall: the wavefunction generally remains nonzero there and beyond it.
Figure 1.
The first four quantum-bouncer wavefunctions and their classical turning points
. Original normalized Airy-function calculation. The vertical dashed lines mark where the potential equals each energy; the decaying tail is retained. Details.