INGENIA

QNT-01

Particle in an infinite well

En = n² π² ħ² /(2 m L²), n = 1, 2, …

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Bound statesSchrödinger 1926

Governing equation

En=n2π222mL2E_n=\dfrac{n^2\pi^2\hbar^2}{2m L^2}

where

n
Quantum number ()
L
Well width (nm)
m
Mass (electron units) (m_e)
E_n
Energy (eV)

Lecture brief

Historical brief

Planck (1900), Einstein’s photoelectric law, Bohr, de Broglie, Heisenberg and Schrödinger’s 1926 equation rebuilt matter as amplitude. These sheets are the first solvable models: wells, spin, tunneling, uncertainty. This sheet (QNT-01 — Particle in an infinite well) is the form associated with Schrödinger 1926. Working symbols: nn, LL, mm \rightarrow EnE_n. Schrödinger's equation with ψ(0)=ψ(L)=0 has sinusoidal eigenfunctions whose energies scale as n²/L², the prototype bound spectrum.

Purpose

Purpose: compute EnE_n from nn, LL, mm in Quantum mechanics via En=n2π222mL2E_n=\dfrac{n^2\pi^2\hbar^2}{2m L^2} En = n² π² ħ² /(2 m L²), n = 1, 2, … Use it when a real quantum mechanics question must be answered in SI before a code check.

Live realistic example

In symbols

Live case. Given n=1.000n = 1.000\,\mathrm{—}, L=1.000nmL = 1.000\,\mathrm{nm}, m=1.000mem = 1.000\,\mathrm{m_e}, the governing relation En=n2π222mL2E_n=\dfrac{n^2\pi^2\hbar^2}{2m L^2} yields En=6.851e9eVE_n = 6.851e-9\,\mathrm{eV}. 1-D infinite walls, electron mass default via u = me if m=1. Move a slider: the numbers are this situation, not a canned story.

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Inputs

Outputs

  • Energy E_n0.0000 eV
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QNT-01 · quantum
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Narration of this film

1-D infinite walls, electron mass default via u = me if m=1.

Schrödinger's equation with ψ(0)=ψ(L)=0 has sinusoidal eigenfunctions whose energies scale as n²/L², the prototype bound spectrum.

Reading speed

Watch on YouTube