Hydrogen atom: quantum numbers (introductory) is a core Quantum Mechanics (UG Intro) concept in Physics. This guide explains what it is, walks through a fully worked example, and lists the key equations you need — with a short quiz to test yourself.

Key equations and worked example

Hydrogen (Z = 1) has one electron in the n = 1 shell. Bohr's model gives its energy levels Eₙ = −13.6/n² eV, so the ground state is −13.6 eV and the first excited state is −3.4 eV. Dropping from n = 2 to n = 1 emits a photon of 10.2 eV — the Lyman-alpha line. Helium (Z = 2) fills the first shell with 2 electrons; lithium (Z = 3) starts the second shell.

• <code>Bohr radius rₙ = n²·a₀ (a₀ ≈ 0.529 Å)</code>
• <code>Energy levels: Eₙ = −13.6·Z²/n² eV</code>
• <code>Photon emitted: ΔE = h·f = 13.6·Z²·(1/n₁² − 1/n₂²) eV</code>
• <code>Shell capacity: 2n² electrons</code>

Hydrogen atom: quantum numbers (introductory) in detail

Hydrogen atom: quantum numbers (introductory) is one of the central ideas in Quantum Mechanics (UG Intro), and it appears in Physics curricula under Wave mechanics. It is worth learning deeply because it connects to so many other topics in this section.

Bohr&#39;s model pictures electrons circling the nucleus in fixed shells of quantized angular momentum (mvr = n·h/2π), each shell holding at most 2n² electrons. It correctly predicts hydrogen&#39;s spectrum but is superseded by quantum mechanics, where &#39;orbits&#39; become probability clouds (orbitals). Still, shells explain the periodic table: elements in the same column have the same outer-shell electron count.

For exams, the pattern is predictable: first a definition or statement of the result, then a direct numerical application of one of the equations above, then a "why" question — why the formula takes that form, or what changes when a variable is doubled or halved. The worked example and quiz below cover exactly that progression.

Quick self-check:

• Q: How many electrons can the n = 2 shell hold?<br />A: 8 — capacity is 2n² = 2×4 = 8.
• Q: What photon is emitted when hydrogen&#39;s electron falls from n = 3 to n = 2?<br />A: ΔE = 13.6×(1/4 − 1/9) ≈ 1.89 eV — the red H-alpha line of the Balmer series.
• Q: Why don&#39;t orbiting electrons spiral into the nucleus in Bohr&#39;s model?<br />A: By postulate, electrons in allowed shells do not radiate; radiation happens only when jumping between shells.
• Q: Where does Bohr&#39;s model fail?<br />A: Multi-electron atoms, fine spectral structure, and the true probabilistic nature of orbitals — quantum mechanics replaces circular orbits with wavefunctions.