Quantum Physics

Bohr Model

Electrons orbit the nucleus in discrete energy levels — first step toward quantum mechanics

The Bohr model (1913) pictures the atom as a tiny solar system — electrons in discrete circular orbits around the nucleus. Each orbit corresponds to a specific energy. Electrons jump between orbits by absorbing or emitting photons of exactly the right energy. Successfully explained hydrogen's emission spectrum (Balmer, Lyman, Paschen series). Replaced by full quantum mechanics in 1920s but introduced quantization concept.

  • Quantized angular momentumL = n·ℏ (n = 1, 2, 3...)
  • Energy levelsE_n = -13.6/n² eV (for hydrogen)
  • Bohr radiusa_0 = 5.29 × 10⁻¹¹ m (n=1 for H)
  • Photon emissionhf = E_n_initial - E_n_final
  • SuccessesExplained H emission (Balmer, Lyman series)
  • LimitationsDoesn't work for multi-electron atoms; replaced by Schrödinger

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Bohr's postulates

Niels Bohr (1913) proposed three radical ideas:

  1. Stationary states. Electrons orbit in specific allowed circular orbits without radiating energy. Classical physics says they should — Bohr declared they don't.
  2. Quantization of angular momentum. Allowed orbits have L = mvr = nℏ, where n = 1, 2, 3, ...
  3. Photon emission. When electron jumps from orbit n_initial to n_final (lower), photon emitted with energy E = hf = E_initial − E_final.

Derived results for hydrogen

Combining quantization with classical mechanics for circular orbits:

QuantityFormulan=1 value
Orbital radiusr_n = n²·a_00.529 × 10⁻¹⁰ m
Bohr radius (constant)a_0 = ε₀h²/(πm·e²)0.529 × 10⁻¹⁰ m
EnergyE_n = -13.6/n² eV-13.6 eV
Velocityv_n = (e²/2ε₀h)/n2.19 × 10⁶ m/s (n=1)
PeriodT_n = 2π·a_0·n³ / v_11.5 × 10⁻¹⁶ s

Hydrogen emission spectrum

Photon emitted from transition n_i → n_f (i > f):

E_photon = E_i - E_f = -13.6 · (1/n_i² - 1/n_f²) eV (for emission)
        = 13.6 · (1/n_f² - 1/n_i²) eV (positive, emitted)

This is the Rydberg formula rewritten.

Seriesn_fRange
Lyman1UV
Balmer2Visible (656, 486, 434, 410 nm)
Paschen3Near IR
Brackett4IR
Pfund5IR

JavaScript — Bohr model calculations

// Bohr radius and energy levels
const a_0 = 5.29e-11;  // m
const E_1 = -13.6;     // eV (hydrogen ground state)

function bohrRadius(n, Z = 1) {
  return n * n * a_0 / Z;  // m
}

function bohrEnergy(n, Z = 1) {
  return E_1 * Z * Z / (n * n);  // eV
}

console.log(`H n=1: r = ${(bohrRadius(1) * 1e10).toFixed(2)} Å, E = ${bohrEnergy(1).toFixed(2)} eV`);
console.log(`H n=2: r = ${(bohrRadius(2) * 1e10).toFixed(2)} Å, E = ${bohrEnergy(2).toFixed(2)} eV`);
console.log(`H n=3: r = ${(bohrRadius(3) * 1e10).toFixed(2)} Å, E = ${bohrEnergy(3).toFixed(2)} eV`);

// Photon energy from transition
function transitionEnergy(n_i, n_f, Z = 1) {
  // Returns positive value (emitted photon)
  return Math.abs(bohrEnergy(n_i, Z) - bohrEnergy(n_f, Z));
}

// Photon wavelength from energy (E in eV → λ in nm)
function eVtoNm(E_eV) {
  return 1240 / E_eV;
}

// Balmer series (n_f = 2)
console.log('Balmer series:');
[3, 4, 5, 6].forEach(n_i => {
  const E = transitionEnergy(n_i, 2);
  console.log(`  ${n_i}→2: ${E.toFixed(2)} eV = ${eVtoNm(E).toFixed(0)} nm`);
});

// Hα (3→2) should be 656 nm — visible red
// H ionization energy
const E_ion_H = 13.6;
console.log(`H ionization: ${E_ion_H} eV`);

// Helium+ (Z=2)
console.log(`He+ n=1: ${bohrEnergy(1, 2)} eV`);  // -54.4

// Velocity in nth orbit
function bohrVelocity(n, Z = 1) {
  return 2.19e6 * Z / n;  // m/s
}

console.log(`H ground state v: ${bohrVelocity(1).toExponential(2)} m/s`);
// 0.7% of c — non-relativistic but close

Where Bohr model applies

  • Hydrogen and hydrogen-like atoms. H, He⁺, Li²⁺ — single electron systems. Bohr formula works exactly (small relativistic and QED corrections).
  • Education. Intuitive intro to atomic physics; pictures quantization, transitions, level diagrams.
  • Astrophysics. Hydrogen lines (e.g., 21 cm H I, Lyman-α at 121 nm) used to map gas in galaxies.
  • Spectroscopy basics. Most atomic spectra teaching starts with Bohr.
  • Plasma physics. Hydrogen plasma analysis, Stark effect, Zeeman effect — Bohr framework as starting point.
  • Quantum mechanics history. Bohr atom was bridge between classical and quantum — key historical step.
  • Atomic clocks. Cesium clock uses transitions; Bohr-style energy level analysis (with full QM corrections).

Common mistakes

  • Treating Bohr orbits as classical. Quantum mechanics replaces orbits with probability distributions (orbitals). Bohr model is a simplification.
  • Applying to multi-electron atoms. Bohr fails for atoms with electron-electron interactions. Use Hartree-Fock or DFT for multi-electron systems.
  • Forgetting Z dependence. Bohr formulas have Z² scaling. He⁺ has 4× the binding energy of H; Li²⁺ has 9×.
  • Using only ground state. Excited states (n > 1) are equally important for transitions and excited-atom spectroscopy.
  • Confusing Bohr radius with nuclear radius. Bohr radius (5.29e-11 m) = electron orbit. Nuclear radius (~10⁻¹⁵ m) is 100,000× smaller.
  • Believing electrons orbit like planets. Bohr model has classical picture but quantum reality is fuzzy probability cloud. Modern picture: orbitals, not orbits.

Frequently asked questions

How did Bohr's model break with classical physics?

Classically, accelerating electron should radiate continuously and spiral into nucleus. Bohr postulated that electrons in certain "stationary states" (specific orbits) DON'T radiate. They radiate only when jumping between orbits. This was ad hoc but matched experiments. Quantization of angular momentum (L = nℏ) was the key new postulate.

How does the model explain hydrogen's emission spectrum?

Hydrogen emits at specific wavelengths (Balmer series visible: 656, 486, 434 nm). Bohr predicted: λ from transitions n_i → n_f, with energies E_n = -13.6/n² eV. Balmer (visible) — transitions to n=2. Lyman (UV) — to n=1. Paschen (IR) — to n=3. Predicted wavelengths matched experiment perfectly for hydrogen.

Why doesn't Bohr's model work for multi-electron atoms?

Bohr model treats electron as single particle in central Coulomb field. For multi-electron atoms, electron-electron interactions matter — can't be reduced to simple central potential. Need full quantum mechanics with proper electron-electron correlation. Bohr works for hydrogen-like (single electron) systems: H, He⁺, Li²⁺, etc.

What's quantization of angular momentum?

Bohr postulated L = nℏ for allowed orbits. n is "principal quantum number." Combined with classical mechanics for circular orbits, this gives discrete radii and energies. Modern QM has L² = ℓ(ℓ+1)ℏ² with ℓ ∈ {0, 1, ..., n-1} — different but reduces to Bohr in limit. Also explains Pauli exclusion via spin.

What's the Bohr radius?

a_0 = 5.29 × 10⁻¹¹ m = 0.529 Å. Size of hydrogen atom in ground state (n=1). Higher n gives larger orbit (a_n = n²·a_0). Used as natural length unit in atomic physics. Bohr's value still used in modern QM (it's the most probable distance for ground state electron in actual quantum picture).

How was the Rydberg formula related?

Rydberg (1888) had empirically: 1/λ = R(1/n_f² - 1/n_i²). Bohr derived this from his model: R = m·e⁴/(8·ε₀²·h³·c) ≈ 1.097 × 10⁷ /m (Rydberg constant). Bohr's success: theoretical derivation of this empirical formula. Implied his model captured something real.

Why is the Bohr model still taught?

Despite being incomplete, it's intuitive — pictures atom as solar system, easy to visualize. Captures key physics: quantization, photon emission via transitions, energy level structure. Useful pedagogical bridge to quantum mechanics. Real atomic physics needs Schrödinger's equation, but Bohr provides building blocks.