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Bounded modern-physics survey · Interactive lesson

The Bohr model and its failures

Bohr's model is the cheapest calculation in atomic physics that returns real numbers: put one quantum rule on a classical orbit and the hydrogen spectrum follows. Learn to run it, to test it by dimensions, Zα and correspondence, and to name the measurements it cannot survive: they are the brief the Schrödinger atom was written to meet.

UPIII-10.02 · Lesson 2 of 9 in this unit. Position is not a completion score.
Starting model: The Bohr model and its failuresLeft: a classical circular orbit of radius 3.00 a₀ about a nucleus of charge 1e, drawn to scale among the faint Bohr orbits n = 1 to 4. Right: one lap of its de Broglie wave, cut open and laid flat, lap 2 dashed; the dial compares the phase each lap starts with. The lap holds 1.73 wavelengths, so lap 2 starts 96° out of step.r = 3.00 a₀, Z = 12πr/λ = 1.73, so L = 1.73 ħeach lap's starting phaseone lap: s = 0 to 2πrphase mismatch per lap 96°solid lap 1, dashed lap 2faint rings: n = 1, 2, 3, 4
Start with a picture. Change the model in the lab below.

Bounded modern-physics survey. This modern-physics material is an introductory survey, not a complete course in relativity, quantum, atomic, nuclear or particle physics. Your university determines the required depth and assessment.

1

Build the model

One quantum rule on a classical orbit: the right energies from the wrong atom.

The key idea

The Bohr model treats a one-electron atom as an electron on a classical circular Coulomb orbit whose angular momentum is restricted to whole multiples of ħ, emitting or absorbing light only when it jumps between those orbits.

Example. In hydrogen the n = 2 orbit has r₂ = 4a₀ = 212 pm and E₂ = −13.6 eV/4 = −3.40 eV; dropping to n = 1 at −13.6 eV releases 10.2 eV, a 122 nm ultraviolet photon, the Lyman-α line.

The complete physical model and assumptions

Bohr kept almost all of classical physics — Newton's second law, Coulomb's force, a circular orbit — and added one rule that classical physics cannot supply: only orbits whose angular momentum is a whole multiple of ħ are allowed, and they do not radiate. Force balance and the rule are two equations in two unknowns, so each integer n fixes a radius rₙ = n²a₀/Z, a speed vₙ = Zαc/n and an energy Eₙ = −13.6 eV × Z²/n², and a photon of energy Eᵢ − Ef appears only when the electron jumps. The Rydberg constant then comes out of mₑ, e, ε₀ and h, right to a few parts in 10⁵ once the nucleus is allowed to recoil. De Broglie later gave the rule a reason: an allowed orbit holds a whole number of electron wavelengths. The model even passes its own tests — v/c = Zα/n is small for light atoms, and at large n the photon frequency tends to the classical orbital frequency — and still fails as a picture of the atom. It gives the ground state an angular momentum of ħ where measurement says zero, draws a flat atom where the real one is spherical, has no rule for two electrons, and predicts where lines sit but not how bright they are or how long states live. Its energies are right because in a 1/r potential the energy depends on n alone; its orbits are not.

1A classical orbit with one quantum rule

Classical physics alone allows every circular orbit. For an electron circling a nucleus of charge Ze, Newton's second law with Coulomb's force gives mₑ v²/r = Zke²/r², with k = 1/(4πε₀) = 8.99 × 10⁹ N m² C⁻². That is one equation in two unknowns, so r can take any value, the energy −Zke²/(2r) varies continuously, and the emitted spectrum should be continuous. The orbit is also unstable: an accelerating charge radiates, and the Larmor rate makes a classical orbit of radius 52.9 pm spiral into the proton in about 1.6 × 10⁻¹¹ s. Bohr's 1913 answer was three postulates that classical physics cannot supply. Certain orbits are stationary and do not radiate. They are the ones with angular momentum L = nħ. Light is emitted or absorbed only in a jump between two of them, with hf = Eᵢ − Ef. Nothing justifies the postulates except whether the numbers they produce match the spectrum.

2Two equations, three results

Put v = nħ/(mₑ r) from the rule into the force balance: mₑ n²ħ²/(mₑ² r³) = Zke²/r², so rₙ = n²ħ²/(Z mₑ ke²) = n²a₀/Z. Check the dimensions: (J s)² divided by kg × J m is J s² kg⁻¹ m⁻¹, and with J = kg m² s⁻² that is m. Put rₙ back into the rule and vₙ = Zke²/(nħ) = Zαc/n, which is 2.19 × 10⁶ m s⁻¹, or c/137, in hydrogen's ground state. For the energy, the force balance says K = ½mₑ v² = Zke²/(2r) while U = −Zke²/r, so E = K + U = −K = U/2, the virial theorem for an inverse-square force. Substituting rₙ gives Eₙ = −(mₑ k²e⁴/(2ħ²)) Z²/n² = −13.6 eV × Z²/n². Each power of Z has a source: r ∝ 1/Z because the pull is Z times stronger, v ∝ Z, and E ∝ Z² because the larger charge and the smaller radius both deepen the well.

3Why whole multiples of ħ: the de Broglie wave

Bohr stated L = nħ; de Broglie, in 1924, gave it a reason. An electron of momentum p carries a wavelength λ = h/p. Confine that wave to a circular track and it meets itself after one lap. If the circumference holds a whole number of wavelengths the wave returns in phase and reinforces itself; if not, each lap arrives shifted and the sum over many laps cancels. The condition 2πr = nλ = nh/(mₑ v) is exactly mₑ v r = nħ. Combined with the Coulomb force balance, a circular orbit of radius r holds N = √(Zr/a₀) wavelengths, so in hydrogen the orbits at a₀, 4a₀ and 9a₀ close with N = 1, 2 and 3, while one at 3a₀ holds 1.73 wavelengths and is forbidden. The argument explains the rule without proving it. It puts the electron wave on a one-dimensional line, but the real wave fills three dimensions: in the Schrödinger solution n − 1 counts radial and angular nodes together, and the ground state has no circulating wave at all.

4Testing the model against its own limits

Three checks decide whether a Bohr-model number can be trusted. First, the nucleus is not infinitely heavy: electron and nucleus both orbit their centre of mass, and the fix is to replace mₑ by the reduced mass μ = mₑ M/(mₑ + M). For hydrogen μ = 0.99946 mₑ, which moves every line by 0.054%; deuterium's μ is larger by 2.7 × 10⁻⁴, enough to shift Hα by 0.18 nm, which is how deuterium was found in 1932. Second, the speed ratio v/c = Zα/n must be small for a nonrelativistic model: 0.0073 in hydrogen, 0.60 for n = 1 in lead. Third, correspondence. The photon for n → n − 1 has f = (13.6 eV/h) Z²[1/(n − 1)² − 1/n²], and the classical orbital frequency is forb = v/(2πr) = Z²αc/(2πa₀n³). Their ratio n(2n − 1)/(2(n − 1)²) is 3 at n = 2 but 1.01 at n = 150, so jumps between neighbouring high orbits radiate at the classical frequency, as they must.

5Failure one: an orbit the ground state does not have

Bohr's ground state is a circular orbit with L = ħ. Measurement says the hydrogen ground state has zero orbital angular momentum: it carries no orbital magnetic moment, and its magnetism comes from electron spin, which the model does not contain. The orbit also lies in a plane, so a Bohr atom would be a flat disc with a preferred axis, while ground-state hydrogen is spherically symmetric. The uncertainty principle rules the orbit out. On the n = 1 orbit p = mₑ v = ħ/a₀; pinning the radius to within 10%, Δr = 0.1a₀, needs Δp ≥ ħ/(2Δr) = 5ħ/a₀, five times the momentum itself, so no definite trajectory of that size can exist. The energies survive because the Coulomb potential is special: its energy depends only on n = nᵣ + l + 1, one more than the total count of radial and angular nodes, so a model that counts n correctly gets Eₙ right whatever it says about l. For n = 1 the only possibility is l = 0.

6Failure two: more electrons, and anything beyond frequencies

Bohr's rule quantises one electron on one orbit. With two electrons it has no principle for arranging them, and the arrangements that can be computed miss: putting helium's two electrons on opposite sides of one ring overshoots the first ionisation energy by about 18%, as the Hard example shows, while He⁺, with one electron, comes out right. The model is also silent on everything but line positions. It gives frequencies but no intensities, no lifetimes and no selection rules. In hydrogen the 2p state decays to 1s in 1.6 ns, while 2s, the same Bohr orbit with the same energy, has no single-photon dipole route to 1s and lives about 0.12 s, nearly 10⁸ times longer. The model has one n = 2 state; nature has several, and a high-resolution spectrometer shows them: Hα resolves into fine-structure components spread over about 0.02 nm. Sommerfeld's elliptical orbits patched the fine structure. Nothing patched the rest.

2

Key equations

Read the units, assumptions and limits before substituting.

Bohr's quantisation rule

L = mₑ v r = nħ, n = 1, 2, 3, …

The only non-classical input. Paired with the force balance mₑ v²/r = Zke²/r², it gives two equations for two unknowns, so each n fixes exactly one orbit.

L in J s; ħ = h/2π = 1.055 × 10⁻³⁴ J s; mₑ = 9.109 × 10⁻³¹ kg; v in m s⁻¹, r in m; n a positive integer

Radius of the nth orbit

rₙ = n² a₀ / Z

Radii grow as n², so n = 10 in hydrogen already sits at 5.29 nm, and a nucleus of charge Ze pulls every orbit in by a factor Z.

a₀ = 4πε₀ħ²/(mₑ e²) = 52.9 pm, the Bohr radius; Z the nuclear charge number, dimensionless; rₙ in m

Speed on the nth orbit

vₙ = Zαc / n

v/c = Zα/n is the model's own validity test: 0.0073 in hydrogen's ground state, but 0.60 for n = 1 about a Z = 82 nucleus, where a nonrelativistic orbit is no longer safe.

α = e²/(4πε₀ħc) = 1/137.04, the fine-structure constant, dimensionless; c = 2.998 × 10⁸ m s⁻¹

Energy of the nth level

Eₙ = −(13.6 eV) Z²/n²

For a 1/r potential E = −K = U/2. Z enters twice, once through the nuclear charge and once through the radius shrinking as 1/Z, hence Z².

13.6 eV = mₑ e⁴/(2(4πε₀)²ħ²); for nuclear mass M put μ = mₑ M/(mₑ + M) for mₑ, giving 13.598 eV in hydrogen

De Broglie closure condition

2πrₙ = nλₙ, with λₙ = h/(mₑ vₙ)

A reason for the rule, not a proof: a wave confined to a circle must come back in phase after one lap. It treats the electron wave as one-dimensional, which the real atom is not.

λₙ the electron wavelength in m; h = 6.626 × 10⁻³⁴ J s. Multiplied out, it is mₑ vₙ rₙ = nħ again

Correspondence at large n

f(n → n − 1) → Z²αc / (2πa₀n³) = forb(n) as n → ∞

At large n a quantum jump must radiate like the classical orbit. The ratio is 3 at n = 2, 1.08 at n = 20 and 1.01 at n = 150, so Bohr's levels pass.

f in Hz; αc/(2πa₀) = 6.58 × 10¹⁵ Hz; the exact ratio f(n → n − 1)/forb(n) is n(2n − 1)/(2(n − 1)²)
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

3.00 a₀
0.25 to 16 a₀; steps of 0.25.
1
1 to 4; steps of 1.

Try this. Drag r from 3.00 to 4.00 a₀: the count climbs from 1.73 to exactly 2, the dashed lap and dashed arrow swing onto the solid ones, and the orbit lands on the n = 2 ring. Then set Z = 2: closure now comes at 2.00 a₀ and 4.50 a₀, the n = 2 and n = 3 orbits pulled in by a factor of two.

Live results

WAVELENGTHS PER LAP 2πr/λ
1.73
PHASE MISMATCH PER LAP
96 °
ORBIT ENERGY E
-4.53 eV
NEAREST BOHR RADIUS n²a₀/Z
4.00 a₀

Results follow this lesson’s model and assumptions. Displayed values are rounded.

Interactive Physics III modelLeft: a classical circular orbit of radius 3.00 a₀ about a nucleus of charge 1e, drawn to scale among the faint Bohr orbits n = 1 to 4. Right: one lap of its de Broglie wave, cut open and laid flat, lap 2 dashed; the dial compares the phase each lap starts with. The lap holds 1.73 wavelengths, so lap 2 starts 96° out of step.r = 3.00 a₀, Z = 12πr/λ = 1.73, so L = 1.73 ħeach lap's starting phaseone lap: s = 0 to 2πrphase mismatch per lap 96°solid lap 1, dashed lap 2faint rings: n = 1, 2, 3, 4
Left: a classical circular orbit of radius 3.00 a₀ about a nucleus of charge 1e, drawn to scale among the faint Bohr orbits n = 1 to 4. Right: one lap of its de Broglie wave, cut open and laid flat, lap 2 dashed; the dial compares the phase each lap starts with. The lap holds 1.73 wavelengths, so lap 2 starts 96° out of step.

Predict → change one variable → check

Plan a change before running it. Every other input stays at the saved baseline.

Saved baseline. Orbit radius r: 3.00 a₀; Nuclear charge Z: 1

Baseline 3.00; choose 0.25 to 16, in steps of 0.25.
4. Compared with the saved baseline, this result will…

This experiment is kept only while this page is open. It does not change saved course progress.

4

Catch the common trap

Because Bohr's energies match hydrogen's spectrum, students take the whole picture as true: the electron circles at exactly a₀ with angular momentum ħ, and n is its angular-momentum quantum number. Matching energies is not matching states. In the Schrödinger atom n fixes the energy but not the angular momentum, which is set by a separate number l = 0, 1, …, n − 1 with |L| = √(l(l + 1)) ħ, so the ground state has l = 0 and L = 0. Its electron has no orbit and no single radius: a₀ is only the most probable distance, and the mean is 1.5a₀. The energies coincide because in a 1/r potential E depends on n alone, and any model that counts n correctly gets E right. Use Bohr's Eₙ and rₙ as scales; do not read its orbits as the atom.

5

Practice & worked examples

3 authored examples. Make an attempt, then reveal the reasoning one step at a time.

EasyExample 1

Test de Broglie's rationale on hydrogen's n = 3 Bohr orbit: find the orbit radius and the electron's speed, compute its de Broglie wavelength, and count how many wavelengths fit around the orbit.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

MediumExample 2

A hydrogen atom in the n = 20 Bohr orbit drops to n = 19. Compare the frequency of the emitted photon with the electron's orbital frequency on the n = 20 and n = 19 orbits, and say what the comparison tests. Treat the proton as infinitely heavy.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

HardExample 3

The Bohr model gives He⁺ right: 54.42 eV to remove its one electron, as measured. Test it on neutral helium. Put both electrons on one n = 1 circular orbit, on opposite sides, each with L = ħ. Find the orbit radius, the total energy, and the predicted first ionisation energy, and compare with the measured 24.59 eV.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

6

Quick check

Select an answer and explain it before checking.

A He⁺ ion (Z = 2) has its electron in the Bohr orbit n = 2. How do its energy, speed, orbit radius and angular momentum compare with those of a hydrogen atom in its ground state?
7

Review & continue

The Bohr model treats a one-electron atom as an electron on a classical circular Coulomb orbit whose angular momentum is restricted to whole multiples of ħ, emitting or absorbing light only when it jumps between those orbits.

  • Explain the relationship without looking at the equation.
  • Check a sign, a unit and a model assumption in your working.
  • Return to the lab or worked example if a step is still unclear.

Optional supporting lessons

These chapter resources can help with earlier ideas; they are not additional required Physics III completion tasks.

Extra challenging questions

Connect several ideas, explore supplied data, and compare your reasoning with a worked solution.