
Optional unit · institution-dependent · Interactive lesson
Blackbody radiation and Planck's quantum hypothesis
Blackbody radiation is where classical physics fails for a reason you can compute. We count the standing waves a hot cavity holds, watch equipartition give each one kT and demand infinite energy, then let Planck's steps of hν make the sum converge. You leave able to read hν/kT as the one number that says which physics a problem needs.
UPIII-09.01 · Lesson 1 of 9 in this unit. Position is not a completion score.Optional unit · institution-dependent. 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. Optional work is not a required completion gate.
Build the model
Count the modes, weight each by Boltzmann, and the infinity goes away.
The key idea
Planck's quantum hypothesis is that a cavity mode of frequency ν can hold energy only in whole steps of hν, so at temperature T its mean energy is hν/(e(hν/kT) − 1) rather than the classical kT.
Example. At 300 K, kT/h = 6.25 THz: a 2.45 GHz microwave mode has hν/kT = 3.9 × 10⁻⁴ and still holds 0.9998kT, while a 30 THz infrared mode has hν/kT = 4.80 and holds only 0.040kT.
The complete physical model and assumptions
A cavity in equilibrium with its walls fills with standing electromagnetic waves, and the spectrum of that radiation depends on temperature alone, not on what the walls are made of. The classical model has two factors, each defensible on its own: counting the allowed standing waves gives 8πν²/c³ modes per unit volume per unit frequency, growing without limit, and equipartition gives every mode the same mean energy kT. Their product, the Rayleigh–Jeans law, fits long-wavelength measurements and predicts infinite total energy. Planck kept the count and replaced the second factor: if a mode can hold energy only in whole steps of hν, the Boltzmann-weighted average becomes hν/(e(hν/kT) − 1). When hν ≪ kT the steps blur into a continuum and the average returns to kT; when hν ≫ kT even one step is improbable and the mode freezes out exponentially, which cuts off the ultraviolet. The resulting spectrum has a single shape in x = hν/kT, from which Wien's displacement follows by differentiation and the T⁴ law by integration. The model assumes equilibrium and a cavity much larger than the wavelengths, so the modes form a continuum. A surface emits this spectrum only if it absorbs perfectly, as the small hole into such a cavity does; real surfaces emit less, by an emissivity factor. It quantises the energy a mode can hold. Whether light itself arrives in lumps is a separate claim, and the photoelectric evidence in the next topic is what forces it.
1Count the standing waves the cavity can hold
Inside a cubical cavity of side L with conducting walls, each field component obeys the wave equation ∂²E/∂x² + ∂²E/∂y² + ∂²E/∂z² = (1/c²) ∂²E/∂t², and the walls allow only standing waves with wave vector k = (π/L)(nₓ, ny, nz) for whole numbers n. Since ω = ck, a mode's frequency is ν = (c/2L)√(nₓ² + ny² + nz²). Counting the modes below ν is counting lattice points inside one octant of a sphere of radius R = 2Lν/c: N(ν) = 2 × (1/8)(4π/3)R³ = 8πVν³/(3c³), where the 2 counts the two polarisations of a transverse wave. Differentiate and divide by V to get g(ν) = 8πν²/c³ modes per unit volume per unit frequency. The count is enormous: a 1 cm³ cavity holds about 2.3 × 10¹¹ modes in every 1 THz band near 500 THz, so a smooth density is safe, and the cavity's shape drops out once L ≫ λ.
2Equipartition hands every mode kT
Each mode is a harmonic oscillator: its energy passes back and forth between electric and magnetic fields as a spring's does between kinetic and potential. Classical statistical mechanics gives any oscillator in equilibrium a mean energy kT, half from each quadratic term, whatever its frequency. Multiply by the mode density and you have the Rayleigh–Jeans law, uRJ = 8πν²kT/c³. It fits measured spectra at long wavelengths and contains no h at all. Its integral over frequency, though, grows as ν³ without bound. Stopping at 750 THz, the violet end of the visible, a cavity at 300 K would already hold 0.54 J m⁻³, about 9 × 10⁴ times the 6.1 × 10⁻⁶ J m⁻³ actually present, and every higher band adds more. A classical cavity could never reach equilibrium: its walls would keep pouring energy into ever-shorter waves. This is the ultraviolet catastrophe, and it is a failure of kT per mode, not of the counting.
3Planck's steps and the Boltzmann average
Planck kept the mode count and changed one assumption: a mode of frequency ν can hold only Eₙ = nhν, with n = 0, 1, 2, … and h = 6.626 × 10⁻³⁴ J s. In equilibrium level n has Boltzmann weight e(−nx), with x = hν/kT. The geometric series Z = Σ e(−nx) = 1/(1 − e(−x)) normalises the probabilities to Pₙ = (1 − e(−x)) e(−nx), and the mean energy is ⟨E⟩ = Σ nhν Pₙ, or more compactly −∂(ln Z)/∂β with β = 1/kT. Either route gives ⟨E⟩ = hν/(eˣ − 1). Now put numbers in. At 300 K a mode at 30 THz has x = 4.80: it sits in its ground state 99.2% of the time, its mean occupation is 0.0083 steps, and ⟨E⟩ = 0.040kT. Reaching even the first level costs 4.8kT, which the Boltzmann factor makes exponentially rare, so high-frequency modes freeze out instead of each claiming kT.
4Unresolvable steps return the classical answer
The correspondence check is an expansion. For x = hν/kT ≪ 1, eˣ − 1 = x + x²/2 + x³/6 + …, so ⟨E⟩ = kT(1 − x/2 + x²/12 − …): at x = 0.01 a mode holds 0.995kT, and at x = 0.1 still 0.951kT. When a step is a small fraction of kT the ladder cannot be told from a continuum, and Planck's law collapses onto Rayleigh–Jeans; letting h → 0 at fixed ν does the same formally. The crossover sits at ν = kT/h, which is 2.08 × 10¹⁰ Hz for every kelvin of temperature: 6.25 THz, a wavelength of 48 μm, at 300 K. A 2.45 GHz microwave mode at room temperature has x = 3.9 × 10⁻⁴ and is thoroughly classical; a 540 THz green-light mode has x ≈ 86 and is frozen solid. What separates the regimes is this ratio, not whether the light is ultraviolet and not the size of the cavity. In the opposite limit, x ≫ 1, ⟨E⟩ ≈ hν e(−x), which is Wien's earlier approximation.
5One universal curve, one peak
Mode density times mean energy is Planck's distribution, u(ν, T) = (8πhν³/c³)/(e(hν/kT) − 1), in J m⁻³ Hz⁻¹. Written in x it becomes (8πk³T³/(h²c³)) x³/(eˣ − 1), so every temperature shares one shape and the peak sits at a fixed x. Setting d/dx[x³/(eˣ − 1)] = 0 gives 3(1 − e(−x)) = x, which has no closed-form root; iterating x → 3(1 − e(−x)) from x = 3 gives 2.851, 2.827, 2.822 and settles at 2.821. So hνₚₑₐₖ = 2.821kT, or νₚₑₐₖ = (5.879 × 10¹⁰ Hz K⁻¹) × T: double the temperature and the peak moves to twice the frequency while its height grows eightfold, as T³. Per unit wavelength the same algebra gives 5(1 − e(−x)) = x, with root 4.965, and λₘₐₓ T = hc/(4.965k) = 2.898 × 10⁻³ m K, the Wien displacement law in its familiar form.
6Integrate the curve for the fourth-power law
The total energy density is the area under the curve. Substituting ν = kTx/h, U/V = (8πk⁴T⁴/(h³c³)) ∫ from 0 to ∞ of x³/(eˣ − 1) dx, and the dimensionless integral is π⁴/15 = 6.494. So U/V = aT⁴ with a = 8π⁵k⁴/(15h³c³) = 7.566 × 10⁻¹⁶ J m⁻³ K⁻⁴. Radiation leaking from a small hole carries flux (c/4)(U/V), the 1/4 from averaging the isotropic flow over directions, so the exitance is M = σT⁴ with σ = 5.670 × 10⁻⁸ W m⁻² K⁻⁴. Dimensions: k⁴T⁴/(h³c²) is J⁴ ÷ (J³ s³ × m² s⁻²) = J s⁻¹ m⁻², a power per area. Limit: σ ∝ h⁻³, so h → 0 sends the total to infinity and the catastrophe returns. Data: the Sun's photosphere at 5772 K gives M = 6.29 × 10⁷ W m⁻², and multiplying by 4πR² with R = 6.96 × 10⁸ m gives 3.83 × 10²⁶ W, the measured solar luminosity.
Key equations
Read the units, assumptions and limits before substituting.
Cavity mode density
g(ν) = 8πν²/c³
Counting standing waves in one octant of k-space. It holds for any cavity shape once the cavity is much larger than λ.
g in modes per m³ per Hz (s m⁻³); ν in Hz; c = 3.00 × 10⁸ m s⁻¹; both polarisations countedRayleigh–Jeans law
uRJ(ν, T) = 8πν²kT/c³
The mode density times equipartition's kT. Correct when hν ≪ kT, but its integral over ν grows as ν³ without bound: the ultraviolet catastrophe.
u in J m⁻³ Hz⁻¹; k = 1.381 × 10⁻²³ J K⁻¹; T in K; no h appearsPlanck's mean energy per mode
⟨E⟩ = hν/(e(hν/kT) − 1)
The Boltzmann average over the ladder Eₙ = nhν. It tends to kT when hν ≪ kT and to hν e(−hν/kT) when hν ≫ kT.
h = 6.626 × 10⁻³⁴ J s; ⟨E⟩ in J; the ratio hν/kT is dimensionlessPlanck distribution
u(ν, T) = (8πhν³/c³)/(e(hν/kT) − 1)
In x = hν/kT it reads (8πk³T³/(h²c³)) x³/(eˣ − 1): one universal shape, stretched along ν by T and in height by T³.
u in J m⁻³ Hz⁻¹ (equivalently J s m⁻³); it is the product g(ν)⟨E⟩Wien displacement law
λₘₐₓ T = hc/(4.965k) = 2.898 × 10⁻³ m K
A 5772 K photosphere peaks at 502 nm per unit wavelength; a 300 K wall peaks near 9.7 μm, which is why thermal cameras work in the 8 to 14 μm band.
λₘₐₓ in m is the peak of the spectrum per unit wavelength; per unit frequency the peak is at hν = 2.821kT insteadStefan–Boltzmann law
M = σT⁴, with σ = 2π⁵k⁴/(15h³c²)
The area under Planck's curve, using ∫ from 0 to ∞ of x³/(eˣ − 1) dx = π⁴/15, times c/4. Since σ ∝ h⁻³, the classical limit h → 0 gives infinite power.
M is the power per unit area leaving a blackbody surface, in W m⁻²; σ = 5.670 × 10⁻⁸ W m⁻² K⁻⁴Interactive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. At 5800 K drag ν from 20 THz to 1000 THz: the mode's share of kT falls from 0.92 to 0.002 as hν/kT passes 1, and that freeze-out keeps the solid curve finite while the dashed one leaves the top. Then take T from 6000 K to 3000 K: the peak halves in frequency and drops to an eighth of its height.
Live results
- hν/kT AT THE MARKER
- 4.47
- ⟨E⟩ PER MODE ÷ kT
- 0.052
- PEAK ν = 2.821kT/h
- 341 THz
- EXITANCE σT⁴
- 64.2 MW m⁻²
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Cavity temperature T: 5800 K; Marker frequency ν: 540 THz
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
The commonest slip is to treat the peak as a fixed feature of the radiation that survives a change of axis: take Wien's λₘₐₓ = b/T, convert it with ν = c/λₘₐₓ, and call the result the peak frequency. For the Sun at 5772 K that gives 5.97 × 10¹⁴ Hz, but the spectrum per unit frequency actually peaks at 2.821kT/h = 3.39 × 10¹⁴ Hz, whose wavelength is 883 nm, not 502 nm. The reason is that uν and uλ are densities, energy per unit frequency interval and per unit wavelength interval, and a density changes when you change variable: uλ = uν |dν/dλ| = uν c/λ², a factor that favours short wavelengths and moves the maximum. What is invariant is the energy in a band, ∫uν dν = ∫uλ dλ over the same band, so totals and band fractions are physical while the location of the peak depends on the axis you chose.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
A ceramic infrared heater panel, 0.30 m by 0.40 m, radiates from one face as a blackbody at 750 K. Find the wavelength at which its spectrum per unit wavelength peaks, the frequency at which its spectrum per unit frequency peaks, and the power the face radiates.
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.
- Wien in wavelength form: λₘₐₓ = b/T = (2.898 × 10⁻³ m K)/(750 K) = 3.86 × 10⁻⁶ m = 3.86 μm, in the mid-infrared.
- Per unit frequency the peak sits at hν = 2.821kT: νₚₑₐₖ = (5.879 × 10¹⁰ Hz K⁻¹)(750 K) = 4.41 × 10¹³ Hz = 44.1 THz.
- Check the trap: c/νₚₑₐₖ = (3.00 × 10⁸ m s⁻¹)/(4.41 × 10¹³ Hz) = 6.80 μm, 1.76 times λₘₐₓ. The two peaks are different points of one spectrum, because uν and uλ are densities over different variables.
- Stefan–Boltzmann: T⁴ = (750 K)⁴ = 3.164 × 10¹¹ K⁴, so M = σT⁴ = (5.670 × 10⁻⁸ W m⁻² K⁻⁴)(3.164 × 10¹¹ K⁴) = 1.79 × 10⁴ W m⁻².
- The face has A = 0.30 m × 0.40 m = 0.12 m², so P = MA = 2.15 × 10³ W. Absorption from a 293 K room trims this by only about 2%, because (293/750)⁴ = 0.023.
Answer. λₘₐₓ = 3.86 μm; νₚₑₐₖ = 44.1 THz (c/νₚₑₐₖ = 6.80 μm, not 3.86 μm); P ≈ 2.2 kW radiated from the face.
MediumExample 2
The cosmic microwave background is blackbody radiation at 2.725 K. A radio survey converts measured intensity into temperature using the Rayleigh–Jeans law. By what percentage does that law overestimate the spectral energy density at 1.4 GHz and at 30 GHz, and above roughly what frequency does the overestimate pass 10%?
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.
- The mode density is common to both laws, so their ratio is the ratio of mean energies per mode: uRJ/u = kT/⟨E⟩ = (eˣ − 1)/x, with x = hν/kT.
- Frequency scale: kT/h = (k/h)T = (2.0837 × 10¹⁰ Hz K⁻¹)(2.725 K) = 5.678 × 10¹⁰ Hz = 56.78 GHz.
- At 1.4 GHz, x = 1.4/56.78 = 0.02466, and (eˣ − 1)/x − 1 ≈ x/2 + x²/6 = 0.0124: a 1.24% overestimate, which is why radio work can quote intensities as Rayleigh–Jeans brightness temperatures.
- At 30 GHz, x = 30/56.78 = 0.5284. The two-term expansion is no longer good enough, so compute exactly: (e(0.5284) − 1)/0.5284 = 0.6962/0.5284 = 1.318, a 31.8% overestimate. The leading term x/2 alone would have said 26%.
- For a 10% overestimate, solve x/2 + x²/6 = 0.10: x = 3[−0.5 + √(0.25 + 0.0667)] = 0.188. The exact condition (eˣ − 1)/x = 1.10 also gives x = 0.188, so ν = 0.188 × 56.78 GHz = 10.7 GHz.
Answer. Overestimates of 1.2% at 1.4 GHz and 32% at 30 GHz; the error passes 10% near 10.7 GHz, where hν ≈ 0.19kT.
HardExample 3
A tungsten filament is modelled as a blackbody at 2700 K. Using the Planck distribution, estimate the fraction of its radiated power that falls in the visible band from 400 THz to 750 THz. Justify any approximation you make.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- The fraction in a band is that band's share of the area under u(ν, T). With x = hν/kT the constants cancel against the Stefan–Boltzmann integral, so the fraction above ν₁ is F(x₁) = (15/π⁴) ∫ from x₁ to ∞ of x³/(eˣ − 1) dx.
- Scale: kT/h = (2.0837 × 10¹⁰ Hz K⁻¹)(2700 K) = 56.26 THz, so the band edges sit at x₁ = 400/56.26 = 7.110 and x₂ = 750/56.26 = 13.33. Both are much greater than 1.
- For x ≫ 1, 1/(eˣ − 1) = e(−x)(1 + e(−x) + …), and e(−7.110) = 8.17 × 10⁻⁴, so keeping only the first term (the Wien limit) changes the answer by about 0.03%, far less than the error in calling tungsten a blackbody.
- Integrating by parts three times: ∫ from x₁ to ∞ of x³e(−x) dx = e(−x₁)(x₁³ + 3x₁² + 6x₁ + 6). At x₁ = 7.110 this is (8.17 × 10⁻⁴)(559.7) = 0.4573; at x₂ = 13.33 it is (1.623 × 10⁻⁶)(2988) = 0.00485.
- Divide by π⁴/15 = 6.494: F(x₁) = 0.0704 and F(x₂) = 0.00075, so the visible band holds 0.0704 − 0.0007 = 0.0697. A direct numerical integration of the full Planck form also gives 0.0697.
- Sense check: the peak is at 2.821 × 56.26 THz = 159 THz per unit frequency, and at b/T = 1.07 μm per unit wavelength; on either axis it lies in the infrared, beyond the 400 THz (750 nm) red edge, so a small visible share is expected. About 93% of the output lies below 400 THz.
Answer. About 7.0% (0.0697) of the filament's radiated power is visible; about 93% is infrared below 400 THz.
Quick check
Select an answer and explain it before checking.
Review & continue
Planck's quantum hypothesis is that a cavity mode of frequency ν can hold energy only in whole steps of hν, so at temperature T its mean energy is hν/(e(hν/kT) − 1) rather than the classical kT.
- 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.