CND-13
Einstein solid heat capacity
C_V = 3 N k_B (θ_E/T)² e^{θ_E/T} / (e^{θ_E/T}−1)². Independent oscillators.
Governing equation
where
- \theta_E
- Einstein temperature (K)
- T
- Temperature (K)
- n
- Amount (mol)
- C_V
- Heat capacity (J/K)
The figure, part by part
Each numbered marker wears the color of its card. Hover a card to light the marker. Tap a marker to jump to that card. The slider walks a red point along the curve; Animate drawing traces it like a pen.
Governing law — red
Domain of the variable — blue
Response curve — green
Rate of change — amber
Lecture brief
Historical brief
Drude electrons, Bloch waves, BCS pairing (1957) and Wiedemann–Franz heat are the first solids-and-metals laws. The lab is conductivity, gap and phonon heat in closed form. This sheet (CND-13 — Einstein solid heat capacity) is the form associated with Einstein solid. Working symbols: , , . Einstein (1907) explained why C_V vanishes as T → 0, before Debye's T³.
Purpose
Live realistic example
In symbols
Calculator
Inputs
Outputs
- Heat capacity C_V15.187 J/K
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Free library
Full libraryFree PDF / open book
- University Physics Vol. 3 (optics, modern)OpenStax · CC BY · Free PDF / open book
- College Physics 2eOpenStax · CC BY · Free PDF / open book
- LibreTexts PhysicsLibreTexts · CC · Free PDF / open book
- SI Brochure (BIPM)BIPM · Free PDF / open book
YouTube channels
Narration of this film
A grid of oscillators, a saturating C.
Einstein (1907) explained why C_V vanishes as T → 0, before Debye's T³.
Watch on YouTube