/* ================= EQUATION STYLE ================= */
Logo DMS Learning

Einstein Theory of Specific Heat of Solids

Failure of Classical Theory

Classical theory (Dulong–Petit law) predicts:

\[ C_V = 3Nk_B \]

This agrees at high temperature but fails at low temperature where experimental results show $C_V \to 0$ as $T \to 0$.

Assumptions of Einstein Model

Einstein model successfully introduced quantum ideas in solid state physics but was later improved by Debye theory.

Einstein theory of Specific Heat (1907):

In every crystal the atom is surrounded by a group of first nearest neighbours, second nearest neighbours etc. Every atom vibrates in the vicinity of it's Lattice point or equillibrium position in a force field exerted by all it's neigbours . Each atom vibrates independently and at a constant frquency. in three dimensional space .Each atom can be treated like a simple harmonic oscillator and the energy of nth ocillator is given by : $$ E_{n}=\left(n+\frac{1}{2}\right) h f \quad \text { Where } \mathrm{n}=0,1,2,3 \ldots . $$

Mean energy of the oscillator is :

As energy of every harmonic oscillator is quantised and energy of nth oscillator is : $$ U_{n}=\left(n+\frac{1}{2}\right) h f $$ Then the average energy of such oscillator is:
$$ \begin{aligned} \langle U\rangle&=\dfrac{\sum_{n=0}^{n=\infty} U_{n} e^{-\left(\dfrac{U_{n}}{k T}\right)}}{\sum_{n=0}^{n=\infty} e^{-\left(\frac{U_{n}}{k T}\right)}}\\ & =\frac{\sum_{0}^{\infty}\left(n+\frac{1}{2}\right) h f e^{-\frac{\left(n+\frac{1}{2}\right) h f}{k T}}}{\sum_{0}^{\infty} e^{-\frac{\left(n+\frac{1}{2}\right) h f}{k T}}} \\ &= h f \frac{\sum_{0}^{\infty} n e^{-\frac{n h f}{k T}} e^{-\frac{h f}{2 k T}}}{\sum_{0}^{\infty} e^{\frac{-n h f}{k T}} e^{-\frac{h f}{2 k T}}}+\frac{1}{2} h f \frac{\sum_{0}^{\infty} e^{-\frac{n h f}{k T}} e^{-\frac{h f}{2 k T}}}{\sum_{0}^{\infty} e^{\frac{-n h f}{k T}} e^{-\frac{h f}{2 k T}}} \\ &= h f \frac{\sum_{0}^{\infty} n e^{-\frac{n h f}{k T}}}{\sum_{0}^{\infty} e^{\frac{-n h f}{k T}}+\frac{1}{2} h f} \frac{\sum_{0}^{\infty} e^{-\frac{n h f}{k T}}}{\sum_{0}^{\infty} e^{\frac{-n h f}{k T}}}=h f\left(\frac{\sum_{0}^{\infty} n e^{-\frac{n h f}{k T}}}{\sum_{0}^{\infty} e^{\frac{-n h f}{k T}}}+\frac{1}{2}\right) \\ &= h f\left(\frac{0+e^{-x}+2 e^{-2 x}+3 e^{-3 x}+4 e^{-4 x}+\ldots . .}{1+e^{-x}+e^{-2 x}+e^{-3 x}+e^{-4 x}+\ldots . .} \frac{1}{2}\right) T a k i n g x=\frac{h f}{k T} \\ &=h f\left(-\frac{d}{d x} \ln \left(1+e^{-x}+e^{-2 x}+e^{-3 x}+e^{-4 x}+\ldots .\right)+\frac{1}{2}\right) \\ &=h f\left(-\frac{d}{d x} \ln \left(1-e^{-x}\right)^{-1}+\frac{1}{2}\right) \\ &=h f\left(\frac{d}{d x} \ln \left(1-e^{-x}\right)+\frac{1}{2}\right)=h f\left(\frac{e^{-x}}{1-e^{-x}}+\frac{1}{2}\right)=h f\left(\frac{1}{2}+\frac{1}{e^{x}-1}\right) \\ &=h f\left(\frac{1}{2}+\frac{1}{e^{h f / k T}-1}\right) \end{aligned} $$
As the crystal contianing N atoms has 3 N harmonic oscillators . The total internal energy of the crystal becomes.
$$ \begin{aligned} U_{\text {total }}& =3 N\langle U\rangle\\ &=3 N\left(\frac{1}{2} h f+\frac{h f}{e^{h f / k T}-1}\right) \\ \Rightarrow U_{\text {total }}&=3 N\left(\frac{1}{2} h f+\frac{h f}{e^{h f / k T}-1}\right) \end{aligned} $$
Then specific heat of the crystal at constant volume is :
$$ \begin{aligned} C_{V}&=\frac{d U_{\text {total }}}{d T}\\ &=0+3 N h f \frac{d}{d T}\left(\frac{1}{e^{h f / k T}-1}\right) \\ & =3 N h f \frac{d}{d T}\left(e^{h f / k T}-1\right)^{-1} \\ & =-(3 N h f)\left(e^{h f / k T}-1\right)^{-2}\left(-e^{h f / k T} \frac{h f}{k T^{2}}\right) \\ & =3 N k\left(\frac{h f}{k T}\right)^{2}\left(\frac{1}{e^{h f / k T}-1}\right)^{2} e^{h f / k T} \\ & =3 N k\left(\frac{\theta_{E}}{T}\right)^{2}\left(\frac{1}{e^{\theta_{E} / T}-1}\right)^{2} e^{\theta_{E} / T} \text { where } h f=k \theta_{E}, \theta_{E} \text { is Einstein Temperature } \end{aligned} $$

Special Case :

(1) When temperature is very high \( T \gg \theta_E \)

\[ \begin{align} C_V &= 3Nk\left(\frac{\theta_E}{T}\right)^2 \left( \frac{1}{1 + \frac{\theta_E}{T} + \frac{1}{2}\left(\frac{\theta_E}{T}\right)^2 + \cdots - 1} \right)^2 \left(1 + \frac{\theta_E}{T} + \frac{1}{2}\left(\frac{\theta_E}{T}\right)^2 + \cdots \right) \\ &= 3Nk\left(\frac{\theta_E}{T}\right)^2 \left( \frac{1}{\frac{\theta_E}{T}} \right)^2 \left(1 + \frac{\theta_E}{T} \right) \\ &= 3Nk\left(1 + \frac{\theta_E}{T} \right) \\ &= 3Nk + 3Nk \cdot \frac{\theta_E}{T} \end{align} \]

Hence, when \( T \to \infty \), \( \frac{\theta_E}{T} \to 0 \),

\[ C_V = 3Nk = 3R \]

(2) When temperature is very low \( T \ll \theta_E \)

\[ \begin{align} C_V &= 3Nk\left(\frac{\theta_E}{T}\right)^2 \left( \frac{1}{e^{\theta_E/T}} \right)^2 e^{\theta_E/T} \quad \text{(since } e^{\theta_E/T} - 1 \approx e^{\theta_E/T} \text{)} \\ &= 3Nk\left(\frac{\theta_E}{T}\right)^2 e^{-\theta_E/T} \\ &= 3R\left(\frac{\theta_E}{T}\right)^2 e^{-\theta_E/T} \end{align} \]

As temperature \( T \to 0 \), the exponential term \( e^{-\theta_E/T} \to 0 \), hence the specific heat \( C_V \to 0 \).

Merits

Limitation of Einstein's Theory :