12.3 Equipartition of Energy, Specific Heats and Mean Free Path
In equilibrium every independent way a molecule can store energy gets, on average, the same share, $\tfrac12k_BT$. Counting those ways predicts the heat capacities of gases and solids; counting collisions gives the mean free path.
Heat one mole of helium in a sealed container by one kelvin and it takes $12.5\ \text{J}$. Do the same with one mole of nitrogen and it takes $20.8\ \text{J}$ โ two-thirds as much again โ although at the same temperature the molecules of both gases have exactly the same mean translational kinetic energy, $\tfrac32k_BT$. Where does the extra energy go? A nitrogen molecule is a dumb-bell of two atoms: besides flying about, it can tumble end over end. Heating it means speeding up the tumbling as well as the flying.
This section counts the independent ways โ the degrees of freedom โ in which a molecule can hold energy, and states the law of equipartition of energy: in thermal equilibrium each one carries, on average, the same energy $\tfrac12k_BT$. That single rule predicts the molar heat capacities $C_v$ and $C_p$ and their ratio $\gamma$ for monatomic, diatomic and polyatomic gases, and the heat capacity $3R$ of solids โ and it shows, where it fails, the first hint of quantum physics. Finally you will see why a molecule moving at $500\ \text{m/s}$ takes so long to cross a room: it travels only about a ten-thousandth of a millimetre โ its mean free path โ before it hits another molecule and changes direction.
Degrees of freedom
To describe the position of a single atom you need three coordinates, $x$, $y$ and $z$, and its kinetic energy has three independent parts: $\tfrac12mv_x^2+\tfrac12mv_y^2+\tfrac12mv_z^2$. A rigid diatomic molecule can also rotate. Take the line joining its two atoms as the $z$-axis: it can spin about the $x$- and $y$-axes, with rotational kinetic energies $\tfrac12I_x\omega_x^2$ and $\tfrac12I_y\omega_y^2$ (Section 6.3). Spin about its own axis does not count โ the atoms are so nearly point-like that the moment of inertia about that axis is negligible. If the bond is not rigid, the two atoms can also vibrate along it, like two masses joined by a spring, adding a vibrational kinetic energy and an elastic potential energy, $\tfrac12\mu\left(\dfrac{dr}{dt}\right)^2+\tfrac12k(r-r_0)^2$.
The degrees of freedom of a molecule are the independent ways in which it can move. For counting energy we count the independent squared terms in the expression for its energy (each $\tfrac12mv_x^2$, $\tfrac12I\omega^2$, $\tfrac12kx^2$ is one); we write $f$ for their number.
- Monatomic (He, Ne, Ar): $3$ translational; $f=3$.
- Diatomic or linear, rigid ($\mathrm{N_2}$, $\mathrm{O_2}$, $\mathrm{H_2}$ at room temperature; $\mathrm{CO_2}$ if it did not vibrate): $3$ translational $+\,2$ rotational; $f=5$.
- Diatomic, vibrating (at high temperature): add $1$ vibrational mode, which carries $2$ terms (kinetic and potential); $f=7$.
- Non-linear polyatomic, rigid ($\mathrm{H_2O}$, $\mathrm{NH_3}$, $\mathrm{CH_4}$): $3$ translational $+\,3$ rotational; $f=6$. Each vibrational mode that is active adds $2$ more.
For a system in thermal equilibrium at absolute temperature $T$, the total energy is shared equally among all the independent squared terms in the energy: each translational and each rotational degree of freedom carries a mean energy $\tfrac12k_BT$, and each vibrational mode carries $2\times\tfrac12k_BT=k_BT$ (half as kinetic and half as potential energy). A molecule with $f$ squared terms has mean energy
$$\overline{\varepsilon}=\frac f2k_BT,\qquad U=\frac f2nRT\ \text{ for } n \text{ moles}.$$For translation you have already proved it: $\tfrac12m\overline{v^2}=\tfrac32k_BT$, so each of $\tfrac12m\overline{v_x^2}$, $\tfrac12m\overline{v_y^2}$, $\tfrac12m\overline{v_z^2}$ is $\tfrac12k_BT$ (Result 12.6). The law says that collisions do the same to every other kind of motion: if the molecules tumbled more slowly than their share, collisions would on average speed up the tumbling at the expense of translation, until the shares were equal. The law was found by Maxwell and Boltzmann; it is a result of classical (Newtonian) statistical physics, and it holds when every mode can take up energy freely โ we shall see when that fails.
Specific heat capacities of gases
The molar heat capacity at constant volume, $C_v$, is the heat needed per mole per kelvin when no work is done, so all of it goes into internal energy: $C_v=\dfrac{1}{n}\dfrac{\Delta U}{\Delta T}$. At constant pressure the gas also expands and does work, and for an ideal gas $C_p=C_v+R$ (Mayer's relation, from Chapter 11, Thermodynamics). Equipartition now predicts both.
For an ideal gas whose molecules have $f$ squared energy terms,
$$C_v=\frac f2R,\qquad C_p=\left(\frac f2+1\right)R,\qquad \gamma=\frac{C_p}{C_v}=1+\frac2f.$$| Molecule | $f$ | $C_v$ | $C_p$ | $\gamma$ |
|---|---|---|---|---|
| monatomic | 3 | $\tfrac32R$ | $\tfrac52R$ | $\tfrac53=1.67$ |
| diatomic, rigid | 5 | $\tfrac52R$ | $\tfrac72R$ | $\tfrac75=1.40$ |
| diatomic, vibrating | 7 | $\tfrac72R$ | $\tfrac92R$ | $\tfrac97=1.29$ |
| non-linear polyatomic, rigid | 6 | $3R$ | $4R$ | $\tfrac43=1.33$ |
A polyatomic molecule with $f_v$ active vibrational modes has $C_v=(3+f_v)R$ if non-linear and $\left(\tfrac52+f_v\right)R$ if linear. The more ways a molecule can store energy, the larger $C_v$ and the closer $\gamma$ is to $1$.
How good are the predictions? Measured values at room temperature (in $\text{J mol}^{-1}\text{K}^{-1}$, with $\tfrac32R=12.5$, $\tfrac52R=20.8$, $3R=24.9$):
| Gas | predicted $C_v$ | measured $C_v$ | measured $\gamma$ |
|---|---|---|---|
| He, Ar | 12.5 | 12.5 | 1.67 |
| $\mathrm{H_2}$, $\mathrm{N_2}$, $\mathrm{O_2}$ | 20.8 | 20.4โ21.1 | 1.40โ1.41 |
| $\mathrm{CH_4}$ | 24.9 | 27.4 | 1.31 |
| $\mathrm{CO_2}$ | 20.8 (rigid, linear) | 28.5 | 1.30 |
The agreement for monatomic and simple diatomic gases is excellent โ a triumph of the molecular picture, since these numbers were measured with calorimeters long before anyone could see a molecule. For $\mathrm{CO_2}$ and $\mathrm{CH_4}$ the measured values are higher than the rigid prediction because some of their vibrations already take up energy at room temperature.
Specific heat capacity of solids โ and where equipartition fails
In a solid each atom is held near a fixed position by its neighbours, as if by springs, and vibrates about it in three independent directions. Each direction is an oscillator with a kinetic and a potential term, so each atom has $f=6$ squared terms and mean energy $6\times\tfrac12k_BT=3k_BT$. A solid hardly expands when heated, so the work done is negligible and $C_p\approx C_v$.
For one mole of a solid element at ordinary temperatures, $U=3RT$, so
$$C=3R\approx25\ \text{J mol}^{-1}\text{K}^{-1}.$$The specific heat capacity is then $c=\dfrac{3R}{M}$: heavier atoms mean fewer atoms per kilogram and a smaller $c$.
Where classical theory fails. Equipartition predicts heat capacities that do not depend on temperature. Experiment disagrees at low temperatures. The $C_v$ of hydrogen gas falls from $\tfrac52R$ to $\tfrac32R$ below about $100\ \text{K}$, as though its molecules forgot how to rotate, and rises towards $\tfrac72R$ above about $2000\ \text{K}$, when the vibration finally joins in. The heat capacity of every solid falls towards zero as $T\to0$, and for diamond it is well below $3R$ even at room temperature. The explanation came from quantum theory: energy can be taken up by rotation and vibration only in steps of a definite size, and when $k_BT$ is much smaller than the step, those modes are "frozen out" and receive no share. Classical equipartition is the high-temperature limit.
Mean free path
If air molecules move at $500\ \text{m/s}$, why does the smell of perfume take minutes to cross a room? Because a molecule does not travel in a straight line for long. It collides with another molecule, is knocked in a new direction, collides again, and so wanders along a zigzag path. Its net progress is very slow.
The mean free path $\lambda$ is the average distance a molecule travels between successive collisions with other molecules. The collision frequency is the average number of collisions a molecule makes per second, about $\dfrac{v}{\lambda}$ where $v$ is a typical molecular speed; its reciprocal is the mean time between collisions.
Model each molecule as a sphere of diameter $d$. Two molecules collide if their centres pass within $d$ of each other. So, as a molecule moves a distance $L$, it hits every molecule whose centre lies inside a cylinder of radius $d$ โ cross-sectional area $\pi d^2$ โ around its path. That cylinder has volume $\pi d^2L$ and contains $n_V\pi d^2L$ molecules, so the molecule makes that many collisions in the distance $L$, and the distance per collision is $\dfrac{1}{n_V\pi d^2}$. Allowing for the motion of the other molecules (what matters is the relative speed, which on average is $\sqrt2$ times the speed of one molecule) reduces this by a factor $\sqrt2$.
For molecules of diameter $d$ at number density $n_V$, using $n_V=\dfrac{p}{k_BT}$ for an ideal gas,
$$\lambda=\frac{1}{\sqrt2\,\pi d^2n_V}=\frac{k_BT}{\sqrt2\,\pi d^2p}.$$At a fixed temperature $\lambda\propto\dfrac1p$; for a given number density it does not depend on temperature; and it falls sharply with molecular size, $\lambda\propto\dfrac{1}{d^2}$.
1. Counting vibration as one degree of freedom. An active vibrational mode has kinetic and potential energy: it contributes $k_BT$, not $\tfrac12k_BT$.
2. Three rotations for a linear molecule. A diatomic or linear molecule has only two rotational degrees of freedom; rotation about its own axis does not count. Non-linear molecules have three.
3. Averaging $\gamma$ for a mixture. Average $C_v$ (weighted by moles), then find $C_p=C_v+R$ and $\gamma=\dfrac{C_p}{C_v}$.
4. $\pi r^2$ instead of $\pi d^2$. Two molecules collide when their centres come within one diameter, so the collision area is $\pi d^2$.
5. "Translational energy depends on the gas." At a given temperature every molecule has $\tfrac32k_BT$ of translational energy; diatomic and polyatomic molecules have extra rotational (and vibrational) energy on top.
6. Applying equipartition at low temperatures. Below a characteristic temperature some modes are frozen out (hydrogen below $100\ \text{K}$ behaves as monatomic); classical equipartition is a high-temperature result.
Exercises
Take $R=8.31\ \text{J mol}^{-1}\text{K}^{-1}$, $k_B=1.38\times10^{-23}\ \text{J/K}$, $N_A=6.02\times10^{23}\ \text{mol}^{-1}$ and $1\ \text{atm}=1.013\times10^5\ \text{Pa}$. Treat diatomic gases as rigid and all gases as ideal unless told otherwise.
- 1 State the number of squared energy terms $f$ for a molecule of (a) helium, (b) oxygen at room temperature, (c) ammonia, $\mathrm{NH_3}$ (rigid), (d) carbon dioxide, treated as a rigid linear molecule.
- 2 Find the mean total energy of an oxygen molecule at $400\ \text{K}$.
- 3 Find the internal energy of $3.0\ \text{mol}$ of argon at $500\ \text{K}$.
- 4 Find the mean rotational kinetic energy of a nitrogen molecule at $300\ \text{K}$.
- 5 For a gas of rigid diatomic molecules, find the ratio of the total internal energy to the translational kinetic energy.
- 6 One mole of helium and one mole of oxygen are at the same temperature. Find the ratio of their internal energies.
- 7 Why is rotation of a diatomic molecule about the line joining its atoms not counted as a degree of freedom?
- 1 Find $C_v$, $C_p$ and $\gamma$ for a monatomic ideal gas, in $\text{J mol}^{-1}\text{K}^{-1}$.
- 2 A gas has $\gamma=1.40$. How many squared energy terms do its molecules have, and what kind of molecules could they be?
- 3 How much heat is needed to raise the temperature of $2.0\ \text{mol}$ of argon by $50\ \text{K}$ (a) at constant volume, (b) at constant pressure?
- 4 Treating methane, $\mathrm{CH_4}$ ($M=16\ \text{g/mol}$), as rigid and non-linear, find $\gamma$ and its specific heat capacity at constant volume per kilogram.
- 5 Find the specific heat capacity at constant volume of helium per kilogram ($M=4.0\ \text{g/mol}$).
- 6 One mole of helium is mixed with one mole of oxygen. Find $C_v$, $C_p$ and $\gamma$ of the mixture.
- 7 At very high temperatures the molecules of a diatomic gas also vibrate. Find $\gamma$ then.
- 8 The measured $C_v$ of carbon dioxide at room temperature is $28.5\ \text{J mol}^{-1}\text{K}^{-1}$, larger than the rigid-molecule prediction. Explain.
- 1 Use the DulongโPetit law to predict the specific heat capacity of lead ($M=207\ \text{g/mol}$); the measured value is $128\ \text{J kg}^{-1}\text{K}^{-1}$.
- 2 Predict the specific heat capacity of iron ($M=55.8\ \text{g/mol}$).
- 3 Estimate the heat needed to warm a $0.50\ \text{kg}$ copper block ($M=63.5\ \text{g/mol}$) by $20\ \text{K}$.
- 4 Why are $C_p$ and $C_v$ almost equal for a solid but very different for a gas?
- 5 Below about $100\ \text{K}$ the molar heat capacity of hydrogen gas at constant volume is close to $\tfrac32R$. What does this tell you about its molecules?
- 1 Taking the diameter of an oxygen molecule as $3.0\times10^{-10}\ \text{m}$, find its mean free path at STP.
- 2 How does the mean free path change if (a) the pressure is halved at constant temperature, (b) the temperature is doubled at constant pressure, (c) the temperature is doubled at constant volume?
- 3 For molecules of diameter $3.0\times10^{-10}\ \text{m}$, find the number density, and the pressure at $300\ \text{K}$, at which the mean free path is $1.0\ \text{m}$.
- 4 Using part 1 and $v_\text{rms}=461\ \text{m/s}$, find the collision frequency of an oxygen molecule at STP.
- 5 At a height of $100\ \text{km}$ the number density of air molecules is about $1.2\times10^{19}\ \text{m}^{-3}$. Find the mean free path there ($d=3.7\times10^{-10}\ \text{m}$).
- 6 (Modelling) A molecule making $N$ random steps of length $\lambda$ wanders a net distance of only about $\lambda\sqrt N$. Using parts 1 and 4, estimate how far a perfume molecule wanders by diffusion in $1\ \text{s}$, and how long it would take to cross a $3\ \text{m}$ room by diffusion alone. What really carries smells across a room?
- 7 Show that $\dfrac{k_BT}{\sqrt2\,\pi d^2p}$ has the dimensions of length.
E1. Board ยท 3 marks State the law of equipartition of energy. Use it to find the molar heat capacities $C_v$ and $C_p$ and the ratio $\gamma$ for a gas of rigid diatomic molecules.
E2. NEET One mole of a monatomic gas is mixed with one mole of a rigid diatomic gas. The ratio $\gamma=\dfrac{C_p}{C_v}$ for the mixture is (a) $1.40$ (b) $1.50$ (c) $1.53$ (d) $1.67$
E3. JEE Main (Numerical value) A vessel contains $8.0\ \text{g}$ of helium ($M=4\ \text{g/mol}$) and $32\ \text{g}$ of oxygen ($M=32\ \text{g/mol}$) at $400\ \text{K}$. Find the total internal energy of the mixture in kJ, to the nearest integer. ($R=8.31\ \text{J mol}^{-1}\text{K}^{-1}$; treat oxygen as rigid.)
E4. JEE Advanced (One or more correct) For an ideal gas of rigid diatomic molecules at temperature $T$: (A) the mean rotational kinetic energy of a molecule is $k_BT$; (B) $\gamma=1.4$; (C) $C_p-C_v=R$ per mole; (D) the translational kinetic energy is $\tfrac25$ of the internal energy.
E5. NEET JEE Main The mean free path of the molecules of a gas is $\lambda$. If both the pressure and the absolute temperature of the gas are doubled, the mean free path becomes (a) $\dfrac\lambda2$ (b) $\lambda$ (c) $2\lambda$ (d) $4\lambda$
E6. Board ยท Case study A materials laboratory measures the specific heat capacities of metals at room temperature. For silver ($M=108\ \text{g/mol}$) it finds $235\ \text{J kg}^{-1}\text{K}^{-1}$, but for diamond (carbon, $M=12\ \text{g/mol}$) only $509\ \text{J kg}^{-1}\text{K}^{-1}$. (i) Explain why classical theory gives a molar heat capacity of $3R$ for a solid. [1] (ii) Predict the specific heat capacity of silver and compare. [2] (iii) Find the measured molar heat capacity of diamond and comment. [1]
Research question. Do the metals in your home obey the DulongโPetit law โ and can you count atoms with a kettle and a thermometer?
Why it matters. In the nineteenth century, chemists used the rule $C\approx3R$ to correct wrongly guessed atomic masses of metals such as uranium and indium. Today engineers use heat capacities to design heat sinks for electronics, cooking pans and thermal energy stores; materials scientists use the departure from $3R$ at low temperatures to study how atoms vibrate in new materials.
What to do. Use the method of mixtures with metal objects of known composition: a bunch of steel washers or nails (iron), aluminium foil folded into a block or an aluminium weight, copper coins or wire, a lead fishing weight.
- Weigh about $100$โ$200\ \text{g}$ of one metal. Heat it in boiling water for five minutes so that it reaches about $100\ ^\circ\text{C}$ (measure the water temperature).
- Put a measured mass of cold water (about $200\ \text{g}$) in an insulated cup (a polystyrene cup inside another) and record its temperature.
- Transfer the metal quickly into the cold water, stir, and record the highest steady temperature.
- Heat lost by metal $=$ heat gained by water: find the metal's specific heat capacity $c$, then its molar heat capacity $cM$. Compare with $3R=24.9\ \text{J mol}^{-1}\text{K}^{-1}$.
- Repeat for every metal and plot $c$ against $\dfrac1M$. DulongโPetit predicts a straight line through the origin of slope $3R$.
Tools: Kitchen scale (1 g resolution), a digital thermometer, insulated cups, a pan of boiling water, tongs, a spreadsheet.
Hand in: A table of $m$, temperatures, $c$ and $cM$ for each metal; the $c$โ$\dfrac1M$ graph with its fitted slope; a discussion of heat losses and of the error from water carried over with the hot metal.
Going further. Look up how the molar heat capacity of a metal varies from $10\ \text{K}$ to $300\ \text{K}$. Find out what Einstein (1907) and Debye (1912) proposed to explain the fall at low temperatures.
๐งช Self-check quiz
Q1. The number of degrees of freedom of a rigid diatomic molecule is
Q2. According to the law of equipartition, the mean energy associated with each translational or rotational degree of freedom of a molecule at temperature $T$ is
Q3. The ratio $\gamma=\dfrac{C_p}{C_v}$ for a monatomic ideal gas is
Q4. By the law of Dulong and Petit, the molar heat capacity of a solid element at ordinary temperatures is about
Q5. The mean free path of the molecules of a gas doubles when