Equation of State – Cambridge A‑Level Physics (9702)
Learning Objective
Recall that the Boltzmann constant k links the macroscopic gas constant R to the number of particles per mole NA:
$$k = \frac{R}{N_{\mathrm A}}$$
1. The Mole
Definition: One mole of a substance contains exactly NA = 6.022 140 76 × 10²³ elementary entities (atoms, molecules, ions, …).
SI unit of amount of substance:mol.
Molar mass (M) is the mass of one mole of a substance (units g mol⁻¹). Numerically it equals the average mass of a single particle expressed in atomic mass units (u).
Conversion between amount of substance and number of particles:
$$n = \frac{N}{N_{\mathrm A}}\qquad\text{or}\qquad N = n\,N_{\mathrm A}$$
where n is the amount in moles and N the total number of particles.
Worked examples
From mass to particles (CO₂):
The molar mass of carbon dioxide is 44.01 g mol⁻¹. A 22.0 g sample contains
$$n = \frac{22.0\;\text{g}}{44.01\;\text{g mol}^{-1}} = 0.500\;\text{mol}$$
and therefore
$$N = 0.500\;\text{mol}\times 6.022\times10^{23}\;\text{mol}^{-1}=3.01\times10^{23}\;\text{molecules}.$$
From particles to mass (H₂):
How many grams of hydrogen correspond to \(2.0\times10^{23}\) molecules?
First find the number of moles:
$$n = \frac{N}{N_{\mathrm A}} = \frac{2.0\times10^{23}}{6.022\times10^{23}} = 0.332\;\text{mol}.$$
The molar mass of H₂ is 2.016 g mol⁻¹, so the mass is
$$m = nM = 0.332\;\text{mol}\times 2.016\;\text{g mol}^{-1}=0.670\;\text{g}.$$
2. Ideal‑Gas Law (Macroscopic Form)
The equation of state for an ideal gas is
$$pV = nRT$$
where
p – pressure (Pa)
V – volume (m³)
n – amount of substance (mol)
R – universal gas constant (8.314 462 618 J mol⁻¹ K⁻¹)
T – absolute temperature (K)
3. The Three Simple Gas Laws
Law
Statement (conditions fixed)
Mathematical form
Boyle’s law
At constant T and n, pressure is inversely proportional to volume.
$$pV = \text{constant}$$
Charles’s law
At constant p and n, volume is directly proportional to absolute temperature.
$$\frac{V}{T} = \text{constant}$$
Avogadro’s law
At constant p and T, volume is directly proportional to the amount of gas.
$$\frac{V}{n} = \text{constant}$$
Bridge paragraph: Combining Boyle’s, Charles’s and Avogadro’s laws eliminates the three separate constants and yields the single macroscopic ideal‑gas equation \(pV = nRT\). This unified form can be rewritten in microscopic terms by substituting \(n = N/N_{\mathrm A}\), where \(N\) is the total number of particles.
4. Microscopic Form of the Equation of State
Replace the amount of substance in the macroscopic law:
$$pV = \frac{N}{N_{\mathrm A}}RT$$
Define the Boltzmann constant \(k = R/N_{\mathrm A}\) to obtain
$$pV = NkT$$
5. Deriving the Boltzmann Constant
From the two equivalent expressions
Macroscopic: \(pV = nRT\)
Microscopic: \(pV = NkT\)
and using \(n = N/N_{\mathrm A}\):
$$\frac{N}{N_{\mathrm A}}RT = NkT \;\;\Longrightarrow\;\; k = \frac{R}{N_{\mathrm A}}.$$
6. Kinetic Theory of Gases – Key Assumptions
The gas consists of a very large number of tiny particles (atoms or molecules) in constant random motion.
The volume of the particles themselves is negligible compared with the container volume.
Collisions between particles, and between particles and the container walls, are perfectly elastic (no loss of kinetic energy).
No intermolecular forces act except during collisions.
The average translational kinetic energy of the particles depends only on temperature.
7. From Kinetic Theory to the Microscopic Equation
Consider a cubic container of side \(L\) (so \(V = L^{3}\)) and a single molecule of mass \(m\) moving with speed component \(c_{x}\) perpendicular to a wall.
Change in momentum on a collision: \(\Delta p = 2mc_{x}\).
Time between successive collisions with the same wall: \(\Delta t = 2L/c_{x}\).
Force exerted on the wall by this molecule:
$$F = \frac{\Delta p}{\Delta t}= \frac{2mc_{x}}{2L/c_{x}}= \frac{mc_{x}^{2}}{L}.$$
Pressure contributed by this molecule:
$$p = \frac{F}{A}= \frac{mc_{x}^{2}}{L^{3}} = \frac{mc_{x}^{2}}{V}.$$
For many molecules the motion is isotropic, so
$$\langle c_{x}^{2}\rangle = \langle c_{y}^{2}\rangle = \langle c_{z}^{2}\rangle = \frac{1}{3}\langle c^{2}\rangle.$$
Summing over all \(N\) particles gives the kinetic‑theory equation of state:
$$pV = \frac{1}{3}\,N\,m\,\langle c^{2}\rangle.$$
8. Connecting Kinetic Theory to Temperature
The average translational kinetic energy of a molecule is
Problem: Calculate the rms speed of nitrogen (N₂) molecules at 300 K. (Molar mass of N₂ = 28.02 g mol⁻¹.)
Mass of one N₂ molecule:
$$m = \frac{M}{N_{\mathrm A}} = \frac{28.02\times10^{-3}\;\text{kg mol}^{-1}}{6.022\times10^{23}\;\text{mol}^{-1}} = 4.65\times10^{-26}\;\text{kg}.$$
Insert into the rms‑speed formula:
$$v_{\text{rms}} = \sqrt{\frac{3kT}{m}} = \sqrt{\frac{3(1.380649\times10^{-23}\;\text{J K}^{-1})(300\;\text{K})}{4.65\times10^{-26}\;\text{kg}}} \approx 5.2\times10^{2}\;\text{m s}^{-1}.$$
11. Quick Revision Checklist
Can you write the ideal‑gas law in both macroscopic (pV = nRT) and microscopic (pV = NkT) forms?
Do you know the definition of a mole, its SI unit (mol), and how to convert between mass, moles, and number of particles?
Can you list the three simple gas laws (Boyle, Charles, Avogadro) and explain how they combine to give the macroscopic equation of state?
Are you able to derive k = R/NA and the kinetic‑theory result pV = (1/3)Nm⟨c²⟩?
Can you use k to calculate average kinetic energy (3/2 kT) and rms speed (√(3kT/m))?
Do you remember the numerical values and units of R, NA and k?
Suggested diagram: Sketch of gas molecules colliding with the walls of a container, illustrating how pressure arises from molecular impacts.
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