13.3Free
Your guide: Sir HamzaBelieves every formula has a story, and units never lie.
Throw a tennis ball at a wall and catch it on the rebound, again and again. Your wall feels a push each time. Now imagine billions of balls every second, too small to see. That steady push is gas pressure.
This section turns that picture into an equation. It links what we measure (pressure and volume) to what we cannot see (the mass and speed of molecules). We start with one molecule in a cube of side L.
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Throw a tennis ball at a wall and catch it on the rebound, again and again. Your wall feels a push each time. Now imagine billions of balls every second, too small to see. That steady push is gas pressure.
This section turns that picture into an equation. It links what we measure (pressure and volume) to what we cannot see (the mass and speed of molecules). We start with one molecule in a cube of side L.
For N molecules of mass m in volume V: PV = ⅓Nm⟨v2⟩, where ⟨v2⟩ is the mean-square speed. With density ρ = Nm/V, this becomes P = ⅓ρ⟨v2⟩.
Q1. Derive the force exerted on a wall by one molecule of mass m moving with velocity vₓ in a cube of side L.
F = mvₓ2 ÷ L
Q2. Starting from P = (Nm/V)⟨vₓ2⟩, show that PV = ⅓Nm⟨v2⟩ and P = ⅓ρ⟨v2⟩.
PV = ⅓Nm⟨v2⟩ · P = ⅓ρ⟨v2⟩
Q3. Numerical 13.2: find the pressure of oxygen at 0 °C if its density is 1.44 kg m−3 and its rms speed is 456.4 m s−1.
P ≈ 1.0 × 105 N m−2
✗ Writing Δp = 0 because the molecule's speed is the same before and after the hit.
✓ Momentum is a vector. The speed is the same but the direction reverses, so Δp = −2mvₓ.
✗ Using the average velocity of the molecules in the formula.
✓ The average velocity is zero, because +v and −v cancel. The formula needs the mean-square speed ⟨v2⟩, or the rms speed squared.
✗ Forgetting the ⅓ and writing PV = Nm⟨v2⟩.
✓ Only the x-part of the motion pushes on the wall, and on average it carries one-third of ⟨v2⟩. So PV = ⅓Nm⟨v2⟩.
1. A molecule of mass m hits a wall with velocity vₓ and rebounds elastically. Its change in momentum is:
(c) −mvₓ − mvₓ = −2mvₓ: the direction reverses.
2. The time between two collisions of the molecule with the same wall is:
(b) It must travel 2L (there and back) at speed vₓ.
3. In a closed room a gas has pressure 3.2 × 105 N m−2 and density 6 kg m−3. The effective (rms) speed of its particles is:
(a) v = √(3P/ρ) = √(3 × 3.2 × 105 ÷ 6) = √(1.6 × 105) = 400 m s−1.
4. If the density of a gas is doubled, with everything else unchanged, its pressure:
(c) P = ⅓ρ⟨v2⟩: with ⟨v2⟩ fixed, pressure is directly proportional to density.
5. Why is ⟨vₓ2⟩ = ⅓⟨v2⟩?
(b) No direction is preferred, so ⟨vₓ2⟩ = ⟨v_y2⟩ = ⟨v_z2⟩, and together they make ⟨v2⟩.