The Distribution of Molecular Speeds — Question 2

Section 19-6 · Physics pages 3134–3135

Question 2 Mode mean and rms speed represent different features of one distribution For a classical equilibrium gas, write the speed density as f(v) = Cv2e−av2 for v ≥0, where a = m/(2kBT). Use C = 4a3/2/√π, ∫∞ 0 v3e−av2dv = 1/(2a2) and ⟨v2⟩= 3/(2a). Take M = .0200 kg/mol, T = 360 K and R = 8.314 J/(mol K). v f(v) vmp Axes and labels specify the model; the sketch is schematic. (a) Derive the most probable speed by differentiation, then calculate the mean and rms speeds. (b) Find the speed standard deviation and its ratio to the mean. Establish the ordering of the three characteristic speeds.
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Question 2 - Solution Mode mean and rms speed represent different features of one distribution v f(v) vmp (a) Method and calculation d ln f dv = 2 v −2av = 0 ⇒vmp = a−1/2 = √ 2RT/M ≈547.087 m/s. v = C/(2a2) = √ 8RT/(πM) ≈617.321 m/s, vrms = √ 3RT/M ≈670.042 m/s. (b) Interpretation and further calculation σ2 v = ⟨v2⟩−v2 = (3 −8/π)RT/M. σv ≈260.519 m/s, σv v = √ 3π/8 −1 ≈.422016. vmp < v < vrms. The asymmetric tail raises the mean above the mode; squaring speeds gives fast particles additional weight. Physical check The rms-minus-mean difference is not the standard deviation; the variances must be subtracted before taking a square root.

Question 2

Mode mean and rms speed represent different features of one distribution

For a classical equilibrium gas, write the speed density as f(v)=Cv2e−av2f(v)=Cv^2e^{-av^2} for v≥0v\ge0, where a=m/(2kBT)a=m/(2k_BT). Use C=4a3/2/πC=4a^{3/2}/\sqrt\pi, ∫0∞v3e−av2dv=1/(2a2)\int_0^\infty v^3e^{-av^2}dv=1/(2a^2) and ⟨v2⟩=3/(2a)\langle v^2\rangle=3/(2a). Take M=.0200M=.0200 kg/mol, T=360T=360 K and R=8.314R=8.314 J/(mol K).

Diagram shown in the original SVG worksheet.

  1. Derive the most probable speed by differentiation, then calculate the mean and rms speeds.

  2. Find the speed standard deviation and its ratio to the mean. Establish the ordering of the three characteristic speeds.

Question 2 - Solution

Mode mean and rms speed represent different features of one distribution

Diagram shown in the original SVG worksheet.

(a) Method and calculation

dln⁡fdv=2v−2av=0⇒vmp=a−1/2=2RT/M≈547.087m/s.\frac{d\ln f}{dv}=\frac2v-2av=0\ \Rightarrow\ v_{\mathrm{mp}}=a^{-1/2}=\sqrt{2RT/M}\approx547.087\,\mathrm{m/s}.v¯=C/(2a2)=8RT/(πM)≈617.321m/s,vrms=3RT/M≈670.042m/s.\overline v=C/(2a^2)=\sqrt{8RT/(\pi M)}\approx617.321\,\mathrm{m/s},\quad v_{\mathrm{rms}}=\sqrt{3RT/M}\approx670.042\,\mathrm{m/s}.

(b) Interpretation and further calculation

σv2=⟨v2⟩−v¯2=(3−8/π)RT/M.\sigma_v^2=\langle v^2\rangle-\overline v^2=(3-8/\pi)RT/M.σv≈260.519m/s,σvv¯=3π/8−1≈.422016.\sigma_v\approx260.519\,\mathrm{m/s},\quad\frac{\sigma_v}{\overline v}=\sqrt{3\pi/8-1}\approx.422016.vmp<v¯<vrms.v_{\mathrm{mp}}<\overline v<v_{\mathrm{rms}}.The asymmetric tail raises the mean above the mode; squaring speeds gives fast particles additional weight.

Physical check

The rms-minus-mean difference is not the standard deviation; the variances must be subtracted before taking a square root.