2.4.6States of Matter (Quantitative)

Maxwell-Boltzmann distribution of speeds — most probable, mean, rms

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1. Building the distribution from scratch

HOW we derive it (Feynman-style, two ingredients):

Ingredient 1 — Boltzmann factor. The probability a molecule has kinetic energy ε=12mv2\varepsilon=\tfrac12 mv^2 falls off like eε/kT=emv2/2kTe^{-\varepsilon/kT}=e^{-mv^2/2kT}. WHY: fewer molecules can afford large energy at temperature TT.

Ingredient 2 — Volume of "velocity shell". Velocity is 3D: (vx,vy,vz)(v_x,v_y,v_z). All velocity vectors with speed near vv live on a spherical shell of radius vv and thickness dvdv. Its volume 4πv2dv\propto 4\pi v^2\,dv. WHY the v2v^2: bigger spheres have more surface, so more ways to have a large speed — this pushes the peak away from v=0v=0.

Multiply the two and add a normalizing constant AA: f(v)=A4πv2how many ways  emv2/2kThow likelyf(v) = A\,\underbrace{4\pi v^2}_{\text{how many ways}}\;\underbrace{e^{-mv^2/2kT}}_{\text{how likely}}

Finding AA (normalization). Require 0f(v)dv=1\int_0^\infty f(v)\,dv=1. Using the Gaussian integral 0v2eαv2dv=14π/α3\int_0^\infty v^2 e^{-\alpha v^2}dv=\tfrac14\sqrt{\pi/\alpha^3} with α=m/2kT\alpha=m/2kT, you get A=(m2πkT)3/2A=\left(\dfrac{m}{2\pi kT}\right)^{3/2}.

Figure — Maxwell-Boltzmann distribution of speeds — most probable, mean, rms

2. The three characteristic speeds — each derived

Let α=m2kT\alpha=\dfrac{m}{2kT} so f(v)v2eαv2f(v)\propto v^2 e^{-\alpha v^2}. Note 1α=2kTm\dfrac1\alpha=\dfrac{2kT}{m}.

(a) Most probable speed vmpv_{mp} — the PEAK

WHAT: the speed at which f(v)f(v) is maximum (most molecules near here). HOW: set dfdv=0\dfrac{df}{dv}=0. ddv(v2eαv2)=(2v2αv3)eαv2=0\frac{d}{dv}\Big(v^2 e^{-\alpha v^2}\Big)=\big(2v-2\alpha v^3\big)e^{-\alpha v^2}=0 Why this step? Product rule; the exponential is never zero, so the bracket must vanish. 2v(1αv2)=0v2=1α=2kTm2v(1-\alpha v^2)=0\Rightarrow v^2=\frac1\alpha=\frac{2kT}{m} vmp=2kTm=2RTM\boxed{v_{mp}=\sqrt{\frac{2kT}{m}}=\sqrt{\frac{2RT}{M}}}

(b) Mean (average) speed vˉ\bar v — the BALANCE point

WHAT: average of speed itself, vˉ=0vf(v)dv\bar v=\int_0^\infty v\,f(v)\,dv. HOW: need 0v3eαv2dv=12α2\int_0^\infty v^3 e^{-\alpha v^2}dv=\dfrac{1}{2\alpha^2}. vˉ=4π(απ)3/212α2=2πα\bar v = 4\pi\Big(\frac{\alpha}{\pi}\Big)^{3/2}\cdot\frac{1}{2\alpha^2}=\frac{2}{\sqrt{\pi\alpha}} Why this step? Now substitute 1α=2kTm\dfrac1\alpha=\dfrac{2kT}{m}, so 1πα=2kTπm\dfrac{1}{\pi\alpha}=\dfrac{2kT}{\pi m} and 2πα=22kTπm=42kTπm=8kTπm\dfrac{2}{\sqrt{\pi\alpha}}=2\sqrt{\dfrac{2kT}{\pi m}}=\sqrt{\dfrac{4\cdot 2kT}{\pi m}}=\sqrt{\dfrac{8kT}{\pi m}} (the factor 22 becomes 44 inside the root, giving 88, not 44). vˉ=8kTπm=8RTπM\boxed{\bar v=\sqrt{\frac{8kT}{\pi m}}=\sqrt{\frac{8RT}{\pi M}}}

(c) Root-mean-square speed vrmsv_{rms} — the ENERGY average

WHAT: vrms=v2v_{rms}=\sqrt{\overline{v^2}}, where v2=0v2f(v)dv\overline{v^2}=\int_0^\infty v^2 f(v)\,dv. This is the one tied to kinetic energy: KE=12mv2=32kT\overline{KE}=\tfrac12 m\overline{v^2}=\tfrac32 kT. HOW: need 0v4eαv2dv=38πα5\int_0^\infty v^4 e^{-\alpha v^2}dv=\dfrac{3}{8}\sqrt{\dfrac{\pi}{\alpha^5}}. v2=4π(απ)3/238πα5=32α=3kTm\overline{v^2}=4\pi\Big(\frac{\alpha}{\pi}\Big)^{3/2}\cdot\frac{3}{8}\sqrt{\frac{\pi}{\alpha^5}}=\frac{3}{2\alpha}=\frac{3kT}{m} vrms=3kTm=3RTM\boxed{v_{rms}=\sqrt{\frac{3kT}{m}}=\sqrt{\frac{3RT}{M}}}


3. Effect of temperature and mass


4. Worked examples


5. Common mistakes (Steel-man + fix)


6. Flashcards

What does f(v)dvf(v)\,dv represent physically?
The fraction of gas molecules with speed between vv and v+dvv+dv.
Why does an extra factor v2v^2 (not just the Boltzmann factor) appear in f(v)f(v)?
The 4πv2dv4\pi v^2\,dv is the volume of the velocity-space spherical shell — more ways to have a large speed, so the peak moves off zero.
Formula for most probable speed vmpv_{mp}?
vmp=2kT/m=2RT/Mv_{mp}=\sqrt{2kT/m}=\sqrt{2RT/M} (found by df/dv=0df/dv=0).
Formula for mean speed vˉ\bar v?
vˉ=8kT/πm=8RT/πM\bar v=\sqrt{8kT/\pi m}=\sqrt{8RT/\pi M}.
Formula for rms speed vrmsv_{rms}?
vrms=3kT/m=3RT/Mv_{rms}=\sqrt{3kT/m}=\sqrt{3RT/M}.
The fixed ratio vmp:vˉ:vrmsv_{mp}:\bar v:v_{rms}?
2:8/π:3=1:1.128:1.225\sqrt2:\sqrt{8/\pi}:\sqrt3 = 1:1.128:1.225.
Which speed is largest and why?
vrmsv_{rms}; squaring over-weights the fast tail.
Which speed relates directly to average KE?
vrmsv_{rms}, since 12mv2=32kT\tfrac12 m\overline{v^2}=\tfrac32 kT.
Effect of raising TT on the curve?
Peak shifts right, curve flattens and widens; area stays 1.
Effect of larger molar mass MM at fixed TT?
Peak shifts left, curve taller and narrower (slower molecules).
vrmsv_{rms} of O₂ at 300 K?
≈ 484 m/s.
Ratio of rms speeds of two gases at same TT?
M2/M1\sqrt{M_2/M_1} (lighter is faster).

Recall Feynman: explain to a 12-year-old

Imagine a huge crowd of bouncy balls in a box, all bumping each other. They don't all move at the same speed — some crawl, most go medium, a few zoom super fast. If you make a chart of "how many balls go this fast," it looks like a hill that's steep on the slow side and has a long slope on the fast side. The top of the hill = the speed most balls have. The average speed is a bit to the right (the fast zoomers pull it over). And if you care about energy (which grows with speed²), the fast ones matter even more, so the "energy speed" is furthest right. Heat the box → all balls speed up (hill slides right). Use heavier balls → they're lazy and slow (hill slides left).

Concept Map

how likely

how many ways

requires

gives

completes

shapes

df/dv = 0 gives peak

balance point average

energy-weighted average

v_mp lt v_bar lt v_rms

Boltzmann factor e^-mv2/2kT

Velocity shell 4 pi v2 dv

Distribution f of v

Normalization integral = 1

Constant A = m/2 pi kT ^3/2

Skewed bell curve

Most probable v_mp

Mean v_bar

RMS v_rms

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, gas ke andar saare molecules ek jaisi speed se nahi chalte. Wo aapas mein tकkar maar-maar ke energy exchange karte rehte hain, isliye koi slow hota hai, koi fast. Agar hum count karein "kitne molecules kis speed pe hain", to ek bell-jaisa curve milta hai jo right side pe lamba tail rakhta hai — kyunki speed 0 se neeche nahi ja sakti, par upar ki koi limit nahi. Isko Maxwell-Boltzmann distribution kehte hain. Curve banta hai do cheezon ke multiply hone se: emv2/2kTe^{-mv^2/2kT} (Boltzmann factor — badi energy hone ke chance kam) aur 4πv24\pi v^2 (velocity-space shell ka volume — badi speed ke liye zyada "ways").

Ab kyunki curve symmetric nahi hai, teen alag "average" nikalte hain. vmpv_{mp} = curve ka peak (sabse zyada molecules yahin), df/dv=0df/dv=0 karke milta hai, value 2RT/M\sqrt{2RT/M}. vˉ\bar v = seedha average speed, 8RT/πM\sqrt{8RT/\pi M}. Yahan ek chhota trap hai: derivation mein 2/πα2/\sqrt{\pi\alpha} aata hai, aur jab 22 ko root ke andar le jaate ho to wo 44 ban jaata hai (kyunki 2X=4X2\sqrt X=\sqrt{4X}), isliye andar ka 22 multiply hoke 88 banta hai — 8kT/πm8kT/\pi m, na ki 44. vrmsv_{rms} = speed square ka average ka root, 3RT/M\sqrt{3RT/M} — yehi wala kinetic energy se juda hai kyunki 12mv2=32kT\tfrac12 m\overline{v^2}=\tfrac32 kT. Order hamesha yaad rakho: vmp<vˉ<vrmsv_{mp}<\bar v<v_{rms}, ratio 1:1.128:1.2251:1.128:1.225.

Physics samajhne ki baat: vrmsv_{rms} sabse bada hota hai kyunki square karne se fast wale molecules ka weight badh jaata hai. Temperature badhao to curve right shift karke chaudha ho jaata hai (area hamesha 1 rehta hai). Bhaari gas (zyada MM) slow hoti hai, curve left shift + patla. Exam tip (80/20): ek speed nikaal lo, baaki do ratio se turant mil jaate hain. Aur bhai — M ko kg/mol mein daalo, g/mol daala to answer galat aayega!

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