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Physics HL · Chapter 9: The Gas Laws

9.4 Boltzmann Equation, RMS Speed, and Internal Energy

Connect molecular speed distributions to pressure and show why average random kinetic energy scales with kelvin temperature.

Estimated time: 30 minutes

From Speed Distribution to RMS Speed

Molecules in a gas do not move at one shared speed. They occupy a distribution of speeds, with the distribution broadening and shifting upward as temperature increases. Because kinetic energy depends on v2v^2, averages based on squared speed are the natural bridge between microscopic motion and macroscopic observables.

crms=v2=3kBTmc_{\mathrm{rms}} = \sqrt{\langle v^2 \rangle} = \sqrt{\frac{3k_B T}{m}}

RMS speed weights faster molecules more strongly because kinetic energy is quadratic in speed.

The square-root dependence means doubling kelvin temperature does not double typical molecular speed; it multiplies rms speed by 2\sqrt{2}. This is a common conceptual checkpoint because many students over-predict speed changes by applying linear intuition to a square-law relationship.

Pressure-Density-RMS Relation

P=13ρcrms2P = \frac{1}{3}\rho c_{\mathrm{rms}}^2

Pressure scales with both particle mass density and squared random speed scale.

This equation is powerful because it ties a measurable macroscopic variable (pressure) to two microscopic-statistical descriptors (density and rms speed). It also clarifies why pressure can rise either by compressing gas (raising density) or by heating it (raising crmsc_{\mathrm{rms}} through temperature).

Combining this relation with PV=NkBTPV = Nk_B T yields one of the central results of kinetic theory: average random molecular kinetic energy is proportional to absolute temperature and independent of gas identity when compared per molecule at the same TT.

Microscopic Kinetic Energy and Internal Energy

Ek=32kBT,Umonatomic=32nRT\langle E_k \rangle = \frac{3}{2}k_B T,\qquad U_{\text{monatomic}} = \frac{3}{2}nRT

For monatomic ideal gases, internal energy is purely translational random kinetic energy.

At this level, internal energy behaves as a state quantity set by nn and TT for monatomic ideal gases. If TT rises while nn is fixed, UU rises linearly. If nn doubles at fixed TT, UU doubles because twice as many particles carry the same average kinetic energy each.

Model Scope Note

The $U = (3/2)nRT$ form is specific to monatomic ideal gases. Polyatomic gases can store energy in additional degrees of freedom.

This distinction between universal per-molecule thermal scaling and species-dependent heat-capacity behavior becomes important in later thermodynamics chapters. For now, keep the monatomic formula as a precise model statement, not a universal statement about all gases.

Simulation: RMS Speed and Internal-Energy Trends

Adjust temperature and molar mass to compare pressure growth, rms speed scaling, and monatomic internal-energy estimates.

Ideal Gas Law Lab

Active law interpretation

Gay-Lussac mode keeps n and V fixed, so pressure scales linearly with kelvin temperature (P/T = constant).

Container micro-view (animated gas particles + piston)

Volume: 10.00 LPressure: 691.7 kPaTemperature: 520.0 K

P-V map with isotherms

V (L)P (kPa)

State diagnostics

P

691.7 kPa

6.83 atm

T

520.0 K

246.9 deg C

V

10.00 L

0.0100 m^3

Pressure index47%
Thermal index65%
Volume fraction21%

Microscopic metrics

RMS speed c_rms: 1800.7 m s^-1

Mean molecular kinetic energy: 1.077e-20 J

Density estimate: 0.640 kg m^-3

Monatomic internal energy estimate: 10375.9 J

Model validity note

Ideal-model caution: this state approaches regimes where intermolecular forces and finite molecular size become important.

Try this workflow: hold n fixed, then switch between Boyle/Charles/Gay-Lussac modes and verify each ratio form before returning to full-state PV = nRT checks.

Test Yourself

For a monatomic ideal gas, n=2.0moln = 2.0\,\text{mol} at T=300KT = 300\,\text{K}. Enter the internal energy in joules.

Hint: Use U=(3/2)nRTU = (3/2)nRT with R=8.31J mol1K1R = 8.31\,\text{J mol}^{-1}\text{K}^{-1}.