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Theme B — The Particulate Nature of Matter

B.3.5 Kinetic Theory of Gases — IB Physics HL Revision Notes & Topical Questions

5 min read 11 parts Lesson 29 of 53 1 quiz

📚 IB Physics HL Hub / Topical Revision
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Curriculum Equation Key قوانين الرقم الهيدروجيني والاتزان الأيوني - pH & Acid-Base Equilibrium FormulasFast Exam Solution
pH = -log[H⁺] | pOH = -log[OH⁻] | pH + pOH = 14 | [H⁺][OH⁻] = 10⁻¹⁴
Word Equation & Conditions: الرقم الهيدروجيني = -لوغاريتم تركيز أيون الهيدروجين | pH + pOH = 14
Location & Specifications: الاتزان الأيوني، كيمياء 3 ثانوي، التحصيلي، و AP Chemistry.
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Lesson summary

B.3.5 Kinetic Theory of Gases — IB PHYSICS SL notes: State the assumptions of the kinetic model of an ideal gas and use it to explain gas pressure and the gas laws.Kinetic theory — a modelled system that approximates the behaviour of real gases as atoms or molecules moving random…

  • Elastic collisions
  • Straight lines
  • Force on the wall
  • Faster molecules
  • Mean square speed
  • Definition

Part 1 of 9The aim of the model

Kinetic theory
  • Kinetic theory a modelled system that approximates the behaviour of real gases as atoms or molecules moving randomly at high speeds.
Link
  • Link it connects microscopic properties to macroscopic properties (pressure and volume).
    • (mass and speed of particles)
Method
  • Method apply Newton's laws to the particles and average over them.

Part 2 of 9Assumptions

1
A gas consists of many identical molecules, all with the same mass, in a container.
2
The volume of the molecules is negligible compared with the volume of the container, so they are point particles.
3
The molecules are in continuous random motion at high speeds.
4
The molecules obey Newton's laws of motion.
5
The molecules collide elastically with each other and with the walls.
6
There are no intermolecular forces except during collisions.
7
The time of a collision is negligible compared with the time between collisions.
8
External forces such as gravity are ignored.
9
The number of molecules is very large, so the average behaviour is considered.
10
Each particle exerts a force on the wall it collides with, and the average of these forces gives a uniform gas pressure.

Part 3 of 9Why the assumptions matter

Elastic collisions
  • Elastic collisions otherwise the gas would lose energy and its temperature would fall.
No forces
  • No forces the internal energy is entirely kinetic.
Straight lines
  • Straight lines between collisions the molecules move at constant velocity.

Part 4 of 9Explaining pressure

Rebound
  • Rebound for a molecule of mass m rebounding elastically, the velocity component perpendicular to the wall reverses and the momentum change is 2mvx.
Force on the wall
  • Force on the wall by Newton's third law the wall receives an equal and opposite impulse.
Averaging
  • Averaging billions of collisions per second give a constant force, and the pressure is the average force per unit area.
Faster molecules
  • Faster molecules a larger momentum change per collision and more collisions per second, so a higher pressure.

Part 5 of 9Explaining the gas laws

LawExplanation
Boyle's law (constant T)The average speed is the same; if the volume halves, molecules reach a wall twice as often and the pressure doubles
Pressure law (constant V)Raising T raises the average kinetic energy, so molecules hit harder and more often and P rises in proportion to T
Charles's law (constant P)When T rises, the volume must grow until the collision rate falls enough to keep the pressure constant

Part 6 of 9Result of the model

Equation
  • Equation p = ⅓ρ⟨c2⟩, or pV = ⅓Nm⟨c2⟩.
  • ρ is the density of the gas in kg m−3.
  • N is the number of molecules and m the mass of one molecule.
  • ⟨c2⟩ is the mean square speed in m2 s−2.
Mean square speed
  • Mean square speed the 'mean square' is an average over all molecules.

Part 7 of 9Root-mean-square speed

1Definition
  • Definition crms = √⟨c2⟩, found by squaring each speed, averaging, and taking the root.
2Compared with the mean speed
  • Compared with the mean speed it is slightly larger, because squaring emphasises large values.
3Result
  • Result crms = √(3RT/M) = √(3kBT/m).
4Lighter molecules
  • Lighter molecules they are faster at the same temperature; hydrogen is about four times faster than oxygen.
5Speed distribution
  • Speed distribution a skewed curve with a single peak and a long tail;
    • raising T moves the peak right and flattens it, with the area unchanged.
6Atmospheres
  • Atmospheres light molecules are the most easily lost from a planet.

Part 8 of 9Real and ideal gases

1Real gases
  • Real gases they do not always obey the ideal gas equation, because the assumptions may fail.
2Ideal approximation is good
  • Ideal approximation is good at low pressure, low density and a temperature well above the boiling point.
3High pressure and density
  • High pressure and density molecules are close, attractive forces act and their volume is not negligible.
4Low temperature
  • Low temperature the gas can become a liquid.
5Further limit
  • Further limit real molecules can rotate and vibrate and store energy that does not appear in the pressure.
6Success of the model
  • Success of the model it explains pressure and temperature in terms of mechanics.

Part 9 of 9More from the specification

1Kinetic energy across gas moles
  • Kinetic energy across gas moles calculating kinetic energy per mole of ideal gas particles provides a thermodynamic means to determine absolute temperature.
2Mole
  • Mole an amount of substance containing 6.02 times 10 to the 23 particles, and molar mass links mass to amount
3Kinetic theory
  • Kinetic theory pressure arises from molecular collisions with walls, and temperature is proportional to mean kinetic energy
4Ideal gas equation
  • Ideal gas equation pV equals nRT, which can be rearranged for any quantity such as amount of argon or helium
5Final state
  • Final state combined gas laws relate initial and final pressure, volume and temperature for a fixed amount
6Helium
  • Product of the fusion of hydrogen in stars.
7Boltzmann constant
  • K = R/NA, the gas constant per molecule
8Avogadro constant
  • The number of particles per mole, 6.02 × 10²³ mol⁻¹
9Thermodynamic temperature
  • The absolute temperature in kelvin.
10N = nNA
What the symbols mean: N = number of particles · n = amount (mol) · NA = Avogadro constant (6.02 × 1023 mol−1)

Key terms

TermMeaning
Kinetic theory of gasesModel explaining gas properties by random motion of many particles
Mean square speedAverage of the squares of the molecular speeds, ⟨c2⟩
R.m.s. speedSquare root of the mean square speed
Elastic collisionCollision in which kinetic energy is conserved
Point particleParticle whose size is negligible
Speed distributionGraph of the number of molecules against speed

Avoid these mistakes

1
Saying all molecules have the same speed — they have a wide range of speeds.
2
Thinking collisions with the walls lose energy — they are elastic.
3
Using the square of the mean speed instead of the mean square speed — use ⟨c2⟩.
4
Saying the model works at all conditions — it fails at high pressure and low temperature.
5
Thinking heavier molecules move faster — at the same T they are slower.

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