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Physics HL · Chapter 7: Thermal Energy Transfers

7.1 Particles, Temperature, and Internal Energy

Connect states of matter to intermolecular forces, then relate Kelvin temperature to average random kinetic energy and thermal equilibrium.

Estimated time: 28 minutes

Particle Models for Solids, Liquids, and Gases

In solids, particles remain close to equilibrium positions and oscillate around them. Strong intermolecular forces keep average separation small and make solids resistant to compression. In liquids, particles remain close but can rearrange continuously, so liquids flow while still showing very low compressibility. In gases, average separation is much larger and intermolecular forces are usually negligible except during brief collisions.

This microscopic difference explains macroscopic density trends. Solids and liquids of the same substance usually have comparable densities, while gases are often orders of magnitude less dense under ordinary conditions. The point is not memorizing one ratio, but understanding why large average separation in gases implies large volume for the same amount of matter.

Temperature as Average Random Kinetic Energy

Ek=32kBT\overline{E_k} = \frac{3}{2}k_B T

For idealized particle models, Kelvin temperature is proportional to average random kinetic energy per particle.

This proportionality is one of the central bridges in thermal physics: temperature is not a vague sensation of hotness, it is a measurable macroscopic variable linked to microscopic random motion. As T increases, average random molecular speed increases. As T decreases, average random motion decreases. The absolute minimum of kinetic energy implies an absolute temperature floor at 0 K.

Be careful with wording: temperature is related to average random kinetic energy, not total internal energy. Two bodies can share the same temperature but have very different total internal energy if their masses, particle counts, or intermolecular potential-energy contributions are different.

Thermal Energy, Internal Energy, and Thermal Equilibrium

When two bodies in contact have different temperatures, energy transfers from the hotter body to the colder body. That transferred energy is thermal energy transfer (often called heat). Internal energy, in contrast, is the microscopic energy already stored in a body: random kinetic energy of particles plus potential energy associated with intermolecular configuration.

Thermal equilibrium is reached when there is no net thermal energy transfer between interacting bodies. In simple contact problems, this corresponds to equal final temperatures. Equilibrium does not require equal internal energies; it requires that the direction-driving temperature difference has vanished.

Why Kelvin Matters in Thermal Physics

T(K)=θ(deg C)+273.15T(\text{K}) = \theta(\text{deg C}) + 273.15

Temperature differences are numerically equal in K and deg C, but absolute thermal laws require Kelvin values.

For calorimetry expressions with ΔT\Delta T, Celsius and Kelvin increments are interchangeable because one degree step is the same size in both scales. But laws with absolute TT itself, such as black-body radiation and kinetic-theory proportionalities, require Kelvin explicitly. Forgetting this conversion can generate impossible answers by factors of hundreds.

Simulation: Particle View of Temperature and Phase

Switch solid-liquid-gas states and change Kelvin temperature to compare spacing, random motion, and energy partition trends.

Thermal Particle Lab

Microstate viewer (60 particles)

Particle spacing and random-motion speed change with phase and temperature.

Energy partition (relative)

Average kinetic (per mol)3928.37 J/mol
Intermolecular potential depth-4.21 a.u.
Internal-energy index15.35 a.u.

Speed distribution sketch

Shift right and flatten as temperature increases.speed

Mean molecule kinetic

6.524e-21 J

RMS speed index

11.71

Compressibility index

0.20

Phase

LIQUID

Use this model to connect the microscopic picture (particle spacing and random motion) with macroscopic language (temperature, compressibility, and internal energy trends).

Interpretation guidance: hold temperature fixed and switch only phase first. You should see spacing and potential-energy depth change strongly while kinetic trend changes less dramatically. Then hold phase fixed and raise temperature; kinetic contributions rise, distribution shifts toward higher speeds, and compressibility trends become easier to explain microscopically.

Test Yourself

Two samples are both at 300 K. Sample A has ten times the mass of sample B. Which statement is best?

Hint: Separate average particle energy from total energy stored by the whole sample.